JPH0773433A - Magnetic recording medium, its production and magnetic recorder - Google Patents

Magnetic recording medium, its production and magnetic recorder

Info

Publication number
JPH0773433A
JPH0773433A JP5221227A JP22122793A JPH0773433A JP H0773433 A JPH0773433 A JP H0773433A JP 5221227 A JP5221227 A JP 5221227A JP 22122793 A JP22122793 A JP 22122793A JP H0773433 A JPH0773433 A JP H0773433A
Authority
JP
Japan
Prior art keywords
magnetic
film
recording medium
magnetic recording
less
Prior art date
Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
Granted
Application number
JP5221227A
Other languages
Japanese (ja)
Other versions
JP3359706B2 (en
Inventor
Akira Ishikawa
石川  晃
Yoshihiro Shiroishi
芳博 城石
Yuzuru Hosoe
譲 細江
Shinan Yaku
四男 屋久
Tomoo Yamamoto
朋生 山本
Kazusukatsu Igarashi
万壽和 五十嵐
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
Hitachi Ltd
Original Assignee
Hitachi Ltd
Priority date (The priority date is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the date listed.)
Filing date
Publication date
Application filed by Hitachi Ltd filed Critical Hitachi Ltd
Priority to JP22122793A priority Critical patent/JP3359706B2/en
Priority to KR1019940017352A priority patent/KR0148842B1/en
Publication of JPH0773433A publication Critical patent/JPH0773433A/en
Priority to KR97047773A priority patent/KR0141381B1/en
Priority to US08/967,346 priority patent/US5815343A/en
Application granted granted Critical
Publication of JP3359706B2 publication Critical patent/JP3359706B2/en
Anticipated expiration legal-status Critical
Expired - Lifetime legal-status Critical Current

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  • Recording Or Reproducing By Magnetic Means (AREA)
  • Manufacturing Of Magnetic Record Carriers (AREA)
  • Magnetic Record Carriers (AREA)
  • Magnetic Heads (AREA)

Abstract

PURPOSE:To provide a magnetic recording medium, its producing method, and a magnetic recorder where low floating of a head and high-density recording are possible. CONSTITUTION:With respect to the magnetic recording medium which is provided with at least a nonmagnetic disk substrate 11 and a magnetic film 14 formed on the nonmagnetic disk substrate 11 directly or with a foundation film 13 of at least one layer between them, the value of a product Brdelta between a residual magnetic flux density Br of the magnetic film 14 measured in the head running direction and an overall film thickness delta of the magnetic film is set to 5Gmum to <80Gmum. Further, the value of an anisotropic magnetic field Hk is set to 7kOe to 20kOe.

Description

【発明の詳細な説明】Detailed Description of the Invention

【0001】[0001]

【産業上の利用分野】本発明は磁気ドラム、磁気テー
プ、磁気ディスク、磁気カード等の磁気記録媒体及び磁
気記録装置に係り、特に高密度磁気記録に好適な薄膜媒
体及びこれを用いた小型大容量磁気記録装置に関する。
BACKGROUND OF THE INVENTION 1. Field of the Invention The present invention relates to a magnetic recording medium such as a magnetic drum, a magnetic tape, a magnetic disk and a magnetic card, and a magnetic recording device, and particularly to a thin film medium suitable for high density magnetic recording and a small and large size using the thin film medium. The present invention relates to a capacitive magnetic recording device.

【0002】[0002]

【従来の技術】近年、電子計算機等の情報処理装置の小
型化・高速化に伴い、磁気ディスク装置その他の外部記
憶装置の大容量化・高速アクセス化に対する要求が高ま
っている。特に、磁気ディスク記録装置は高密度化・高
速化に適した情報記憶装置であり、その需要が一段と強
まりつつある。
2. Description of the Related Art In recent years, as information processing devices such as electronic computers have become smaller and faster, there has been an increasing demand for larger capacity and faster access to magnetic disk devices and other external storage devices. In particular, the magnetic disk recording device is an information storage device suitable for high density and high speed, and its demand is further increasing.

【0003】磁気ディスク装置に用いられる記録媒体と
しては、酸化物磁性体の粉末を基板上に塗布した媒体
と、金属磁性体の薄膜を基板上にスパッタ蒸着した薄膜
媒体が開発されている。この中で薄膜媒体は、塗布型の
媒体に比べて磁気記録層に含まれる磁性体の密度が高い
ため、高密度の記録再生に適している。薄膜媒体の基板
にはAl−Mg合金、化学強化ガラス、有機樹脂、セラ
ミックス等が用いられ、さらに基板表面にはヘッド粘着
防止あるいは磁気特性向上の目的で中心線平均粗さ(以
後、Raと略記する)が2〜10nm程の溝や突起が形
成される。
As a recording medium used in a magnetic disk device, a medium in which powder of an oxide magnetic material is coated on a substrate and a thin film medium in which a thin film of a metal magnetic material is sputter-deposited on a substrate have been developed. Among them, the thin film medium is suitable for high-density recording / reproduction because the magnetic substance contained in the magnetic recording layer has a higher density than the coating type medium. Al-Mg alloy, chemically strengthened glass, organic resin, ceramics, etc. are used for the substrate of the thin film medium, and the center line average roughness (hereinafter abbreviated as Ra) is used on the substrate surface for the purpose of preventing head adhesion or improving magnetic characteristics. Groove) or protrusion having a thickness of 2 to 10 nm is formed.

【0004】また、磁気ヘッドの再生部に巨大磁気抵抗
効果型(以後、GMRと略記する)素子を用いることに
より、ヘッドの再生感度を従来の誘導型磁気ヘッドに比
べて向上した記録再生分離型ヘッド(以後、GMRヘッ
ドと略記する)が開発されている。GMRヘッドを用い
れば記録ビットの面積が小さくても充分な信号S/Nが
得られるので、媒体の記録密度を飛躍的に向上すること
ができる。
Further, by using a giant magnetoresistive effect type element (hereinafter abbreviated as GMR) in the reproducing portion of the magnetic head, the reproducing sensitivity of the head is improved as compared with the conventional induction type magnetic head. A head (hereinafter abbreviated as GMR head) has been developed. If a GMR head is used, a sufficient signal S / N can be obtained even if the recording bit area is small, so that the recording density of the medium can be dramatically improved.

【0005】磁性膜には主に、飽和磁束密度(Bs)の
高いCo合金スパッタ膜が用いられる。Co合金は六方
最密充填型(hexagonal close packed;hcp)の結晶
構造を有し、磁化容易軸は結晶のc軸である。従って、
面内記録方式ではc軸が基板面と平行となるよう結晶を
配向成長させる必要がある。このため、下地膜として体
心立方構造(body centered cubic :bcc)のCr、
あるいはCr−Ti、Cr−V等の合金膜を用い、この
上にCo合金薄膜をエピタキシャル成長させる技術が用
いられる。
A Co alloy sputtered film having a high saturation magnetic flux density (Bs) is mainly used for the magnetic film. Co alloy has a hexagonal close packed (hcp) crystal structure, and the easy axis of magnetization is the c-axis of the crystal. Therefore,
In the in-plane recording method, it is necessary to orient and grow the crystal so that the c axis is parallel to the substrate surface. Therefore, Cr having a body centered cubic (bcc) structure,
Alternatively, a technique of using an alloy film of Cr-Ti, Cr-V or the like and epitaxially growing a Co alloy thin film on the alloy film is used.

【0006】従来の磁性膜の磁気特性は、例えば、雑誌
「アイ・イー・イー・イー トランサクション オン マ
グネティクス」第29巻(1993年)、307頁に記
載されるように、ヘッド走行方向に測定した磁性膜の残
留磁化量(以後、Brと略記する)と磁性膜の総膜厚
(δ)の積(Brδ)は80〜180Gμm程度、ヘッ
ド走行方向に測定した保磁力(Hc)は1600〜21
00Oe程度である。
The magnetic characteristics of the conventional magnetic film are measured in the head traveling direction as described in, for example, the magazine "EEE Transaction on Magnetics" Vol. 29 (1993), p. 307. The product (Brδ) of the measured residual magnetization of the magnetic film (hereinafter abbreviated as Br) and the total film thickness (δ) of the magnetic film is about 80 to 180 Gμm, and the coercive force (Hc) measured in the head traveling direction is 1600. ~ 21
It is about 00 Oe.

【0007】また、雑誌「アイ・イー・イー・イー ト
ランサクション オン マグネティクス」第29巻(19
93年)、292頁には、透過電子顕微鏡により磁性膜
の結晶格子を観察することにより、結晶粒界、c軸の配
向性、面心立方格子型(facecentered cubic :fc
c)結晶構造を有する異相の存在、及び積層欠陥の密度
等を解析した結果が記載されている。
Also, the magazine "I-E-E-Transaction on Magnetics" Vol. 29 (19
1993, p. 292, by observing the crystal lattice of the magnetic film with a transmission electron microscope, the crystal grain boundaries, the orientation of the c-axis, the face centered cubic (fc)
c) The results of analysis of the presence of a different phase having a crystal structure, the density of stacking faults, and the like are described.

【0008】[0008]

【発明が解決しようとする課題】今後、記録密度をさら
に向上するには、再生感度の高いGMRヘッドの開発、
及びGMRヘッドに適応した磁気特性を有し、かつヘッ
ドの浮上量を低減すべく表面を従来より平滑化した記録
媒体の開発が必須である。従来技術による記録媒体とG
MRヘッドを用いて記録再生実験を行ったところ、Br
δが80Gμm以上あり、GMRヘッドで再生すると出
力とともにノイズが大幅に増加し、高いS/Nを得るこ
とができなかった。また、Brδが大きい場合にGMR
ヘッドの出力が飽和し、再生信号波形が正側と負側で非
対称となり、信号の弁別が困難になる問題があった。ま
た、媒体のBrδが大きいとGMR膜の磁化が過度に回
転して不安定化するため、ヘッドよりバルクハウゼンノ
イズが発生して記録ビットエラーを発生する問題があっ
た。
In order to further improve the recording density in the future, development of a GMR head having high reproduction sensitivity,
Also, it is essential to develop a recording medium having magnetic characteristics adapted to a GMR head and having a smoother surface than before in order to reduce the flying height of the head. Conventional recording medium and G
When a recording / reproducing experiment was performed using an MR head, Br
δ was 80 Gμm or more, and when reproduced with a GMR head, noise increased significantly with output, and high S / N could not be obtained. Also, when Brδ is large, GMR
There is a problem that the output of the head is saturated and the reproduced signal waveform becomes asymmetric between the positive side and the negative side, which makes it difficult to discriminate the signals. Further, when the Br δ of the medium is large, the magnetization of the GMR film excessively rotates and becomes unstable, which causes a problem that Barkhausen noise occurs from the head and a recording bit error occurs.

【0009】このような問題を解決するには媒体のBr
δを80Gμm未満に低減することが有効である。その
ためには、磁性膜の膜厚δ、あるいは残留磁束密度Br
を減少する必要がある。ところが、いずれの方法によっ
てもBrδを上記値とすると、媒体の保磁力Hcが従来
の媒体に比べ著しく低下し、1000Oe未満となっ
た。このようにHcが低下すると、線記録密度が100
kBPI以上と高記録密度の領域ではヘッド出力が著し
く低下するため、エラーを発生するという問題があっ
た。
To solve such a problem, Br of the medium is used.
It is effective to reduce δ to less than 80 Gμm. For that purpose, the thickness δ of the magnetic film or the residual magnetic flux density Br
Need to be reduced. However, when Brδ was set to the above value by any method, the coercive force Hc of the medium was significantly lower than that of the conventional medium and was less than 1000 Oe. When Hc decreases in this way, the linear recording density becomes 100.
In a high recording density region of kBPI or higher, the head output is remarkably reduced, which causes a problem that an error occurs.

【0010】また、上記従来技術による媒体では、媒体
ノイズの低減には磁性膜の粒子間相互作用の低下が有効
との考えから、磁性膜結晶粒の孤立化の手法が提案され
てきた。しかし、この方法では保磁力角形比(S* )の
低下に伴う高記録密度での出力低下や、磁性膜の耐食性
が低下する問題があった。また、媒体からの磁束を有効
にGMRヘッドで検出するためには、ヘッドの浮上量を
0.1μm以下とする必要がある。しかし、従来の媒体
ではヘッド粘着防止あるいは磁気特性向上の目的で、基
板表面にRaが2nm以上のテクスチャーが形成されて
おり、浮上量を下げるとテクスチャーの突起部とヘッド
が接触しやすく、浮上量を0.1μm以下に低減できな
いという問題がある。従って、ヘッドが安定に浮上でき
るように、従来より表面が平滑な媒体を形成する必要が
ある。
Further, in the above-mentioned medium according to the prior art, a method of isolating magnetic film crystal grains has been proposed because it is considered that the reduction of the inter-particle interaction of the magnetic film is effective for reducing the medium noise. However, this method has a problem that the output at a high recording density is reduced due to the decrease in the coercive force squareness ratio (S * ) and the corrosion resistance of the magnetic film is reduced. Further, in order for the magnetic flux from the medium to be effectively detected by the GMR head, the flying height of the head needs to be 0.1 μm or less. However, in the conventional medium, a texture with Ra of 2 nm or more is formed on the substrate surface for the purpose of preventing head sticking or improving magnetic characteristics. When the flying height is reduced, the protrusions of the texture easily come into contact with the head, and the flying height increases. Is not reduced to 0.1 μm or less. Therefore, it is necessary to form a medium having a smoother surface than in the past so that the head can fly stably.

