JP2875746B2 - Interference film thickness meter - Google Patents

Interference film thickness meter

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Publication number
JP2875746B2
JP2875746B2 JP24858294A JP24858294A JP2875746B2 JP 2875746 B2 JP2875746 B2 JP 2875746B2 JP 24858294 A JP24858294 A JP 24858294A JP 24858294 A JP24858294 A JP 24858294A JP 2875746 B2 JP2875746 B2 JP 2875746B2
Authority
JP
Japan
Prior art keywords
film thickness
film
interference
waveform
interference fringes
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.)
Expired - Fee Related
Application number
JP24858294A
Other languages
Japanese (ja)
Other versions
JPH0886619A (en
Inventor
厚 染谷
浩樹 藤下
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.)
Canon Marketing Japan Inc
Original Assignee
Canon Hanbai KK
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 Canon Hanbai KK filed Critical Canon Hanbai KK
Priority to JP24858294A priority Critical patent/JP2875746B2/en
Publication of JPH0886619A publication Critical patent/JPH0886619A/en
Application granted granted Critical
Publication of JP2875746B2 publication Critical patent/JP2875746B2/en
Anticipated expiration legal-status Critical
Expired - Fee Related legal-status Critical Current

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Description

【発明の詳細な説明】DETAILED DESCRIPTION OF THE INVENTION

【0001】[0001]

【産業上の利用分野】本発明は物体表面に施された透明
若しくは半透明の薄膜の膜厚を膜の上面と下面とからの
反射波面をティルトさせ、これらを干渉させることによ
り測定する干渉膜厚計に関するものである。
BACKGROUND OF THE INVENTION 1. Field of the Invention The present invention relates to an interference film for measuring the thickness of a transparent or translucent thin film applied to the surface of an object by tilting a wavefront reflected from the upper surface and the lower surface of the film and causing them to interfere with each other. It concerns the thickness gauge.

【0002】[0002]

【従来の技術】従来技術として知られている干渉膜厚計
は、上下面からの反射波をP偏光、S偏光に分離し、そ
れぞれをウォーラストンプリズムによってティルトする
ことで生じた干渉縞の間隔をビデオカメラの1ライン上
の光量分布のピーク位置間距離を測定することで測定し
ていた(図4(a))。
2. Description of the Related Art An interference film thickness meter known as a prior art separates reflected waves from the upper and lower surfaces into P-polarized light and S-polarized light, and tilts each of them by a Wollaston prism to form an interval between interference fringes. Was measured by measuring the distance between the peak positions of the light intensity distribution on one line of the video camera (FIG. 4A).

【0003】[0003]

【発明が解決しようとする課題】一方、現在では1μm
以下の薄膜を0.01μm程度の分解能で測定すること
が要求されている。ところが、従来の干渉膜厚計は膜厚
1μm〜30μm程度の比較的厚い膜を測定するのに用
いられ、分解能も0.1μmが限度である。これは、薄
膜の膜厚を測定する場合、上面反射波同士及び下面反射
波同士の基準干渉縞に、上面と下面との反射波の干渉縞
が重なってしまい(図4(b))、この状態で基準干渉
縞と膜厚干渉縞(上下反射波面の干渉縞)との間隔を計
ることが困難であることなどが原因として挙げられる。
On the other hand, at present, 1 μm
It is required to measure the following thin films with a resolution of about 0.01 μm. However, the conventional interference film thickness meter is used to measure a relatively thick film having a film thickness of about 1 μm to 30 μm, and the resolution is limited to 0.1 μm. This is because when measuring the film thickness of the thin film, the interference fringes of the reflected waves of the upper surface and the lower surface overlap the reference interference fringes of the upper surface reflected waves and the lower surface reflected waves (FIG. 4B). The reason is that it is difficult to measure the interval between the reference interference fringe and the thickness interference fringe (the interference fringes of the vertically reflected wavefront) in the state.

【0004】一方、上記干渉膜厚計ではウォーラストン
プリズム内に干渉縞ができるため、プリズムの傷、ごみ
の付着等によって測定が不可能になることから、これら
傷、ごみ等がないように研磨工程や清掃に時間がかか
り、コストが高騰化すると云う問題もある。
On the other hand, in the interference film thickness meter, since interference fringes are formed in the Wollaston prism, the measurement becomes impossible due to scratches on the prism, adhesion of dust, and the like. There is also a problem that it takes time for processes and cleaning, and the cost rises.