【0011】以上の課題及び状況を鑑み、本発明の第1
の目的は、再生感度の高いGMRヘッドに適応した、高
S/Nが得られる記録媒体を提供することである。すな
わち、GMRヘッドの浮上量0.1μm以下において線
記録密度150kBPI以上、トラック密度10kTP
I以上での記録再生(面記録密度で1.5GMb/in
2 以上に対応)時のS/Nの値が1以上の磁気記録媒体
を提供することである。本発明の第2の目的はこのよう
な媒体を再現性良く製造する方法を提供することであ
り、第3の目的は、このような媒体を用いた大容量で信
頼性の高い磁気記録装置を提供することである。
In view of the above problems and circumstances, the first aspect of the present invention
It is an object of the present invention to provide a recording medium adapted to a GMR head having high reproduction sensitivity and capable of obtaining high S / N. That is, when the flying height of the GMR head is 0.1 μm or less, the linear recording density is 150 kBPI or more and the track density is 10 kTP.
Recording / reproduction at I or higher (1.5 GMb / in in areal recording density)
It is to provide a magnetic recording medium having an S / N value of 1 or more (corresponding to 2 or more). A second object of the present invention is to provide a method of manufacturing such a medium with good reproducibility, and a third object of the present invention is to provide a large-capacity and highly reliable magnetic recording apparatus using such a medium. Is to provide.

【0012】[0012]

【課題を解決するための手段】GMRヘッドを用いる場
合には、媒体としてヘッドの走行方向に測定した磁性膜
の残留磁化量と磁性膜の総膜厚の積(Brδ)を減少
し、かつ、磁性膜の異方性磁界(Hk)を増加すること
により、磁化遷移部の反磁界の影響を低減することが重
要である。
When a GMR head is used, the product (Brδ) of the residual film thickness of the magnetic film and the total film thickness of the magnetic film measured in the running direction of the head as a medium is reduced, and It is important to reduce the influence of the demagnetizing field of the magnetization transition portion by increasing the anisotropic magnetic field (Hk) of the magnetic film.

【0013】本発明者らは媒体の磁気特性と、GMRヘ
ッドによる記録再生特性について鋭意研究を重ねた結
果、上記目的を達成するためには、媒体の磁性膜のヘッ
ド走行方向に測定した残留磁化Brと磁性膜総膜厚δと
の積Brδを5Gμm以上、80Gμm未満とし、か
つ、上記媒体の異方性磁界Hkの値が7kOe以上、2
0kOe以下とすることが有効であることを見出した。
特に、150kBPI以上の線記録密度において媒体ノ
イズをさらに低減し、S/Nを向上するためには、上記
Brδの値を5Gμm以上、30Gμm以下とすること
が好ましい。
As a result of intensive studies on the magnetic characteristics of the medium and the recording / reproducing characteristics of the GMR head, the present inventors have found that, in order to achieve the above object, the residual magnetization of the magnetic film of the medium measured in the head traveling direction. The product Brδ of Br and the total magnetic film thickness δ is set to 5 Gm or more and less than 80 Gm and the anisotropic magnetic field Hk of the medium is 7 kOe or more, 2
It has been found that it is effective to set it to 0 kOe or less.
In particular, in order to further reduce the medium noise and improve the S / N at a linear recording density of 150 kBPI or more, the value of Brδ is preferably 5 Gm or more and 30 Gm or less.

【0014】上記Hkの値はトルクメーターを用いて以
下に述べる方法により測定することができる。すなわ
ち、磁性膜試料の基板面内に磁界を印加しながら、試料
を基板面で360度往復回転し、得られたトルク曲線の
内側の面積を求める。この面積は回転履歴損失Wrと呼
ばれる。このWrを印加磁界の逆数に対してプロット
し、高磁界側でWrが0となる磁界がHkである。
The value of Hk can be measured by the method described below using a torque meter. That is, while applying a magnetic field to the substrate surface of the magnetic film sample, the sample is reciprocally rotated 360 degrees on the substrate surface, and the area inside the obtained torque curve is obtained. This area is called a rotation history loss Wr. This Wr is plotted against the reciprocal of the applied magnetic field, and the magnetic field at which Wr becomes 0 on the high magnetic field side is Hk.

【0015】上記磁気記録媒体において、総磁性膜厚δ
を5nm、30nm以下とし、保磁力を1000Oe以
上、3500Oe以下とすると、磁化遷移領域の磁化の
乱れが低減して磁化遷移領域の幅が減少し、高記録密度
領域においても高い出力が得られる。磁性膜結晶の粒界
の幅が0.5nm以上、5nm以下であるとHcが向上
し、ノイズが低減する。
In the above magnetic recording medium, the total magnetic film thickness δ
When the coercive force is 5 nm or more and 30 nm or less and the coercive force is 1000 Oe or more and 3500 Oe or less, the disorder of the magnetization in the magnetization transition region is reduced, the width of the magnetization transition region is reduced, and high output can be obtained even in the high recording density region. When the width of the grain boundary of the magnetic film crystal is 0.5 nm or more and 5 nm or less, Hc is improved and noise is reduced.

【0016】上記磁気記録媒体において、磁性膜が六方
晶型の結晶構造を有し、そのc軸が実質的に基板面内方
向に配向しており、さらに、六方晶型の格子定数のa及
びcの長さの比c/aの値を1.3以上、1.6以下と
すると異方性磁界が向上する。ここで、c及びaの値は
磁性膜のX線回折分析法、電子線回折分析法、又は透過
電子顕微鏡観察法により求められ、X線回折分析におい
ては必要に応じて試料面を入射X線に対して傾斜させる
ことが必要である。
In the above magnetic recording medium, the magnetic film has a hexagonal crystal structure, the c-axis thereof is substantially oriented in the in-plane direction of the substrate, and the hexagonal lattice constants a and When the ratio of the length of c, c / a, is 1.3 or more and 1.6 or less, the anisotropic magnetic field is improved. Here, the values of c and a are obtained by an X-ray diffraction analysis method, an electron beam diffraction analysis method, or a transmission electron microscope observation method of the magnetic film. In the X-ray diffraction analysis, the incident X-ray may be incident on the sample surface as necessary. It is necessary to tilt with respect to.

【0017】上記磁気記録媒体において、六方晶構造を
有する磁性膜結晶中の面心立方格子(fcc)を形成す
る積層欠陥の密度を5%以下とすると異方性磁界が向上
する。上記磁性膜の結晶粒界の幅、あるいは積層欠陥の
密度は高分解能の透過電子顕微鏡により100個程度の
磁性膜結晶粒の格子像を直接観察し、平均化することに
より求めることができる。
In the above magnetic recording medium, if the density of stacking faults forming face-centered cubic lattice (fcc) in the magnetic film crystal having a hexagonal crystal structure is set to 5% or less, the anisotropic magnetic field is improved. The width of the crystal grain boundary of the magnetic film or the density of stacking faults can be obtained by directly observing and averaging the lattice images of about 100 magnetic film crystal grains with a high resolution transmission electron microscope.

【0018】上記磁気記録媒体において、磁性膜中の酸
素、炭素、窒素の合計濃度を1原子%以下とすると異方
性磁界がより向上する。ここで、磁性膜中の酸素、炭
素、窒素の合計濃度は蛍光X線分析法や、Csイオンと
の分析元素とのクラスターイオンを用いた二次イオン質
量分析法により求めることができる。本明細書で示した
磁気記録媒体の作製に当たっては、成膜真空槽の排気速
度や膜の成長速度を増したり、非磁性下地膜及び磁性膜
形成時に、基板に負のバイアス電圧を10V以上、50
0V以下印加すると、膜の結晶性が向上し、異方性磁界
が向上する。交流バイアスでも直流成分を含んでいれば
同様の効果が得られる。
In the above magnetic recording medium, when the total concentration of oxygen, carbon and nitrogen in the magnetic film is 1 atomic% or less, the anisotropic magnetic field is further improved. Here, the total concentration of oxygen, carbon, and nitrogen in the magnetic film can be obtained by a fluorescent X-ray analysis method or a secondary ion mass spectrometry method using cluster ions of Cs ions and analysis elements. In manufacturing the magnetic recording medium described in this specification, the evacuation rate of the film forming vacuum chamber and the film growth rate are increased, and a negative bias voltage of 10 V or more is applied to the substrate during formation of the nonmagnetic underlayer film and the magnetic film. Fifty
When 0 V or less is applied, the crystallinity of the film is improved and the anisotropic magnetic field is improved. The same effect can be obtained even if an AC bias contains a DC component.

【0019】上記バイアス電圧の印加や、イオン打ち込
み法などにより、磁性膜及び下地膜中に、Ar、Xe、
Krの少なくとも一つの元素を0.1%以上、5%以下
の原子濃度で存在せしめると、膜面内に圧縮応力が増し
て異方性磁界や保磁力が向上する。特に原子半径の大き
いXeあるいはKrを混入すると、膜面内の圧縮応力を
大幅に向上でき、異方性磁界や保磁力を向上できる。
By applying the above bias voltage, the ion implantation method, etc., Ar, Xe,
When at least one element of Kr is made to exist at an atomic concentration of 0.1% or more and 5% or less, compressive stress increases in the film surface and the anisotropic magnetic field and coercive force improve. In particular, when Xe or Kr having a large atomic radius is mixed, the compressive stress in the film surface can be significantly improved, and the anisotropic magnetic field and the coercive force can be improved.

【0020】また、上記磁気記録媒体において、磁性膜
がCoを主たる成分とし、これにNi、Cr、Mo、
W、Zr、Ta、Nb、Al、Si、Pt、B、あるい
はPのいずれか少なくとも1種の元素を添加すると、高
いHcが得られる。特に、磁性膜がCoを主たる成分と
し、Crを磁性膜中に15原子%以上、22原子%以下
の濃度で添加すると、媒体のノイズが著しく低減する。
In the above magnetic recording medium, the magnetic film contains Co as a main component, and Ni, Cr, Mo,
High Hc is obtained by adding at least one element selected from the group consisting of W, Zr, Ta, Nb, Al, Si, Pt, B, and P. In particular, when the magnetic film has Co as a main component and Cr is added to the magnetic film at a concentration of 15 atom% or more and 22 atom% or less, noise of the medium is significantly reduced.

【0021】媒体成膜時の基板温度を200℃以上、5
00℃以下とすると、磁性膜中の偏析構造が促進されて
Hcが向上する。成膜後に媒体を200℃以上の温度で
熱処理すると偏析などが促進され、さらに保磁力が高
く、またノイズも低くなる。ただし、熱処理温度として
は600℃よりも高くすると粒径が肥大化し、ノイズが
増加するので、熱処理は600℃以下で行うことが望ま
しい。
The substrate temperature during film formation is 200 ° C. or higher, 5
When the temperature is 00 ° C. or less, the segregation structure in the magnetic film is promoted and Hc is improved. When the medium is heat-treated at a temperature of 200 ° C. or higher after film formation, segregation is promoted, coercive force is increased, and noise is reduced. However, if the heat treatment temperature is higher than 600 ° C., the grain size becomes large and noise increases, so it is desirable to perform the heat treatment at 600 ° C. or lower.

【0022】Cr、Mo、W、V、Ta、Nb、Zr、
Ti、B、Be、C、Ni−P、Ni−Bの少なくとも
一つを主たる成分とする膜厚0.5nm以上、5nm以
下の非磁性中間層により、磁性膜を2層以上に多層化す
ると媒体ノイズが著しく低減する。磁性膜表面のヘッド
走行方向と垂直の方向に測定した中心線平均粗さRaを
0.3nm以上、1.9nm以下とすると、ヘッド浮上
量が0.1μm以下でも安定に浮上できる。また、上記
磁気記録媒体が磁性膜上に保護膜を有し、保護膜表面の
ヘッド走行方向と垂直の方向に測定した中心線平均粗さ
Raを0.3nm以上、3nm以下とすると、ヘッド浮
上量が0.1μm以下でも安定に浮上できる。
Cr, Mo, W, V, Ta, Nb, Zr,
When the magnetic film is multi-layered into two or more layers by a non-magnetic intermediate layer having a film thickness of 0.5 nm or more and 5 nm or less containing at least one of Ti, B, Be, C, Ni-P, and Ni-B as a main component. Media noise is significantly reduced. When the center line average roughness Ra measured in the direction perpendicular to the head running direction on the surface of the magnetic film is 0.3 nm or more and 1.9 nm or less, stable flying can be achieved even if the head flying height is 0.1 μm or less. Further, when the magnetic recording medium has a protective film on the magnetic film and the center line average roughness Ra measured in the direction perpendicular to the head running direction on the surface of the protective film is 0.3 nm or more and 3 nm or less, the head flying height increases. Even if the amount is 0.1 μm or less, it is possible to stably float.

【0023】非磁性ディスク基板と磁性膜との間にC
r、Mo、W、Nb、あるいはTaを主たる成分とし、
Ti、Pt、Pd、Si、Fe、V、Ru、P、Bのい
ずれか少なくとも1種の元素を添加した合金下地膜を磁
性膜に隣接して形成し、その膜厚を5nm以上、500
nm以下とすると磁性層の配向性が向上し異方性磁界が
向上するとともに、媒体ノイズが低下する。さらに、前
記下地層を少なくとも2層の非磁性層で構成し、基板側
下地層をZr、Si、Ti、Sc、Al、C、Ge、S
b、Ga、Ru、Pd、V、Nb、Ta、Hf、Rh、
Ni−P、Ni−Bもしくはこれらを主たる成分とする
合金とすると、化学強化ガラス、有機樹脂、Ti、S
i、カーボン、あるいはTiO2 、SiC等のセラミッ
ク材料からなる基板を用いたときでも異方性磁界が向上
するとともに、高いBrや保磁力が得られる。
C is provided between the non-magnetic disk substrate and the magnetic film.
r, Mo, W, Nb, or Ta as the main component,
An alloy underlayer film containing at least one element selected from Ti, Pt, Pd, Si, Fe, V, Ru, P, and B is formed adjacent to the magnetic film, and the film thickness is 5 nm or more and 500.
When the thickness is less than or equal to nm, the orientation of the magnetic layer is improved, the anisotropic magnetic field is improved, and the medium noise is reduced. Further, the underlayer is composed of at least two nonmagnetic layers, and the substrate-side underlayer is Zr, Si, Ti, Sc, Al, C, Ge, S.
b, Ga, Ru, Pd, V, Nb, Ta, Hf, Rh,
Ni-P, Ni-B, or alloys containing these as the main components, chemically strengthened glass, organic resin, Ti, S
Even when a substrate made of i, carbon, or a ceramic material such as TiO 2 or SiC is used, the anisotropic magnetic field is improved and high Br and coercive force are obtained.

【0024】磁性層としてはCo、Fe、Niもしくは
これらを主たる成分とする合金が望ましく、特にCo−
Ni、Co−Cr、Co−Fe、Co−Mo、Co−
W、Co−Re等の合金を主たる成分とし、六方晶結晶
構造の(110)結晶格子面が基板と略平行となるよう
結晶を配向成長させるとHcが向上するので望ましい。
また、優れた耐食性を求める場合には磁性膜を構成する
磁性体としてCo−Ni−Zr、Co−Cr−Ta、C
o−Ni−Cr、Co−Cr−Ptを主たる成分とする
合金を用いることが望ましい。
For the magnetic layer, Co, Fe, Ni or an alloy containing these as the main components is desirable.
Ni, Co-Cr, Co-Fe, Co-Mo, Co-
It is preferable to use an alloy such as W or Co-Re as a main component, and to orient the crystal so that the (110) crystal lattice plane of the hexagonal crystal structure is substantially parallel to the substrate because Hc is improved.
In addition, when excellent corrosion resistance is required, Co-Ni-Zr, Co-Cr-Ta, C is used as a magnetic material forming the magnetic film.
It is desirable to use an alloy containing o-Ni-Cr and Co-Cr-Pt as main components.

【0025】磁性膜の保護層としてカーボン、水素添加
カーボン、もしくはカーボンを主たる成分とする非磁性
材料を膜厚10〜50nm形成し、さらに吸着性のパー
フルオロアルキルポリエーテル等の潤滑層を膜厚3〜2
0nm設けることにより信頼性が高く、高密度記録が可
能な磁気記録媒体が得られる。保護層にはWC、(W−
Mo)−C等の炭化物、(Zr−Nb)−N、Si3
4 等の窒化物、SiO2 、ZrO2 等の酸化物、あるい
はB、B4C、MoS2 、Rh等を用いると耐摺動性、
耐食性を向上できるので好ましい。これらの保護膜はマ
スクを用いて表面をエッチングし、面積比で1〜20%
の突起を設けるか、成膜条件、組成等を調整し、異相突
起を析出せしめることで、保護膜が磁性膜表面に比べて
大きな面粗さを有することがより好ましい。
Carbon as a protective layer for the magnetic film, hydrogenation
Carbon or non-magnetic with carbon as the main component
Form a material with a film thickness of 10 to 50 nm and
A lubrication layer such as fluoroalkyl polyether has a thickness of 3 to 2
High reliability by setting 0 nm and high density recording possible
An effective magnetic recording medium can be obtained. WC, (W-
Mo) -C and other carbides, (Zr-Nb) -N, Si3N
FourNitride such as SiO2 , ZrO2Oxides, etc.
Is B, BFourC, MoS2, Rh, etc.
It is preferable because the corrosion resistance can be improved. These protective films are
1 to 20% in area ratio by etching the surface using a disc
Projections or adjust film formation conditions, composition, etc.
The protective film allows the protective film to be
It is more preferable to have a large surface roughness.

【0026】また、媒体表面のRaを従来より小さい値
とした場合に、CSS動作時のヘッドの粘着を抑制する
には、磁性膜上に保護膜を形成した後に微細マスクを用
いてプラズマエッチングすることで表面に高さ20nm
以下の微細な凹凸を形成したり、化合物、混合物のター
ゲットを用いて保護膜表面に微細な突起が生じるように
形成したり、あるいは熱処理によって表面に微細な凹凸
を形成すると、CSS動作時にヘッドと媒体の摩擦力が
低減でき、ヘッドが媒体に粘着する問題が回避される。
When the Ra on the surface of the medium is set to a value smaller than the conventional value, in order to suppress the adhesion of the head during CSS operation, plasma protection is performed using a fine mask after forming a protective film on the magnetic film. 20nm height on the surface
When the following fine irregularities are formed, or when fine protrusions are formed on the surface of the protective film by using a target of a compound or mixture, or when fine irregularities are formed on the surface by heat treatment, the head and The frictional force of the medium can be reduced, and the problem of the head sticking to the medium is avoided.

【0027】本磁気記録媒体とトラック幅が2μm以下
のGMRヘッドとを組合せることにより、大容量で高信
頼性の磁気記録装置を提供することができる。また、最
尤復号法による信号処理回路とを組み合わせるとさらに
記録密度を向上することができる。
By combining this magnetic recording medium with a GMR head having a track width of 2 μm or less, it is possible to provide a magnetic recording device having a large capacity and high reliability. Further, by combining with a signal processing circuit based on the maximum likelihood decoding method, the recording density can be further improved.

【0028】[0028]

【作用】媒体の残留磁化Brと膜厚δの積Brδが過度
に大きいとGMR膜の磁化回転が不安定となり、ヘッド
よりバルクハウゼンノイズが発生する。また、Brδが
増すと記録ビットの遷移領域において反磁界Hdが増し
て磁化の揺らぎが大きくなるため、再生感度が高いGM
Rヘッドを用いた場合に媒体ノイズNdが著しく大きく
なる。また、GMRヘッドは再生感度が高いためBrδ
が80Gμm以上では再生出力が飽和して出力信号の波
形が非対称となる。一方、Brδが5Gμm未満では再
生出力が小さく、媒体ノイズの大きさと同程度となるた
め高い信号S/Nが得られない。従って、使用するGM
Rヘッドの再生感度に適合して媒体のBrδを5Gμm
以上、80Gμm未満の範囲に制御することで高いS/
Nを得ることができる。
If the product Brδ of the residual magnetization Br of the medium and the film thickness δ is excessively large, the magnetization rotation of the GMR film becomes unstable, and Barkhausen noise is generated from the head. Further, as Brδ increases, the diamagnetic field Hd increases in the transition region of the recording bit and the fluctuation of the magnetization increases, so that the GM having high reproduction sensitivity.
When the R head is used, the medium noise Nd becomes extremely large. Further, since the GMR head has high reproduction sensitivity, Brδ
Is 80 Gμm or more, the reproduction output is saturated and the waveform of the output signal becomes asymmetric. On the other hand, when Br δ is less than 5 Gμm, the reproduction output is small and the magnitude of the medium noise is about the same, so that a high signal S / N cannot be obtained. Therefore, the GM to use
Brδ of the medium is 5 Gμm in conformity with the reproducing sensitivity of the R head.
As described above, high S / is achieved by controlling in the range of less than 80 Gμm.
N can be obtained.

【0029】Brδを5Gμm以上、30Gμm以下の
範囲に制御することにより記録ビットにおける磁化の揺
らぎを低減することができ、150kBPI以上の高い
線記録密度で媒体ノイズを著しく低減することができ
る。また、150kBPI以上の高い線記録密度では記
録ビットの長さが短くなり、磁化遷移部のジグザグした
形状がビット長さと同程度となる。また、磁化遷移部間
の相互作用も現われ、記録ビットの形状は従来の低記録
密度時のような理想的な長方形ではなく、不規則な形状
となりやすい。このような場合にも高い出力を得るため
には媒体の磁性膜の異方性磁界Hkの値を7kOe以
上、20kOeと従来より高くし、磁化遷移部の反磁界
の影響を低減することが有効である。
By controlling Brδ in the range of 5 Gμm or more and 30 Gμm or less, the fluctuation of the magnetization in the recording bit can be reduced, and the medium noise can be remarkably reduced at the high linear recording density of 150 kBPI or more. Further, at a high linear recording density of 150 kBPI or more, the length of the recording bit becomes short, and the zigzag shape of the magnetization transition portion becomes approximately the same as the bit length. Further, the interaction between the magnetization transition portions also appears, and the shape of the recording bit is not an ideal rectangular shape as in the conventional low recording density, but tends to be an irregular shape. Even in such a case, in order to obtain a high output, it is effective to increase the value of the anisotropic magnetic field Hk of the magnetic film of the medium to 7 kOe or more and 20 kOe, which is higher than the conventional value, and reduce the influence of the demagnetizing field of the magnetization transition portion. Is.

【0030】また、Hcを1000Oe以上とするため
にはδを5nm以上、30nm以下の値とする必要があ
る。Hcを1000Oe以上とすると磁化遷移領域の幅
が減少して出力半減記録密度D50が向上するため、高線
記録密度時にも高い出力が得られ、同時に媒体ノイズN
dが減少するため再生信号のS/Nが向上する。また、
Hcを3500Oeよりも高くするとオーバーライト特
性が20dB以下となるので、Hcを3500Oe以下
とすることが好ましい。媒体の総磁性膜厚δを5nm以
下とすると、δが減少するに従い磁性膜の結晶粒径が小
さくなり、磁化の温度ゆらぎの効果等により保磁力Hc
は低下する。磁性膜厚δを30nm以上とすると磁性膜
が垂直方向に磁化しやすくなるためHcが低下するので
好ましくない。
Further, in order to set Hc to 1000 Oe or more, it is necessary to set δ to a value of 5 nm or more and 30 nm or less. When Hc is 1000 Oe or more, the width of the magnetization transition region is reduced and the output half recording density D 50 is improved, so that a high output can be obtained even at a high linear recording density, and at the same time, the medium noise N
Since d is reduced, the S / N ratio of the reproduced signal is improved. Also,
When Hc is higher than 3500 Oe, the overwrite characteristic becomes 20 dB or less, so it is preferable to set Hc to 3500 Oe or less. When the total magnetic film thickness δ of the medium is 5 nm or less, the crystal grain size of the magnetic film becomes smaller as δ decreases, and the coercive force Hc is reduced due to the effect of temperature fluctuation of magnetization.
Will fall. When the magnetic film thickness δ is 30 nm or more, the magnetic film is likely to be magnetized in the perpendicular direction and Hc is lowered, which is not preferable.

【0031】磁性膜結晶の粒界の幅を0.5nm以上、
5nm以下とすると磁気クラスター間の磁気的な相互作
用が低減し、Hcが向上するとともに媒体ノイズが低減
する。六方晶型結晶構造を有する磁性膜のc軸を実質的
に基板面内方向に配向し、さらに、磁性膜結晶に基板面
内方向の圧縮歪を付与し、六方晶型の格子定数のa及び
cの長さの比c/aの値を1.3以上、1.6以下とす
ると、逆磁歪効果によりHkやHcを従来より向上でき
る。
The width of the grain boundary of the magnetic film crystal is 0.5 nm or more,
When the thickness is 5 nm or less, magnetic interaction between magnetic clusters is reduced, Hc is improved, and medium noise is reduced. The c-axis of the magnetic film having a hexagonal crystal structure is oriented substantially in the in-plane direction of the substrate, and compressive strain in the in-plane direction of the magnetic film is imparted to the hexagonal lattice constant a and When the value of the ratio c / a of the lengths of c is 1.3 or more and 1.6 or less, Hk and Hc can be improved by the inverse magnetostrictive effect as compared with the conventional case.

【0032】磁性膜結晶中の面心立方格子を形成する積
層欠陥の密度を5%以下と低減すると、磁気異方性定数
の大きい六方晶型結晶を、磁壁の幅程度の20〜30n
mの均一な大きさに制御できるので、HkやHcが向上
する。磁性膜中の酸素、炭素、窒素の合計濃度を1原子
%以下とすると、磁性膜の六方晶型結晶格子の乱れや欠
陥が低減するため磁気異方性定数が増し、HkやHcが
向上する。
When the density of stacking faults forming the face-centered cubic lattice in the magnetic film crystal is reduced to 5% or less, a hexagonal crystal having a large magnetic anisotropy constant is converted into a magnetic domain wall having a width of 20 to 30 n.
Since H can be controlled to a uniform size, Hk and Hc are improved. When the total concentration of oxygen, carbon, and nitrogen in the magnetic film is 1 atomic% or less, disorder and defects of the hexagonal crystal lattice of the magnetic film are reduced, so that the magnetic anisotropy constant is increased and Hk and Hc are improved. .