【0005】本発明は上記したような従来技術の問題点
に鑑みなされたものであり、その主な目的は、撮像素子
上に干渉縞同士が重ならず、1μm以下の薄膜を0.0
1μm程度の分解能で測定することが可能であり、取扱
い、メンテナンスも容易な干渉膜厚計を提供することに
ある。
The present invention has been made in view of the above-mentioned problems of the prior art, and its main purpose is to form a thin film having a thickness of 1 μm or less such that interference fringes do not overlap each other on an image sensor.
An object of the present invention is to provide an interference film thickness meter which can measure at a resolution of about 1 μm and is easy to handle and maintain.

【0006】[0006]

【課題を解決するための手段】上記した目的は本発明に
よれば、基板上に直接若しくは別の膜を介して形成され
た膜に照明光を照射し、該膜の上面及び下面からの反射
光を複屈折性プリズムによりP偏光波とS偏光波とに分
け、それぞれ別方向に傾けて、それらの波面の交線にて
生じる膜厚干渉縞の間隔を計測して膜厚を測定する干渉
膜厚計に於て、予め前記目的の膜のない状熊でその表面
から反射したP偏光波面とS偏光波面との交線にて生じ
基準干渉縞のみの波形を記憶する手段と、受光手段に
て前記膜厚干渉縞を含む像を結像させ、前記基準干渉縞
の波形を前記受光手段にて結像させた像の干渉縞波形か
ら減じる手段と、前記基準干渉縞の波形を減じた後の一
対の干渉縞の波形のピーク位置の間隔から前記膜の膜厚
を求める手段とを有することを特徴とする干渉膜厚計を
提供することにより達成される。
According to the present invention, a film formed directly on a substrate or through another film is irradiated with illumination light and reflected from the upper and lower surfaces of the film. The light is divided into a P-polarized wave and an S-polarized wave by a birefringent prism, tilted in different directions, and the film thickness is measured by measuring the interval of the film thickness interference fringe generated at the intersection of the wavefronts. In the film thickness meter , the surface without the target film
At the intersection of the P-polarized wavefront and the S-polarized wavefront reflected from
Means for storing the reference interference fringe only waveform that, to form an image including the thickness fringe by the light receiving unit, the interference fringe image obtained by imaging the waveform of the reference interference fringe in the light receiving means Means for subtracting from the waveform, and means for obtaining the film thickness of the film from the interval between the peak positions of the pair of interference fringe waveforms after subtracting the waveform of the reference interference fringe. Achieved by providing.

【0007】[0007]

【作用】このように、予め基準干渉縞の波形を記憶さ
せ、測定された干渉縞の波形からこの基準干渉縞の波形
減じ、上面からの反射波面と下面からの反射波面との
膜厚干渉縞のみを基準干渉縞のあった位置の両側に残
し、これらの干渉縞のピーク位置間隔を測定して1/2
にすれば、1μm以下の薄膜であってもその膜厚を容易
に、かつ正確に測定できる。このとき、例えばウォーラ
ストンプリズムを用いた場合、その頂角を小さくして上
面からの反射波面同士及び下面からの反射波面同士の基
準干渉縞と、上面及び下面からの反射波面の膜厚干渉縞
との間隔を広げると更に良い。また、上記複屈折性プリ
ズムに傷、ごみ等があっても上記減算処理によりその影
響が軽減され、または完全に除去される。
As described above, the waveform of the reference interference fringe is stored in advance, and the waveform of the reference interference fringe is obtained from the measured interference fringe waveform.
And only the film thickness interference fringes of the reflected wavefront from the upper surface and the reflected wavefront from the lower surface are left on both sides of the position where the reference interference fringes existed, and the peak position interval of these interference fringes is measured to be 1 /.
Accordingly, the thickness of a thin film of 1 μm or less can be easily and accurately measured. At this time, for example, when a Wollaston prism is used, the apex angle is reduced and the reference interference fringes between the reflected wavefronts from the upper surface and between the reflected wavefronts from the lower surface, and the thickness interference fringes of the reflected wavefronts from the upper and lower surfaces are reduced. It is even better to increase the distance between them. Further, even if the birefringent prism has a flaw, dust or the like, the influence thereof is reduced or completely removed by the subtraction processing.