【0033】このような高Hk、高Hc磁性膜を形成す
るためには、非磁性下地膜及び磁性膜形成時に、成膜室
の排気速度を増して水蒸気等の不純物ガス濃度を低減
し、成膜速度を増すとともに、基板に実質的に負のバイ
アス電圧を10V以上、500V以下印加することが有
効である。特に、−200V以上の電圧を印加すること
により所望の磁気特性の磁性膜を形成することが可能で
ある。これは、成膜室中の不純物ガス濃度の低減、成膜
速度の増加、バイアス電圧の印加により、基板や下地膜
表面の汚染層除去、酸素や窒素等の不純物の除去、蒸着
粒子の基板表面拡散の促進による結晶格子の欠陥や乱れ
の低減、結晶粒界への非磁性元素の偏析による結晶粒界
の発達によるためである。
In order to form such a high Hk and high Hc magnetic film, at the time of forming the non-magnetic underlayer film and the magnetic film, the evacuation speed of the film forming chamber is increased to reduce the concentration of impurity gas such as water vapor. It is effective to increase the film speed and apply a substantially negative bias voltage of 10 V or more and 500 V or less to the substrate. In particular, it is possible to form a magnetic film having desired magnetic characteristics by applying a voltage of -200V or more. This is because the concentration of the impurity gas in the deposition chamber is reduced, the deposition rate is increased, and the bias voltage is applied to remove the contaminated layer on the surface of the substrate and the underlying film, the removal of impurities such as oxygen and nitrogen, and the substrate surface of vapor deposition particles. This is because defects and disorder of the crystal lattice are reduced by promoting diffusion, and crystal grain boundaries are developed due to segregation of nonmagnetic elements to the crystal grain boundaries.

【0034】また、高Hk、高Hc磁性膜を形成するた
めには、下地膜の結晶格子の大きさを磁性膜の結晶格子
の大きさと整合させ、結晶格子の欠陥や乱れを低減する
ことが重要である。このためには、Cr、Mo、W、N
b、あるいはTaを主たる成分とする下地層に、Ti、
Pt、Pd、Si、Fe、V、Ru、P、Bのいずれか
少なくとも1種の元素を添加することが有効である。ま
た、磁性膜と同様に、下地膜の結晶格子の欠陥や乱れを
低減することも重要であり、そのためには前記下地層を
少なくとも2層の非磁性層で構成し、基板側下地層をZ
r、Si、Ti、Sc、Al、C、Ge、Sb、Ga、
Ru、Pd、V、Nb、Ta、Hf、Rh、Ni−P、
Ni−Bもしくはこれらを主たる成分とする合金とする
ことで、基板材料に起因する結晶配向性の乱れや、不純
物の拡散を抑制できる。
Further, in order to form a high Hk and high Hc magnetic film, the size of the crystal lattice of the underlayer film should be matched with the size of the crystal lattice of the magnetic film to reduce defects and disorder of the crystal lattice. is important. To this end, Cr, Mo, W, N
b or Ta is the main component of the underlying layer, Ti,
It is effective to add at least one element selected from Pt, Pd, Si, Fe, V, Ru, P, and B. Further, like the magnetic film, it is important to reduce defects and disorder of the crystal lattice of the underlayer. For that purpose, the underlayer is composed of at least two non-magnetic layers, and the substrate-side underlayer is made of Z.
r, Si, Ti, Sc, Al, C, Ge, Sb, Ga,
Ru, Pd, V, Nb, Ta, Hf, Rh, Ni-P,
By using Ni-B or an alloy containing these as the main components, the disorder of the crystal orientation due to the substrate material and the diffusion of impurities can be suppressed.

【0035】また、媒体からの磁束を有効にGMRヘッ
ドで検出するためには、ヘッドの浮上量を減少すること
が有効である。ここで、ヘッド走行方向と垂直の方向に
測定した媒体保護膜表面の中心線平均粗さRaを0.3
nm以上、3nm以下とすると浮上量が0.1μm以下
でもヘッドが安定に浮上する。また、磁性膜表面の、ヘ
ッド走行方向と垂直の方向に測定した中心線平均粗さR
aを0.3nm以上、1.9nm以下とすると浮上量が
0.1μm以下においてもヘッドが安定に浮上する。
In order to effectively detect the magnetic flux from the medium with the GMR head, it is effective to reduce the flying height of the head. Here, the center line average roughness Ra of the surface of the medium protective film measured in the direction perpendicular to the head traveling direction is 0.3.
When the thickness is not less than 3 nm and not more than 3 nm, the head flies stably even if the flying height is not more than 0.1 μm. Further, the center line average roughness R measured on the surface of the magnetic film in a direction perpendicular to the head traveling direction.
When a is 0.3 nm or more and 1.9 nm or less, the head flies stably even when the flying height is 0.1 μm or less.

【0036】磁性膜上に保護膜を形成した後に微細マス
クを用いてプラズマエッチングすることで表面に高さ2
0nm以下の微細な凹凸を形成したり、化合物、混合物
のターゲットを用いて保護膜表面に微細な突起を生じせ
しめたり、あるいは熱処理によって表面に微細な凹凸を
形成すると、ヘッドと媒体と接触面積、摩擦力が低減す
るため、ヘッドが媒体に粘着する問題が回避されるの
で、上記処理等により保護膜を磁性膜表面と異なる面粗
さを有するようにすることが特に好ましい。本発明によ
る媒体はS/Nが極めて高いため、トラック幅が2μm
以下のGMRヘッドで再生した場合に、トラック密度1
0kTPI以上、150kBPI以上の高い記録密度に
おいてS/Nが1以上の大容量磁気記録装置が得られ
る。
After forming a protective film on the magnetic film, plasma etching is performed using a fine mask to increase the height of the surface to 2
When fine irregularities of 0 nm or less are formed, fine projections are formed on the surface of the protective film by using a target of a compound or mixture, or fine irregularities are formed on the surface by heat treatment, the contact area between the head and the medium, Since the frictional force is reduced and the problem of the head sticking to the medium is avoided, it is particularly preferable to make the protective film have a surface roughness different from that of the magnetic film surface by the above-mentioned treatment or the like. Since the medium according to the present invention has an extremely high S / N, the track width is 2 μm.
Track density of 1 when reproduced with the following GMR head
A high-capacity magnetic recording device having an S / N of 1 or more can be obtained at a high recording density of 0 kTPI or more and 150 kBPI or more.

【0037】[0037]

【実施例】以下、実施例により本発明をさらに詳細に説
明する。図1は、本発明に係る薄膜媒体の断面構造を模
式的に示したものである。同図において、符号11はA
l−Mg合金、化学強化ガラス、有機樹脂、Ti、S
i、カーボン、あるいはTiO2 、SiC等のセラミッ
クス等からなる基板、12及び12’は基板11の両面
に形成したNi−P、Ni−W−P等からなる非磁性メ
ッキ層である。Al−Mg合金を基板として用いた場合
にはこのようなメッキ層を備えたものを基板として用い
ることが好ましいが、その他の基板については12及び
12’はなくてもよい。13及び13’はCr、Mo、
W、V、Ta、Nb、Zr、Ti、B、Be、C、Ni
−P、Ni−Bのいずれかを主な成分とする合金からな
る金属下地膜、14及び14’は当該下地膜の上に形成
したCo−Ni、Co−Cr、Co−Fe、Co−M
o、Co−W、Co−Pt、Co−Re、Co−P、C
o−Ni−Pt、Co−Cr−Ta、Co−Cr−P
t、Co−Ni−Cr、Co−Cr−Al、Co−Cr
−Nb、Co−Ni−P、あるいはCo−Cr−Si等
からなる金属磁性層、15及び15’は当該磁性膜の上
に形成したカーボン、WC、(W−Mo)−C、(W−
Zr)−C、SiC、(Zr−Nb)−N、Si
34 、SiO2 、ZrO2 、ボロン、B4C、Mo
2 、あるいはRh等からなる非磁性保護膜をそれぞれ
示す。
EXAMPLES The present invention will be described in more detail below with reference to examples.
Reveal FIG. 1 shows a cross-sectional structure of a thin film medium according to the present invention.
It is shown as a formula. In the figure, reference numeral 11 is A
1-Mg alloy, chemically strengthened glass, organic resin, Ti, S
i, carbon, or TiO2, SiC, etc.
Substrate 12 and 12 'are both sides of the substrate 11.
Non-magnetic film made of Ni-P, Ni-WP, etc.
It is a layer. When using Al-Mg alloy as the substrate
Used a substrate with such a plating layer as the substrate
However, for other substrates, 12 and
12 'may be omitted. 13 and 13 'are Cr, Mo,
W, V, Ta, Nb, Zr, Ti, B, Be, C, Ni
-P, Ni-B made of an alloy containing as a main component
Metal base film, 14 and 14 'are formed on the base film
Co-Ni, Co-Cr, Co-Fe, Co-M
o, Co-W, Co-Pt, Co-Re, Co-P, C
o-Ni-Pt, Co-Cr-Ta, Co-Cr-P
t, Co-Ni-Cr, Co-Cr-Al, Co-Cr
-Nb, Co-Ni-P, Co-Cr-Si, etc.
And 15 and 15 'are formed on the magnetic film.
Formed on carbon, WC, (W-Mo) -C, (W-
Zr) -C, SiC, (Zr-Nb) -N, Si
3NFour, SiO2, ZrO2, Boron, BFourC, Mo
S 2, Or a non-magnetic protective film made of Rh, etc., respectively.
Show.

【0038】〔実施例1〕外径95mm、内径25m
m、厚さ0.8mmのAl−4Mg(原子記号の前に付
した数字は当該素材の含有量を示す。含有量の単位は重
量%)からなるディスク基板の両面にNi−12P(重
量%)からなるメッキ層を膜厚13μm形成した。この
非磁性基板の表面を、ラッピングマシンを用いて中心線
平均粗さRaが0.3nmとなるまで平滑に研磨し、洗
浄及び乾燥した。その後、テープポリッシングマシンを
用い、平均砥粒径0.5μm以下の研磨剤の存在下で、
研磨テープをコンタクトロールを通してディスク基板1
1を回転させながらディスク面の両側に押しつけること
により、基板表面にヘッド走行方向に深さや密度が不規
則なテクスチャー溝を形成した。さらに、基板に付着し
た研磨剤等の汚れを洗浄して乾燥した。半径方向に測定
した基板表面の溝の中心線平均粗さRaは0.7nm、
ヘッド走行方向と略垂直方向の距離1μmにおける、深
さ1nm以上、50nm以下の溝の平均密度は20本で
あった。
[Example 1] Outer diameter 95 mm, inner diameter 25 m
Ni-12P (wt%) on both sides of a disk substrate made of Al-4Mg with a thickness of 0.8 mm (the number preceding the atomic symbol indicates the content of the material. The unit of the content is wt%). 13 μm in thickness was formed on the plated layer of (1). The surface of this non-magnetic substrate was smooth-polished using a lapping machine until the centerline average roughness Ra became 0.3 nm, washed and dried. Then, using a tape polishing machine, in the presence of an abrasive having an average abrasive grain size of 0.5 μm or less,
Disk substrate 1 with polishing tape through contact roll
By pressing 1 on both sides of the disk surface while rotating, texture grooves having irregular depth and density in the head running direction were formed on the substrate surface. Further, dirt such as abrasives attached to the substrate was washed and dried. The center line average roughness Ra of the groove on the substrate surface measured in the radial direction is 0.7 nm,
The average density of the grooves having a depth of 1 nm or more and 50 nm or less was 20 at a distance of 1 μm in the direction substantially perpendicular to the head traveling direction.

【0039】このディスク基板24をスパッタリング装
置内で、真空槽体積当りの水蒸気の排気速度200l/
s以上の排気ポンプを用いて、2nTorrの真空度に
保持し、基板を250℃に加熱した後0.5mTorr
のアルゴン圧の条件のもとで膜厚50nmのCr下地膜
23を形成した。この下地膜上にCo−17Cr−5T
a(原子%)合金系磁性膜22を膜厚5〜30nm成膜
した。その後、磁性膜上に膜厚20nmの水素含有カー
ボン保護膜21を形成した。さらに、保護膜表面に開口
部のピッチ1μm以上、100μm以下の粒子化マスク
を設置した。その後、マスクに覆われない部分の保護膜
を酸素プラズマエッチングにより深さ1nm以上、20
nm以下エッチングし、保護膜が磁性膜表面と比べて異
なる面粗さを有するようにした。
The disk substrate 24 is placed in a sputtering apparatus and the exhaust rate of water vapor per volume of the vacuum chamber is 200 l /
Using an exhaust pump of s or more, the degree of vacuum is maintained at 2 nTorr, the substrate is heated to 250 ° C., and then 0.5 mTorr.
A Cr underlayer 23 having a film thickness of 50 nm was formed under the conditions of argon pressure. Co-17Cr-5T is formed on this base film.
An a (atomic%) alloy magnetic film 22 was formed to a thickness of 5 to 30 nm. After that, a hydrogen-containing carbon protective film 21 having a film thickness of 20 nm was formed on the magnetic film. Further, a particle-forming mask having an opening pitch of 1 μm or more and 100 μm or less was provided on the surface of the protective film. After that, the portion of the protective film not covered by the mask is etched by oxygen plasma to a depth of 1 nm or more,
The protective film has a surface roughness different from that of the surface of the magnetic film by etching to a thickness of not more than nm.

【0040】その結果、図2に示すように、カーボン保
護膜表面にピッチ1μm以上、100μm以下の凹凸2
5が形成された。当該保護膜上に吸着性のパーフルオロ
アルキルポリエーテル等の潤滑層を形成した。媒体の静
磁気特性(Hc、Br、Hk)を最大印加磁界14kO
eの振動式磁化測定機(VSM)、トルクメーターによ
り測定した。また、記録再生特性を、ヘッド浮上量0.
06μm、実効ギャップ長0.4μm、トラック幅2μ
m、再生部にGMR素子を有する複合型薄膜磁気ヘッド
を用いて線記録密度150kBPIにおいて記録再生S
/Nの値を求めた。
As a result, as shown in FIG. 2, unevenness 2 having a pitch of 1 μm or more and 100 μm or less on the surface of the carbon protective film.
5 was formed. A lubricating layer such as an adsorbent perfluoroalkylpolyether was formed on the protective film. The magnetostatic characteristics (Hc, Br, Hk) of the medium are the maximum applied magnetic field of 14 kO.
The measurement was performed using a vibration type magnetometer (e.g., e.g., e.g., VSM) and a torque meter. In addition, the recording / reproducing characteristic is set to 0.
06μm, effective gap length 0.4μm, track width 2μ
m, recording / reproducing S at a linear recording density of 150 kBPI using a composite type thin film magnetic head having a GMR element in the reproducing section.
The value of / N was determined.

【0041】上記媒体において、磁性膜の膜厚δを制御
することにより、ヘッド走行方向に測定した媒体磁性膜
の残留磁化Brとδとの積Brδの値を5Gμm以上、
79Gμm以下とし、さらに、成膜室の排気速度、下地
膜及び磁性膜の成膜速度、及び成膜時の基板側の直流バ
イアス電圧を−10V〜−500Vの範囲で制御するこ
とにより、Hkを5kOeから30kOeまで変化させ
た媒体を作成した。
In the above medium, by controlling the film thickness δ of the magnetic film, the value Brδ of the residual magnetization Br and δ of the medium magnetic film measured in the head traveling direction is set to 5 Gμm or more,
Hg is controlled to 79 Gμm or less, and further, by controlling the evacuation speed of the film forming chamber, the film forming speed of the underlying film and the magnetic film, and the DC bias voltage on the substrate side during film formation in the range of −10 V to −500 V. A medium in which the pressure was changed from 5 kOe to 30 kOe was prepared.

【0042】図3にHkと記録再生時のS/Nの関係を
示す。Hkが7kOe以上、20kOe以下の範囲でS
/Nを1以上にできることが確認できた。この時のヘッ
ド走行方向に測定した保磁力Hcは1000Oe以上、
3500Oe以下であった。上記方法により形成された
磁気記録媒体をX線回折分析した結果、Cr下地層では
体心立方構造の(200)結晶格子面が基板面と略並行
となるよう結晶が配向成長していることが確認された。
また、磁性層では六方晶構造の(110)面がディスク
基板表面と略並行となり、c軸がディスク基板表面と略
並行となるよう配向していた。また、磁性膜中の酸素、
炭素、窒素の合計濃度は1原子%以下であることが確認
された。
FIG. 3 shows the relationship between Hk and S / N during recording and reproduction. S in the range where Hk is 7 kOe or more and 20 kOe or less
It was confirmed that / N could be 1 or more. At this time, the coercive force Hc measured in the head traveling direction is 1000 Oe or more,
It was 3500 Oe or less. As a result of X-ray diffraction analysis of the magnetic recording medium formed by the above method, it was found that in the Cr underlayer, crystals were oriented and grown so that the (200) crystal lattice plane of the body-centered cubic structure was substantially parallel to the substrate surface. confirmed.
Further, in the magnetic layer, the (110) plane of the hexagonal structure was oriented substantially parallel to the disk substrate surface, and the c-axis was oriented substantially parallel to the disk substrate surface. Also, oxygen in the magnetic film,
It was confirmed that the total concentration of carbon and nitrogen was 1 atomic% or less.

【0043】また、基板のテクスチャー形成時の砥粒径
や加工時間を制御することにより、保護膜表面の半径方
向に測定した中心線平均粗さRaを0.3nm以上、3
nm以下で、磁性膜表面の中心線平均粗さRaを0.3
nm以上、1.9nm以下とした媒体を用いて、浮上量
0.06μmにおいてMRヘッドを媒体内周から外周ま
で10万回シークした結果、ヘッドと媒体の接触は起こ
らないことが確認された。
Further, the center line average roughness Ra measured in the radial direction of the protective film surface is 0.3 nm or more and 3 by controlling the abrasive grain size and the processing time during the texture formation of the substrate.
The center line average roughness Ra of the magnetic film surface is 0.3 nm or less.
As a result of seeking 100,000 times from the inner circumference to the outer circumference of the MR head at a flying height of 0.06 μm using a medium having a thickness of not less than 1.9 nm and not more than 1.9 nm, it was confirmed that the head did not come into contact with the medium.

【0044】以上の効果は磁性材料にCo−10Ni−
10Cr(原子%)、Co−40Ni−5Zr(原子
%)、Co−30Ni−10Pt(原子%)を用いた場
合でも同様に認められた。また、下地膜を形成せずに基
板上に磁性膜を直接形成した場合には、保磁力が下地膜
を形成した場合に比べて100〜200Oe低下した
が、S/Nは1以上であることが確認された。また、磁
性膜を、Cr、Mo、W、V、Ta、Nb、Zr、T
i、B、Be、C、Ni−P、及びNi−Bの一種から
なる、膜厚0.5nm以上、5nm以下の非磁性中間層
により二層化した場合には、媒体ノイズが単層の磁性膜
の約2/3に低下し、S/Nの値はさらに向上した。
The above effect is obtained by applying Co-10Ni- to the magnetic material.
The same was found when 10Cr (atomic%), Co-40Ni-5Zr (atomic%), and Co-30Ni-10Pt (atomic%) were used. Further, when the magnetic film is directly formed on the substrate without forming the base film, the coercive force is reduced by 100 to 200 Oe as compared with the case where the base film is formed, but the S / N is 1 or more. Was confirmed. Further, the magnetic film is formed of Cr, Mo, W, V, Ta, Nb, Zr, T.
When a non-magnetic intermediate layer composed of i, B, Be, C, Ni-P, and Ni-B and having a film thickness of 0.5 nm or more and 5 nm or less is formed into two layers, the medium noise is a single layer. It was reduced to about 2/3 that of the magnetic film, and the S / N value was further improved.

【0045】〔実施例2〕外径65mm、内径20m
m、厚さ0.3mmのカナサイトガラス基板表面を、ラ
ッピングマシンを用いて中心線平均粗さRaが0.3n
mとなるまで平滑に研磨し、洗浄及び乾燥した。このデ
ィスク基板をスパッタリング装置内で、真空槽体積当り
の水蒸気の排気速度400l/s以上の排気ポンプを用
いて真空保持し、基板温度を400℃まで加熱した後、
5mTorrのアルゴン圧の条件のもとで第1層下地膜
としてTiを20nm形成し、次いで第2層下地膜とし
てはCr−15Ti(原子%)合金を膜厚50nm形成
した。この複合下地膜上に膜厚10nmのCo−Cr−
Pt−Si磁性膜を形成した。その際、基板側に13.
56MHzの高周波バイアス電圧を300W印加した。
この時、バイアス電圧の直流成分は−300V、Brδ
の値は25Gμmであった。
[Embodiment 2] Outer diameter 65 mm, inner diameter 20 m
The center line average roughness Ra of the n-sided canasite glass substrate having a thickness of 0.3 mm and a thickness of 0.3 mm was 0.3 n using a lapping machine.
It was smoothly polished until it reached m, washed and dried. This disk substrate was held in vacuum in a sputtering device using an exhaust pump having an exhaust rate of water vapor per volume of a vacuum chamber of 400 l / s or more, and after heating the substrate temperature to 400 ° C.,
Under the conditions of an argon pressure of 5 mTorr, Ti was formed to a thickness of 20 nm as the first underlayer film, and then a Cr-15Ti (atomic%) alloy was formed to a thickness of 50 nm as the second underlayer film. A 10 nm thick Co-Cr- film is formed on the composite underlayer.
A Pt-Si magnetic film was formed. At that time, 13.
A high frequency bias voltage of 56 MHz was applied at 300 W.
At this time, the DC component of the bias voltage is -300 V, Br?
The value of was 25 Gμm.

【0046】磁性膜中のCr、Pt、Siの添加濃度を
5原子%以上、20原子%以下の範囲で制御することに
より、高分解能透過電子顕微鏡により観察される磁性膜
結晶の粒界の幅を、0.1nm以上、10nm以下の範
囲で制御した。この時のBrδの値は5Gμm以上、3
0Gμm以下、Hkの値は7kOe以上、20kOe以
下であった。
By controlling the additive concentration of Cr, Pt, and Si in the magnetic film in the range of 5 atom% or more and 20 atom% or less, the grain boundary width of the magnetic film crystal observed by a high resolution transmission electron microscope. Was controlled in the range of 0.1 nm or more and 10 nm or less. The value of Brδ at this time is 5 Gμm or more, 3
The value of Hk was 0 Gμm or less, and the value of Hk was 7 kOe or more and 20 kOe or less.

【0047】図4に磁性膜結晶の粒界の幅と、保磁力H
c、及びヘッド浮上量0.03μm、線記録密度200
kPBIにおける記録再生S/Nの値の関係を示す。粒
界の幅が0.5nm以上、5nm以下においてHcが1
000Oe以上、3500Oe以下、S/Nが1以上と
なり、良好な特性を示した。本実施例の方法により形成
された磁気記録媒体をX線回折分析した結果、Cr下地
層では体心立方構造の(110)結晶格子面が基板面と
略並行となるよう結晶が配向成長していることが確認さ
れた。また、磁性層では六方晶構造の(100)面がデ
ィスク基板表面と略並行となるよう配向していた。ま
た、保護膜表面の中心線平均粗さRaは1.0nm、磁
性膜表面の中心線平均粗さRaは0.9nmであった。
FIG. 4 shows the width of the grain boundary of the magnetic film crystal and the coercive force H.
c, head flying height 0.03 μm, linear recording density 200
The relationship between the recording / reproducing S / N values in kPBI is shown. Hc is 1 when the width of the grain boundary is 0.5 nm or more and 5 nm or less
000 Oe or more, 3500 Oe or less, and S / N of 1 or more, showing good characteristics. As a result of X-ray diffraction analysis of the magnetic recording medium formed by the method of this example, crystals were oriented and grown in the Cr underlayer so that the (110) crystal lattice plane of the body-centered cubic structure was substantially parallel to the substrate surface. Was confirmed. Moreover, in the magnetic layer, the (100) plane of the hexagonal structure was oriented so as to be substantially parallel to the surface of the disk substrate. The center line average roughness Ra of the protective film surface was 1.0 nm, and the center line average roughness Ra of the magnetic film surface was 0.9 nm.

【0048】本実施例の媒体を用いて、浮上量0.03
μmにおいてGMRヘッドを媒体内周から外周まで10
万回シークした結果、ヘッドと媒体の接触は起こらない
ことが確認された。本効果は第1層下地膜としてZr、
Si、Sc、Al、C、Ge、Sb、Ga、Ru、P
d、V、Nb、Ta、Hf、Rh、Ni−P、Ni−B
もしくはこれらを主たる成分とする合金を用いた場合で
も同様に認められた。
Using the medium of this example, the flying height is 0.03.
At the μm, the GMR head is 10
As a result of 10,000 seeks, it was confirmed that contact between the head and the medium did not occur. This effect is achieved by using Zr as the first underlayer film,
Si, Sc, Al, C, Ge, Sb, Ga, Ru, P
d, V, Nb, Ta, Hf, Rh, Ni-P, Ni-B
Alternatively, it was similarly observed when an alloy containing these as the main components was used.

【0049】〔実施例3〕外径48mm、内径12m
m、厚さ0.3mmのカーボン基板表面を、ラッピング
マシンを用いて中心線平均粗さRaが0.3nmとなる
まで平滑に研磨し、洗浄及び乾燥した。その後、テープ
ポリッシングマシンを用い、平均砥粒径1μm以下のダ
イアモンド研磨剤の存在下で、研磨テープをコンタクト
ロールを通してディスク基板を回転させながらディスク
面の両側に押しつけることにより、基板表面に深さや密
度が不規則なテクスチャー溝を形成した。さらに、基板
に付着した研磨剤等の汚れを洗浄して乾燥した。
[Embodiment 3] Outer diameter 48 mm, inner diameter 12 m
The surface of the carbon substrate having a thickness of 0.3 mm and a thickness of 0.3 mm was smoothly polished using a lapping machine until the center line average roughness Ra was 0.3 nm, washed and dried. After that, using a tape polishing machine, in the presence of a diamond abrasive having an average abrasive grain size of 1 μm or less, the polishing tape is pressed against both sides of the disk surface while rotating the disk substrate through a contact roll, so that the depth and density of the substrate surface are increased. Formed irregular texture grooves. Further, dirt such as abrasives attached to the substrate was washed and dried.