【0008】[0008]

【実施例】以下、本発明の好適実施例を添付の図面につ
いて詳しく説明する。図1は、本発明が適用された干渉
膜厚計の光学素子及び処理ブロックの関係を示す図であ
る。光ファイバを介して発光装置から導光される照明光
は投光装置1からハーフミラー2に反射され、対物レン
ズ3を介して被測定物に照射されるようになっている。
また、被測定物に反射した光はハーフミラー2を透過
し、結像レンズ4、偏光フィルタ5を介して複屈折性プ
リズムとしてのウォーラストンプリズム6に入射し、P
偏光波とS偏光波とに分けられ、ティルトされ、偏光フ
ィルタ7、リレーレンズ8を介してCCDカメラ9に入
射することとなる。
BRIEF DESCRIPTION OF THE DRAWINGS FIG. 1 is a block diagram of a preferred embodiment of the present invention. FIG. 1 is a diagram showing a relationship between an optical element and a processing block of an interference film thickness meter to which the present invention is applied. Illumination light guided from the light emitting device via the optical fiber is reflected from the light projecting device 1 to the half mirror 2 and illuminates the object to be measured via the objective lens 3.
The light reflected on the object to be measured passes through the half mirror 2 and enters the Wollaston prism 6 as a birefringent prism via the imaging lens 4 and the polarizing filter 5.
The light is split into a polarized wave and an S-polarized wave, tilted, and enters the CCD camera 9 via the polarizing filter 7 and the relay lens 8.

【0009】CCDカメラ9に上記光が入射すると、光
電変換され、増幅器・フィルタブロック10にて増幅さ
れ、フィルタリングされて映像としてビデオモニタ11
に表示される(図2)と共に画像取り込みブロック12
で画像取り込み及びA/D変換される。ここで、本実施
例ではCCDカメラ9は768ドット×494ラインの
素子を有し、そのうちの中央の512ドット×128ラ
インの画像を測定領域に定めている。
When the light enters the CCD camera 9, the light is photoelectrically converted, amplified by an amplifier / filter block 10, filtered, and displayed as an image on a video monitor 11.
(FIG. 2) and the image capturing block 12
Is subjected to image capture and A / D conversion. Here, in the present embodiment, the CCD camera 9 has an element of 768 dots × 494 lines, of which an image of 512 dots × 128 lines at the center is defined as a measurement area.

【0010】A/D変換された512ドット×128ラ
インの画像はコンピュータ13に入力され、後記する平
均化、基準干渉縞波形の減算、膜厚干渉縞のピーク検
出、ピーク間距離の計算及び膜厚の計算が行われ、図示
されない出力装置からその結果が出力されることとな
る。
The A / D-converted image of 512 dots × 128 lines is input to the computer 13, and is averaged as described later, the subtraction of the reference interference fringe waveform, the detection of the peak of the film thickness interference fringe, the calculation of the distance between peaks and the film. The thickness is calculated, and the result is output from an output device (not shown).

【0011】以下に、CCDカメラ9に干渉縞を含む光
が入射した後の処理について詳細に説明する。まず、図
3(a)に示すようなCCDカメラ9からの生出力波形
を増幅器・フィルタブロック10にて増幅し、フィルタ
リングして各ラインからの信号波形を図3(b)に示す
ような波形に整形する。そして、画像取り込みブロック
12で、必要な中央128ラインの各信号波形から両端
128ドットのデータをカットして各ラインの波形を図
3(c)に示すような波形にトリミングする。
Hereinafter, the processing after light including interference fringes is incident on the CCD camera 9 will be described in detail. First, a raw output waveform from the CCD camera 9 as shown in FIG. 3A is amplified by an amplifier / filter block 10, filtered, and a signal waveform from each line is converted into a waveform as shown in FIG. To be shaped. Then, the image capturing block 12 cuts data of 128 dots at both ends from the necessary signal waveforms of the central 128 lines, and trims the waveform of each line into a waveform as shown in FIG.

【0012】次に、コンピュータ13内にて128ライ
ンからの各信号波形を平均化し、予め成膜されていない
上記被測定物に対して上記測定を行った結果の信号波
形、即ち基準干渉縞のみを有する信号波形を減じる(図
3(d))。その後、図3(d)の波形で各膜厚干渉縞
波形A、Bのピークを各々求め、ピーク値間隔をCCD
の素子数から計算する。ピーク間隔をy、膜の屈折率を
n、ウォーラストンプリズムによるP偏光波面及びS偏
光波面の傾き角をαとして膜厚dは次の式で与えられ
る。
Next, the signal waveforms from the 128 lines are averaged in the computer 13, and the signal waveform obtained as a result of performing the above measurement on the object to be measured on which no film is formed in advance, that is, only the reference interference fringes is obtained. Is reduced (FIG. 3 (d)) . Later, it obtains each waveform at the peak of the film thickness fringe waveform A, B in FIG. 3 (d), CCD peak value interval
Is calculated from the number of elements. The film thickness d is given by the following equation, where y is the peak interval, n is the refractive index of the film, and α is the inclination angle of the P-polarized wavefront and the S-polarized wavefront by the Wollaston prism.