【0050】半径方向に測定した基板表面の溝の中心線
平均粗さRaは0.5nm、ヘッド走行方向と略垂直方
向の距離1μmにおける、深さ1nm以上、50nm以
下の溝の平均密度は50本であった。このディスク基板
をスパッタリング装置内で、真空槽体積当りの水蒸気の
排気速度500l/s以上の排気ポンプを用いて真空保
持し、基板温度を400℃まで加熱した後、1mTor
rのアルゴン圧の条件のもとでCr−15Ti下地膜を
10nm形成した。この下地膜上に膜厚5nmのCo−
Cr−Pt−Ta磁性膜を形成した。この時のBrδの
値は10Gμmであった。
The center line average roughness Ra of the grooves on the substrate surface measured in the radial direction is 0.5 nm, and the average density of the grooves having a depth of 1 nm or more and 50 nm or less at a distance of 1 μm in the direction substantially perpendicular to the head running direction is 50. It was a book. This disk substrate was held in a vacuum in a sputtering apparatus by using an exhaust pump having an evacuation rate of water vapor per vacuum chamber volume of 500 l / s or more, and the substrate temperature was heated to 400 ° C., and then 1 mTorr.
A Cr-15Ti base film was formed to a thickness of 10 nm under the condition of an argon pressure of r. Co-film with a thickness of 5 nm is formed on this base film.
A Cr-Pt-Ta magnetic film was formed. At this time, the value of Brδ was 10 Gμm.

【0051】成膜時の直流バイアス電圧を−10V〜−
500Vの範囲で制御することにより、六方晶型結晶構
造を有する磁性膜の格子定数a及びcの長さの比c/a
の値、及び下地膜及び磁性膜中のAr濃度を変化させ
た。この時のBrδの値は5Gμm以上、30Gμm以
下、Hcは1000Oe以上、3500Oe以下であっ
た。
The DC bias voltage during film formation is from −10V to −
By controlling in the range of 500 V, the ratio of the lattice constants a and c of the magnetic film having the hexagonal crystal structure c and the length ratio c / a
And the Ar concentration in the underlayer film and the magnetic film were changed. At this time, the value of Brδ was 5 Gμm or more and 30 Gμm or less, and Hc was 1000 Oe or more and 3500 Oe or less.

【0052】図5に磁性膜の格子定数比c/aと、H
k、及びヘッド浮上量0.03μm、線記録密度200
kPBIにおける記録再生S/Nの値の関係を示す。格
子定数比c/aが1.3以上、1.6以下において、H
kの値は7kOe以上、20kOe以下となり、S/N
は1以上と良好な特性を示した。また、下地膜及び磁性
膜中のAr濃度が0.01原子%以上、5原子%以下の
時にHkの値は8kOe以上、20kOe以下となり、
S/Nは1.2以上とさらに良好な特性を示した。
FIG. 5 shows the lattice constant ratio c / a of the magnetic film and H
k, head flying height 0.03 μm, linear recording density 200
The relationship between the recording / reproducing S / N values in kPBI is shown. When the lattice constant ratio c / a is 1.3 or more and 1.6 or less, H
The value of k is 7 kOe or more and 20 kOe or less, and S / N
Shows a good characteristic of 1 or more. When the Ar concentration in the underlayer and the magnetic film is 0.01 atomic% or more and 5 atomic% or less, the value of Hk is 8 kOe or more and 20 kOe or less,
The S / N ratio was 1.2 or more, which was a better characteristic.

【0053】本実施例の方法により形成された磁気記録
媒体をX線回折分析した結果、Cr下地層では体心立方
構造の(100)結晶格子面が基板面と略並行となるよ
う結晶が配向成長していることが確認された。また、磁
性層では六方晶構造の(110)面がディスク基板表面
と略並行となるよう配向していた。保護膜表面の中心線
平均粗さRaは1.0nm、磁性膜表面の中心線平均粗
さRaは0.5nmであった。
As a result of X-ray diffraction analysis of the magnetic recording medium formed by the method of this example, the crystals were oriented in the Cr underlayer so that the (100) crystal lattice plane of the body-centered cubic structure was substantially parallel to the substrate surface. It was confirmed that it was growing. Further, in the magnetic layer, the (110) plane of the hexagonal structure was oriented so as to be substantially parallel to the disk substrate surface. The center line average roughness Ra of the protective film surface was 1.0 nm, and the center line average roughness Ra of the magnetic film surface was 0.5 nm.

【0054】本実施例の媒体を用いて、浮上量0.03
μmにおいてGMRヘッドを媒体内周から外周まで10
万回シークした結果、ヘッドと媒体の接触は起こらない
ことが確認された。本効果はCr、Mo、W、Nb、あ
るいはTaを主たる成分とし、Pt、Pd、Si、F
e、V、Ru、P、Bのいずれか少なくとも1種の元素
を1原子%以上、30原子%以下添加した合金下地膜
を、膜厚5nm以上、500nm以下で形成した場合で
も同様に認められた。
Using the medium of this example, the flying height is 0.03.
At the μm, the GMR head is 10
As a result of 10,000 seeks, it was confirmed that contact between the head and the medium did not occur. This effect is mainly composed of Cr, Mo, W, Nb, or Ta, and Pt, Pd, Si, F
Even when an alloy underlayer film in which at least one element selected from e, V, Ru, P, and B is added in an amount of 1 atomic% or more and 30 atomic% or less with a film thickness of 5 nm or more and 500 nm or less is similarly recognized. It was

【0055】〔実施例4〕外径48mm、内径12m
m、厚さ0.3mmのSi−C基板表面を、ラッピング
マシンを用いて中心線平均粗さRaが0.3nmとなる
まで平滑に研磨し、洗浄及び乾燥した。このディスク基
板をスパッタリング装置内で、真空槽体積当りの水蒸気
の排気速度500l/s以上の排気ポンプを用いて真空
保持し、基板温度を100℃〜400℃の範囲で加熱し
た後、1mTorrのXe圧のもとで下地膜としてNi
−Bを50nm形成し、次いでCo−Ni−Pt−Ta
磁性膜を10nm形成した。この時、磁性膜中のPt及
びTaの濃度を1原子%以上、30原子%以下、磁性膜
膜厚を1nm以上、40nm以下の範囲で変化させるこ
とにより、残留磁束密度膜厚積Brδの値を1Gμm以
上、200Gμm以下の範囲で変化せしめた。
[Embodiment 4] Outer diameter 48 mm, inner diameter 12 m
The surface of the Si-C substrate having a thickness of 0.3 mm and a thickness of 0.3 mm was smoothly polished using a lapping machine until the centerline average roughness Ra was 0.3 nm, washed and dried. This disk substrate was held in a vacuum in a sputtering apparatus by using an exhaust pump having an evacuation rate of water vapor per volume of a vacuum chamber of 500 l / s or more, and the substrate temperature was heated in the range of 100 ° C. to 400 ° C., after which Xe of 1 mTorr was applied. Ni underlayer under pressure
-B is formed to a thickness of 50 nm, and then Co-Ni-Pt-Ta is formed.
A magnetic film having a thickness of 10 nm was formed. At this time, the values of the residual magnetic flux density film thickness product Brδ are changed by changing the concentrations of Pt and Ta in the magnetic film within the range of 1 atomic% to 30 atomic% and the magnetic film thickness within the range of 1 nm to 40 nm. Was changed in the range of 1 Gm or more and 200 Gm or less.

【0056】図6にBrδと保磁力Hcの関係を示す。
Brδが5Gμm以上、80Gμm未満の時にHcは1
000Oe以上、3500Oe以下となった。また、ヘ
ッド浮上量0.02μm、線記録密度250kPBIに
おける記録再生S/Nは、Brδが5Gμm以上、80
Gμm未満の時に1以上となり、さらにBrδが5Gμ
m以上、30Gμm以下の時には媒体ノイズが著しく低
下してS/Nは1.2以上となった。さらに、成膜時の
直流バイアス電圧を−10V〜−500Vの範囲で制御
することにより、下地膜及び磁性膜中のXe濃度を制御
した結果、Xe濃度が0.01原子%以上、5原子%以
下の時にHkの値は10kOe以上、20kOe以下と
なり、S/Nは1.5以上とさらに良好な特性を示し
た。
FIG. 6 shows the relationship between Brδ and coercive force Hc.
Hc is 1 when Brδ is 5 Gμm or more and less than 80 Gμm
It was 000 Oe or more and 3500 Oe or less. Further, the recording / reproducing S / N at a head flying height of 0.02 μm and a linear recording density of 250 kPBI has a Brδ of 5 Gμm or more, 80
When it is less than Gμm, it becomes 1 or more, and Brδ is 5Gμ.
When m or more and 30 Gμm or less, the medium noise was remarkably reduced and the S / N became 1.2 or more. Furthermore, the Xe concentration in the underlayer film and the magnetic film was controlled by controlling the DC bias voltage during film formation in the range of -10V to -500V. As a result, the Xe concentration was 0.01 atom% or more and 5 atom% or more. In the following cases, the value of Hk was 10 kOe or more and 20 kOe or less, and the S / N ratio was 1.5 or more, showing further excellent characteristics.

【0057】〔実施例5〕外径65mm、内径20m
m、厚さ0.3mmのTiO2 基板表面を、ラッピング
マシンを用いて中心線平均粗さRaが0.3nmとなる
まで平滑に研磨し、洗浄及び乾燥した。その後、テープ
ポリッシングマシンを用い、平均砥粒径1μm以下のダ
イアモンド研磨剤の存在下で、研磨テープをコンタクト
ロールを通してディスク基板を回転させながらディスク
面の両側に押しつけることにより、基板表面に深さや密
度が不規則なテクスチャー溝を形成した。さらに、基板
に付着した研磨剤等の汚れを洗浄して乾燥した。半径方
向に測定した基板表面の溝の中心線平均粗さRaは0.
7nm、ヘッド走行方向と略垂直方向の距離1μmにお
ける、深さ1nm以上、50nm以下の溝の平均密度は
100本であった。
[Embodiment 5] Outer diameter 65 mm, inner diameter 20 m
The surface of the TiO 2 substrate having a thickness of 0.3 mm and a thickness of 0.3 mm was smoothed by a lapping machine until the centerline average roughness Ra became 0.3 nm, washed and dried. After that, using a tape polishing machine, in the presence of a diamond abrasive having an average abrasive grain size of 1 μm or less, the polishing tape is pressed against both sides of the disk surface while rotating the disk substrate through a contact roll, so that the depth and density of the substrate surface are increased. Formed irregular texture grooves. Further, dirt such as abrasives attached to the substrate was washed and dried. The center line average roughness Ra of the groove on the substrate surface measured in the radial direction is 0.
The average density of the grooves having a depth of 1 nm or more and 50 nm or less was 100 at a distance of 7 nm and a distance of 1 μm in the direction substantially perpendicular to the head traveling direction.

【0058】このディスク基板をスパッタリング装置内
で、真空槽体積当りの水蒸気の排気速度500l/s以
上の排気ポンプを用いて真空保持し、基板温度を100
℃から400℃の範囲で加熱した後、0.1mTorr
から5mTorrの範囲のKr圧のもとで第1層下地膜
としてRuを10nm形成し、次いで第2層下地膜とし
てCr−5Si合金を膜厚10nm形成した。この複合
下地膜上に膜厚5nmのCo−Cr−Ta磁性膜を形成
した。この時のBrδの値は20Gμmであった。成膜
時の基板温度、Kr分圧を制御することにより、磁性膜
結晶中の面心立方格子型の結晶格子の密度を制御した。
この時のHcは1000Oe以上、3500Oe以下で
あった。
The disk substrate was vacuum-held in a sputtering apparatus by using an exhaust pump having an exhaust rate of water vapor per volume of the vacuum chamber of 500 l / s or more, and the substrate temperature was set to 100.
0.1mTorr after heating in the range of ℃ to 400 ℃
Under a Kr pressure in the range from 1 to 5 mTorr, Ru was formed to a thickness of 10 nm as a first-layer underlayer film, and then Cr-5Si alloy was formed to a thickness of 10 nm as a second-layer underlayer film. A Co-Cr-Ta magnetic film having a thickness of 5 nm was formed on this composite underlayer. At this time, the value of Brδ was 20 Gμm. By controlling the substrate temperature and the Kr partial pressure during film formation, the density of the face-centered cubic crystal lattice in the magnetic film crystal was controlled.
Hc at this time was 1000 Oe or more and 3500 Oe or less.

【0059】図7に面心立方格子型の結晶格子密度と、
Hk、及びヘッド浮上量0.02μm、線記録密度25
0kPBIにおける記録再生S/Nの値の関係を示す。
成膜時の基板温度を向上し、Kr分圧を低下するに従い
面心立方格子型の結晶格子密度が減少し、面心立方格子
型の結晶格子密度が0.01%以上、5%以下におい
て、Hkの値は7kOe以上、20kOe以下となり、
S/Nは1以上と良好な特性を示した。さらに、成膜時
の直流バイアス電圧を−10Vから−500Vの範囲で
制御することにより、下地膜及び磁性膜中のKr濃度を
制御した結果、Kr濃度が0.01原子%以上、5原子
%以下の時にHkの値は10kOe以上、20kOe以
下となり、S/Nは1.2以上とさらに良好な特性を示
した。
FIG. 7 shows the face centered cubic lattice type crystal lattice density,
Hk, head flying height 0.02 μm, linear recording density 25
The relationship between the values of recording / reproducing S / N at 0 kPBI is shown.
As the substrate temperature during film formation is increased and the Kr partial pressure is decreased, the face-centered cubic lattice type crystal lattice density is reduced. When the face-centered cubic lattice type crystal lattice density is 0.01% or more and 5% or less. , Hk is 7 kOe or more and 20 kOe or less,
The S / N ratio was 1 or more, indicating good characteristics. Furthermore, by controlling the DC bias voltage during film formation in the range of −10 V to −500 V, the Kr concentration in the underlayer and the magnetic film was controlled. As a result, the Kr concentration was 0.01 atomic% or more and 5 atomic% or more. In the following cases, the value of Hk was 10 kOe or more and 20 kOe or less, and the S / N ratio was 1.2 or more, showing further excellent characteristics.

【0060】本実施例の方法により形成された磁気記録
媒体をX線回折分析した結果、Cr−Si下地層では体
心立方構造の(110)結晶格子面が基板面と略並行と
なるよう結晶が配向成長していることが確認された。ま
た、磁性層では六方晶構造の(100)面がディスク基
板表面と略並行となるよう配向していた。また、保護膜
表面の中心線平均粗さRaは1.0nm、磁性膜表面の
中心線平均粗さRaは0.9nmであった。
As a result of the X-ray diffraction analysis of the magnetic recording medium formed by the method of this example, the Cr-Si underlayer was crystallized so that the (110) crystal lattice plane of the body-centered cubic structure was substantially parallel to the substrate surface. It was confirmed that the grains were oriented and grown. Moreover, in the magnetic layer, the (100) plane of the hexagonal structure was oriented so as to be substantially parallel to the surface of the disk substrate. The center line average roughness Ra of the protective film surface was 1.0 nm, and the center line average roughness Ra of the magnetic film surface was 0.9 nm.

【0061】本実施例の媒体を用いて、浮上量0.02
μmにおいてGMRヘッドを媒体内周から外周まで10
万回シークした結果、ヘッドと媒体の接触は起こらない
ことが確認された。本効果は第1層下地膜としてZr、
Si、Sc、A 、C、Ge、Sb、Ga、Ru、P
d、V、Nb、Ta、Hf、Rh、Ni−P、Ni−B
もしくはこれらを主たる成分とするZr−Ta、Si−
C、Sc−V、Al−Mg、V−Fe、Nb−Cr、T
a−Cr、Hf−Zr、Ta−Mo等の合金を用いた場
合でも同様に認められた。
Using the medium of this embodiment, the flying height is 0.02.
At the μm, the GMR head is 10
As a result of 10,000 seeks, it was confirmed that contact between the head and the medium did not occur. This effect is achieved by using Zr as the first underlayer film,
Si, Sc, A, C, Ge, Sb, Ga, Ru, P
d, V, Nb, Ta, Hf, Rh, Ni-P, Ni-B
Alternatively, Zr-Ta, Si-containing these as main components
C, Sc-V, Al-Mg, V-Fe, Nb-Cr, T
The same was found when alloys such as a-Cr, Hf-Zr, and Ta-Mo were used.

【0062】〔実施例6〕実施例1〜5に示した媒体と
同等の特性を有する磁気記録媒体4枚を使用し、Co−
Ni−FeもしくはCo−Ta−Zr合金を記録用磁極
材とし、再生部にGMR素子を有する複合型薄膜磁気ヘ
ッド7個と、サーボ用のNi−Fe合金を記録再生用磁
極とする薄膜ヘッドとを組み合わせた磁気記録装置を試
作した。本装置は、平面図8(a)及びA−A’断面図
8(b)に示すように、磁気記録媒体81、磁気記録媒
体駆動部82、磁気ヘッド83、磁気ヘッド駆動部8
4、記録再生信号処理系85などの部品から構成され
る。
[Embodiment 6] Four magnetic recording media having the same characteristics as those of the media shown in Embodiments 1 to 5 were used, and Co-
A composite thin-film magnetic head having Ni-Fe or Co-Ta-Zr alloy as a recording magnetic pole material and a GMR element in a reproducing portion, and a thin-film head having a servo Ni-Fe alloy as a recording / reproducing magnetic pole. A magnetic recording device was manufactured by combining the above. As shown in a plan view 8 (a) and an AA ′ cross-sectional view 8 (b), this apparatus includes a magnetic recording medium 81, a magnetic recording medium drive unit 82, a magnetic head 83, and a magnetic head drive unit 8.
4. The recording / playback signal processing system 85 and other components.

【0063】この磁気記録装置を使用し、スペーシング
0.03μmにおいてエラーが発生するまでの平均時間
を求めたところ従来装置に比較して2〜3倍になり、信
頼性が極めて高いことを実証できた。また、本実施例で
試作した磁気記録装置はヘッド浮上量が低いため、信号
の記録再生における位相マージンが広くなり、面記録密
度を比較例の媒体を用いた浮上量0.12μmの場合の
10倍に高めることができ、小形で大容量の磁気記録装
置を提供できた。
Using this magnetic recording device, when the average time until an error occurred at a spacing of 0.03 μm was obtained, it was 2-3 times that of the conventional device, demonstrating extremely high reliability. did it. Further, since the magnetic recording device prototyped in this example has a low head flying height, the phase margin in recording / reproducing a signal is wide, and the areal recording density is 10 when the flying height is 0.12 μm using the medium of the comparative example. It was possible to provide a compact and large-capacity magnetic recording device that can be doubled in size.

【0064】本装置を用いてトラック幅が2μm以下の
GMRヘッドで再生した場合に200kBPI以上の高
い記録密度においてS/Nが1以上、さらに、オーバー
ライト(O/W)特性が26dB以上の大容量磁気記録
装置が得られた。特に、10kTPI以上の高記録密度
時にも本実施例の媒体はトラック幅方向の書きにじみが
充分に行われるため、高いS/Nが得られた。また、基
板表面のテクスチャー形状が小さいためサーボ信号の品
位も高く、良好なヘッド位置決めができた。サーボ用ヘ
ッドを複合ヘッドとした場合にも同様の効果が得られ
た。
When reproducing with a GMR head having a track width of 2 μm or less using this apparatus, the S / N is 1 or more at a high recording density of 200 kBPI or more, and the overwriting (O / W) characteristic is 26 dB or more. A capacitive magnetic recording device was obtained. In particular, even at a high recording density of 10 kTPI or higher, the medium of the present example sufficiently bleeds in the track width direction, so that a high S / N was obtained. Also, since the texture shape of the substrate surface is small, the quality of the servo signal is high, and good head positioning was possible. Similar effects were obtained when the servo head was a composite head.

【0065】本実施例では、Co−Ni−Feもしくは
CoTaZr合金を磁極材とする薄膜磁気ヘッドを用い
た場合について説明したが、NiFe、Fe−Al合金
磁性膜、もしくはこれらを用いた多層磁性膜等を記録用
磁極材とする録再分離型薄膜磁気ヘッド、CoTaZ
r、FeAlSi合金等をギャップ部に設けたメタル・
イン・ギャップ型(MIG)録再分離複合磁気ヘッド、
さらには誘導型薄膜ヘッド又はMIGヘッドを用いた場
合にも同様の効果が得られることを確認した。
In the present embodiment, the case of using the thin film magnetic head having the magnetic pole material of Co--Ni--Fe or CoTaZr alloy has been described. However, the NiFe, Fe--Al alloy magnetic film, or the multilayer magnetic film using them. Recording / reproducing separated thin-film magnetic head having recording magnetic pole material, CoTaZ
Metal with r, FeAlSi alloy, etc. provided in the gap
In-gap (MIG) recording / reproducing composite magnetic head,
Furthermore, it was confirmed that the same effect was obtained when an inductive thin film head or MIG head was used.

【0066】[0066]

【発明の効果】本発明によれば、再生感度の高いGMR
ヘッドに適応した高S/Nで、しかもGMRヘッドが浮
上量0.1μm以下で浮上可能な磁気記録媒体、及びそ
の製造方法、さらにこれを用いた小形で大容量の磁気記
録装置を提供できる。
According to the present invention, a GMR having high reproduction sensitivity
It is possible to provide a magnetic recording medium having a high S / N suitable for a head and capable of being floated by a GMR head with a flying height of 0.1 μm or less, a manufacturing method thereof, and a small-sized and large-capacity magnetic recording device using the same.

【図面の簡単な説明】[Brief description of drawings]

【図1】本発明に係る薄膜型磁気記録媒体の断面構造
図。
FIG. 1 is a sectional structural view of a thin film magnetic recording medium according to the present invention.

【図2】本発明の一実施例の薄膜型磁気記録媒体の断面
構造図。
FIG. 2 is a sectional structural view of a thin film magnetic recording medium of one embodiment of the present invention.

【図3】本発明の一実施例の薄膜型磁気記録媒体の異方
性磁界Hkと、記録再生時のS/Nとの関係を示す図。
FIG. 3 is a diagram showing a relationship between an anisotropic magnetic field Hk of a thin film magnetic recording medium of one embodiment of the present invention and S / N at the time of recording / reproducing.

【図4】本発明の一実施例の薄膜型磁気記録媒体の磁性
膜結晶の粒界の幅と、保磁力Hc、及び記録再生時のS
/Nとの関係を示す図。
FIG. 4 is a graph showing the width of the grain boundary of the magnetic film crystal of the thin film magnetic recording medium according to the embodiment of the present invention, the coercive force Hc, and S at the time of recording / reproducing.
The figure which shows the relationship with / N.

【図5】本発明の一実施例の薄膜型磁気記録媒体の磁性
膜の格子定数比c/aと、異方性磁界Hk、及び記録再
生時のS/Nとの関係を示す図。
FIG. 5 is a diagram showing the relationship between the lattice constant ratio c / a of the magnetic film of the thin film magnetic recording medium of one embodiment of the present invention, the anisotropic magnetic field Hk, and the S / N during recording / reproduction.

【図6】本発明の一実施例の薄膜型磁気記録媒体の残留
磁束密度膜厚積Brδと保磁力Hcとの関係を示す図。
FIG. 6 is a diagram showing a relationship between a residual magnetic flux density film thickness product Brδ and a coercive force Hc of a thin film magnetic recording medium according to an example of the present invention.

【図7】本発明の一実施例の薄膜型磁気記録媒体の磁性
膜結晶中の面心立方格子型の結晶格子の密度と、異方性
磁界Hk、及び記録再生時のS/Nとの関係を示す図。
FIG. 7 shows the density of the face-centered cubic lattice type crystal lattice in the magnetic film crystal of the thin film type magnetic recording medium of one embodiment of the present invention, the anisotropic magnetic field Hk, and the S / N at the time of recording / reproducing. The figure which shows a relationship.

【図8】本発明の一実施例の磁気記録装置の断面構造
図。
FIG. 8 is a sectional structural view of a magnetic recording apparatus according to an embodiment of the present invention.

【符号の説明】[Explanation of symbols]

11…磁気ディスク基板、12,12’…非磁性メッキ
層、13,13’…金属下地膜、14,14’…金属磁
性膜、15,15’…非磁性保護膜、21…非磁性保護
膜、22…金属磁性膜、23…非磁性下地膜、24…磁
気ディスク基板、25…保護膜エッチング部、81…磁
気記録媒体、82…磁気記録媒体駆動部、83…磁気ヘ
ッド、84…磁気ヘッド駆動部、85…記録再生信号処
理系
11 ... Magnetic disk substrate, 12, 12 '... Non-magnetic plating layer, 13, 13' ... Metal base film, 14, 14 '... Metal magnetic film, 15, 15' ... Non-magnetic protective film, 21 ... Non-magnetic protective film , 22 ... Metal magnetic film, 23 ... Non-magnetic underlayer film, 24 ... Magnetic disk substrate, 25 ... Protective film etching section, 81 ... Magnetic recording medium, 82 ... Magnetic recording medium drive section, 83 ... Magnetic head, 84 ... Magnetic head Drive unit, 85 ... Recording / reproducing signal processing system

───────────────────────────────────────────────────── フロントページの続き (72)発明者 屋久 四男 東京都国分寺市東恋ヶ窪一丁目280番地 株式会社日立製作所中央研究所内 (72)発明者 山本 朋生 東京都国分寺市東恋ヶ窪一丁目280番地 株式会社日立製作所中央研究所内 (72)発明者 五十嵐 万壽和 東京都国分寺市東恋ヶ窪一丁目280番地 株式会社日立製作所中央研究所内 ─────────────────────────────────────────────────── --- Continuation of the front page (72) Inventor Yasuo Yaku 1-280 Higashi Koigakubo, Kokubunji, Tokyo Inside Central Research Laboratory, Hitachi, Ltd. Central Research Laboratory, Mfg. Co., Ltd. (72) Inventor Manwakazu Igarashi 1-280, Higashikoigakubo, Kokubunji, Tokyo Metropolitan Research Center, Hitachi, Ltd.

Claims (21)

【特許請求の範囲】[Claims] 【請求項1】 非磁性ディスク基板と、該非磁性ディス
ク基板上に直接もしくは少なくとも一層の下地膜を介し
て形成された磁性膜を少なくとも一層有する磁気記録媒
体において、ヘッド走行方向に測定した磁性膜の残留磁
化Brと磁性膜の総膜厚δとの積Brδの値が5Gμm
以上、80Gμm未満であり、かつ、上記媒体の異方性
磁界Hkの値が7kOe以上、20kOe以下であるこ
とを特徴とする磁気記録媒体。
1. A magnetic recording medium comprising a non-magnetic disk substrate and at least one magnetic film formed on the non-magnetic disk substrate directly or via at least one underlayer film, the magnetic film being measured in a head traveling direction. The value of the product Brδ of the residual magnetization Br and the total film thickness δ of the magnetic film is 5 Gμm.
As described above, the magnetic recording medium is less than 80 Gμm and the anisotropic magnetic field Hk of the medium is 7 kOe or more and 20 kOe or less.
【請求項2】 Brδの値が5Gμm以上、30Gμm
以下であることを特徴とする請求項1記載の磁気記録媒
体。
2. The value of Brδ is 5 Gμm or more and 30 Gμm.
The magnetic recording medium according to claim 1, wherein:
【請求項3】 保磁力が1000Oe以上、3500O
e以下であることを特徴とする請求項1又は2記載の磁
気記録媒体。
3. A coercive force of 1000 Oe or more and 3500 Oe.
3. The magnetic recording medium according to claim 1, wherein the magnetic recording medium is e or less.
【請求項4】 磁性膜結晶の粒界の幅が0.5nm以
上、5nm以下であることを特徴とする請求項1、2又
は3記載の磁気記録媒体。
4. The magnetic recording medium according to claim 1, 2 or 3, wherein the grain boundary width of the magnetic film crystal is 0.5 nm or more and 5 nm or less.
【請求項5】 磁性膜は実質的に六方晶型結晶構造を有
し、該磁性膜のc軸が実質的に基板面内方向に配向して
おり、六方晶型の格子定数のa及びcの長さの比c/a
の値が1.3以上、1.6以下であることを特徴とする
請求項1〜4のいずれか1項記載の磁気記録媒体。
5. The magnetic film has a substantially hexagonal crystal structure, the c-axis of the magnetic film is oriented substantially in the in-plane direction of the substrate, and the hexagonal lattice constants a and c are used. Ratio of length c / a
5. The magnetic recording medium according to claim 1, wherein the value of is 1.3 or more and 1.6 or less.
【請求項6】 磁性膜は実質的に六方晶型結晶構造を有
し、該磁性膜結晶中に存在する面心立方格子を形成する
積層欠陥の密度が5%以下であることを特徴とする請求
項1〜5のいずれか1項記載の磁気記録媒体。
6. The magnetic film has a substantially hexagonal crystal structure, and the density of stacking faults forming a face-centered cubic lattice present in the magnetic film crystal is 5% or less. The magnetic recording medium according to claim 1.
【請求項7】 磁性膜及び/又は下地膜中に、Ar、X
e、Krの少なくとも一つの元素が0.01%以上、5
%以下の原子濃度で存在することを特徴とする請求項1
〜6のいずれか1項記載の磁気記録媒体。
7. Ar, X in the magnetic film and / or underlayer film
At least one element of e and Kr is 0.01% or more, 5
% Of the atomic concentration is present or less.
7. The magnetic recording medium according to any one of claims 6 to 6.
【請求項8】 Cr、Mo、W、V、Ta、Nb、Z
r、Ti、B、Be、C、Ni−P、Ni−Bの少なく
とも一つを主たる成分とする膜厚0.5nm以上、5n
m以下の非磁性中間層を介して、磁性膜が2層以上に多
層化されていることを特徴とする請求項1〜7のいずれ
か1項記載の磁気記録媒体。
8. Cr, Mo, W, V, Ta, Nb, Z
A film thickness of 0.5 nm or more and 5 n containing at least one of r, Ti, B, Be, C, Ni-P, and Ni-B as a main component.
8. The magnetic recording medium according to claim 1, wherein the magnetic film is multi-layered into two or more layers via a non-magnetic intermediate layer of m or less.
【請求項9】 磁性膜表面のヘッド走行方向と垂直の方
向に測定した中心線平均粗さが0.3nm以上、1.9
nm以下であることを特徴とする請求項1〜8のいずれ
か1項記載の磁気記録媒体。
9. The center line average roughness measured in the direction perpendicular to the head running direction on the surface of the magnetic film is 0.3 nm or more and 1.9.
The magnetic recording medium according to claim 1, wherein the magnetic recording medium has a thickness of not more than nm.
【請求項10】 磁性膜上に保護膜を有し、かつ該保護
膜が磁性膜表面に比べて大きな面粗さを有することを特
徴とする請求項1〜9のいずれか1項記載の磁気記録媒
体。
10. A magnetic film according to claim 1, wherein a protective film is provided on the magnetic film, and the protective film has a larger surface roughness than the surface of the magnetic film. recoding media.
【請求項11】 保護膜表面のヘッド走行方向と垂直の
方向に測定した中心線平均粗さRaが0.3nm以上、
3nm以下であることを特徴とする請求項10記載の磁
気記録媒体。
11. The center line average roughness Ra measured in the direction perpendicular to the head running direction on the surface of the protective film is 0.3 nm or more,
The magnetic recording medium according to claim 10, which has a thickness of 3 nm or less.
【請求項12】 非磁性ディスク基板と磁性膜との間に
Cr、Mo、W、Nb又はTaを主たる成分とし、T
i、Pt、Pd、Si、Fe、V、Ru、P又はBのい
ずれか少なくとも1種の元素を添加した合金下地膜が磁
性膜に隣接して形成され、その膜厚が5nm以上、50
0nm以下であることを特徴とする請求項1〜11のい
ずれか1項記載の磁気記録媒体。
12. A thin film containing Cr, Mo, W, Nb or Ta as a main component between the non-magnetic disk substrate and the magnetic film, and
An alloy underlayer film containing at least one element selected from i, Pt, Pd, Si, Fe, V, Ru, P and B is formed adjacent to the magnetic film and has a thickness of 5 nm or more, 50
It is 0 nm or less, The magnetic recording medium of any one of Claims 1-11 characterized by the above-mentioned.
【請求項13】 前記下地膜が少なくとも2層の非磁性
膜で構成され、基板側下地膜がZr、Si、Ti、S
c、Al、C、Ge、Sb、Ga、Ru、Pd、V、N
b、Ta、Hf、Rh、Ni−P又はNi−B、もしく
はこれらを主たる成分とする合金であることを特徴とす
る請求項1〜12のいずれか1項記載の磁気記録媒体。
13. The base film is composed of at least two non-magnetic films, and the base film on the substrate side is Zr, Si, Ti, S.
c, Al, C, Ge, Sb, Ga, Ru, Pd, V, N
13. The magnetic recording medium according to claim 1, which is b, Ta, Hf, Rh, Ni-P or Ni-B, or an alloy containing any of these as a main component.
【請求項14】 磁性膜がCo−Cr−Ta系、Co−
Cr−Ni系又はCo−Cr−Pt系の合金を主成分と
することを特徴とする請求項1〜13のいずれか1項記
載の磁気記録媒体。
14. The magnetic film is a Co—Cr—Ta system, Co—
The magnetic recording medium according to any one of claims 1 to 13, which comprises a Cr-Ni-based or Co-Cr-Pt-based alloy as a main component.
【請求項15】 基板がAl−Mg合金、化学強化ガラ
ス、有機樹脂、Ti、Si、カーボン、又はTiO2
SiC等のセラミックスからなることを特徴とする請求
項1〜14のいずれか1項記載の磁気記録媒体。
15. The substrate is an Al—Mg alloy, chemically strengthened glass, organic resin, Ti, Si, carbon, or TiO 2 ,
15. The magnetic recording medium according to claim 1, wherein the magnetic recording medium is made of ceramics such as SiC.
【請求項16】 非磁性ディスク基板上にスパッタリン
グ法によって磁性膜を形成する工程を含む請求項1〜1
5のいずれか1項記載の磁気記録媒体の製造方法におい
て、 前記工程において非磁性ディスク基板に負のバイアス電
圧を10V以上、500V以下印加することを特徴とす
る請求項1〜15のいずれか1項記載の磁気記録媒体の
製造方法
16. A method of forming a magnetic film on a non-magnetic disk substrate by a sputtering method.
16. The method for manufacturing a magnetic recording medium according to claim 5, wherein a negative bias voltage of 10 V or more and 500 V or less is applied to the nonmagnetic disk substrate in the step. Manufacturing method of magnetic recording medium according to item
【請求項17】 非磁性ディスク基板上にスパッタリン
グ法によって非磁性材料からなる下地膜を形成する第1
の工程、前記工程で形成された下地膜の上にスパッタリ
ング法によって磁性膜を形成する第2の工程を含む請求
項1〜15のいずれか1項記載の磁気記録媒体の製造方
法において、 前記第1の工程及び第2の工程において非磁性ディスク
基板に負のバイアス電圧を10V以上、500V以下印
加することを特徴とする請求項1〜15のいずれか1項
記載の磁気記録媒体の製造方法
17. A base film made of a non-magnetic material is formed on a non-magnetic disk substrate by a sputtering method.
16. The method of manufacturing a magnetic recording medium according to claim 1, further comprising: 16. The method of manufacturing a magnetic recording medium according to claim 1, wherein a negative bias voltage of 10 V or more and 500 V or less is applied to the non-magnetic disk substrate in the first step and the second step.
【請求項18】 磁気記録媒体と、磁気記録媒体駆動手
段と、巨大磁気抵抗効果素子を再生手段を有する磁気ヘ
ッドと、磁気ヘッド駆動手段と、記録再生信号処理手段
を有する磁気記録装置において、磁気ヘッドの浮上量が
0.1μm以下であり、ヘッド走行方向に測定した磁気
記録媒体中の磁性膜の残留磁化Brと総膜厚δとの積B
rδの値が5Gμm以上、80Gμm以下であり、か
つ、上記媒体の異方性磁界Hkの値が7kOe以上、2
0kOe以下であることを特徴とする磁気記録装置。
18. A magnetic recording device comprising a magnetic recording medium, a magnetic recording medium driving means, a magnetic head having a giant magnetoresistive effect element as a reproducing means, a magnetic head driving means, and a recording / reproducing signal processing means. The flying height of the head is 0.1 μm or less, and the product B of the residual film thickness Br of the magnetic film in the magnetic recording medium and the total film thickness δ measured in the head traveling direction.
The value of rδ is 5 Gμm or more and 80 Gμm or less, and the value of the anisotropic magnetic field Hk of the medium is 7 kOe or more, 2
A magnetic recording device characterized by being 0 kOe or less.
【請求項19】 磁気記録媒体の線記録密度が150k
BPI以上であることを特徴とする請求項18記載の磁
気記録装置。
19. The magnetic recording medium has a linear recording density of 150 k.
The magnetic recording device according to claim 18, wherein the magnetic recording medium has a BPI or more.
【請求項20】 磁気記録媒体の記録トラック密度が1
0kTPI以上であることを特徴とする請求項18記載
の磁気記録装置。
20. The recording track density of a magnetic recording medium is 1
The magnetic recording device according to claim 18, wherein the magnetic recording device has a recording capacity of 0 kTPI or more.
【請求項21】 請求項1〜15のいずれか1項記載の
磁気記録媒体と、磁気記録媒体駆動手段と、磁気記録再
生部を有する磁気ヘッドと、磁気ヘッド駆動手段と、記
録再生信号処理手段とを含む磁気記録装置。
21. A magnetic recording medium according to claim 1, a magnetic recording medium driving means, a magnetic head having a magnetic recording / reproducing section, a magnetic head driving means, and a recording / reproducing signal processing means. And a magnetic recording device including.
JP22122793A 1993-07-22 1993-09-06 Magnetic recording media Expired - Lifetime JP3359706B2 (en)

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JP22122793A JP3359706B2 (en) 1993-09-06 1993-09-06 Magnetic recording media
KR1019940017352A KR0148842B1 (en) 1993-07-22 1994-07-19 Magnetic recording medium, process for producing the same and magnetic recording system
KR97047773A KR0141381B1 (en) 1993-07-22 1997-09-19 Magnetic recording medium and its production and magnetic recorder
US08/967,346 US5815343A (en) 1993-07-22 1997-10-27 Magnetic recording medium, process for producing the same and magnetic recording system

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Cited By (6)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
EP1047548A4 (en) * 1998-01-15 2002-10-29 Flextor Inc A metal foil disk for high areal density recording in environments of high mechanical shock
US6596420B2 (en) 1996-05-20 2003-07-22 Hitachi, Ltd. Magnetic recording media and magnetic recording system using the same
US6878459B2 (en) 2000-12-27 2005-04-12 Migaku Takahashi Magnetic recording medium with Cr underfilm
JP2008090913A (en) * 2006-09-29 2008-04-17 Hoya Corp Magnetic recording medium
KR100976013B1 (en) * 2007-08-30 2010-08-17 티디케이가부시기가이샤 Magnetic recording and reproducing apparatus
US7864468B2 (en) 2007-08-30 2011-01-04 Tdk Corporation Magnetic recording and reproducing apparatus including a magnetic recording medium and a magnetic head for recording data on the magnetic recording medium

Cited By (7)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US6596420B2 (en) 1996-05-20 2003-07-22 Hitachi, Ltd. Magnetic recording media and magnetic recording system using the same
US7056604B2 (en) 1996-05-20 2006-06-06 Hitachi Global Storage Technologies Japan, Ltd. Magnetic recording media and magnetic recording system using the same
EP1047548A4 (en) * 1998-01-15 2002-10-29 Flextor Inc A metal foil disk for high areal density recording in environments of high mechanical shock
US6878459B2 (en) 2000-12-27 2005-04-12 Migaku Takahashi Magnetic recording medium with Cr underfilm
JP2008090913A (en) * 2006-09-29 2008-04-17 Hoya Corp Magnetic recording medium
KR100976013B1 (en) * 2007-08-30 2010-08-17 티디케이가부시기가이샤 Magnetic recording and reproducing apparatus
US7864468B2 (en) 2007-08-30 2011-01-04 Tdk Corporation Magnetic recording and reproducing apparatus including a magnetic recording medium and a magnetic head for recording data on the magnetic recording medium

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