【0013】[0013]

【数1】d=y・sinα/2n## EQU1 ## d = y · sin α / 2n

【0014】このようにして従来の干渉膜厚計で不可能
であった膜厚1μm以下の膜厚でも0.01μm程度の
分解能で、再現性±0.02μm程度に達する高精度の
測定が可能となる。ここで、ウォーラストンプリズムや
他の光学系に傷、ごみの付着等があっても多数のライン
の各信号波形を平均化すること及び同じウォーラストン
プリズムを含む同じ光学系で予め膜のない被測定物に対
して行った膜厚測定により得られた基準干渉縞のみを有
する信号波形を、実際の膜厚測定により得られた膜厚干
渉縞を有する信号波形から減じることにより、その影響
が軽減され、または完全に除去される。
In this way, even with a film thickness of 1 μm or less, which is impossible with a conventional interference film thickness meter, high-precision measurement with a resolution of about 0.01 μm and a reproducibility of about ± 0.02 μm is possible. Becomes Here, even if the Wollaston prism and other optical systems have scratches, dust and the like, the signal waveforms of many lines are averaged, and the same optical system including the same Wollaston prism has no film in advance. The effect is reduced by subtracting the signal waveform having only the reference interference fringes obtained by the film thickness measurement performed on the measurement object from the signal waveform having the film thickness interference fringes obtained by the actual film thickness measurement. Or completely removed.

【0015】尚、本実施例では複屈折性プリズムとして
ウォーラストンプリズムを用いたが、ニコルプリズム、
グラン・トムソンプリズムやローションプリズムなど、
P偏光とS偏光とを分離して傾けることができるもので
あれば良いことは云うまでもない。また、ピディコン或
いはニュービコン等の撮像管に於ては温度ドリフトによ
る誤差を除くことが困難であり、これも分解能を向上で
きない原因となっていたが、撮像をCCDカメラで行う
ことによりこの問題をも解消できた。
In this embodiment, a Wollaston prism is used as the birefringent prism.
Gran Thomson prism, lotion prism, etc.
It goes without saying that it is only necessary to be able to separate and incline the P-polarized light and the S-polarized light. In addition, it is difficult to remove an error due to a temperature drift in an image pickup tube such as a pidicon or a new vidone, and this also causes a problem in that the resolution cannot be improved. It was resolved.

【0016】本発明の別の実施例としてCCDカメラに
代えてラインセンサの素子ピッチの小さいものを用いる
ことも可能である。その場合、干渉縞をラインセンサ上
に結合する倍率を大きくすることにより分解能を向上さ
せることも可能である。
As another embodiment of the present invention, a line sensor having a small element pitch can be used instead of a CCD camera. In this case, the resolution can be improved by increasing the magnification at which the interference fringes are combined on the line sensor.

【0017】ラインセンサを使用する場合、走査する干
渉縞上の位置が一定になるため、ウォーラストンプリズ
ムや光学系上のウォーラストンプリズムに傷、ごみの付
着等の影響(ノイズ)が出易いが、上記実施例同様に同
じウォーラストンプリズムを含む同じ光学系で予め膜の
ない被測定物に対して行った膜厚測定により得られた基
準干渉縞のみを有する信号波形を、実際の膜厚測定によ
り得られた膜厚干渉縞を有する信号波形から減じること
により、その影響が軽減され、または完全に除去され
る。また、CCDカメラによる平均化処理と同様に複数
本のラインセンサを並べて同時に測定を行い、各出力波
形を平均化することでも上記影響を軽減できる。云うま
でもなく、これらを組み合わせれば一層上記影響を除去
できる。加えて、ラインセンサの走査を、時間をずらし
て複数回行えば、ランダムノイズと固定ノイズとが同時
に除去できる。
When a line sensor is used, the position on the interference fringe to be scanned is constant, so that the Wollaston prism and the Wollaston prism on the optical system are liable to be affected (noise) such as scratches and dust adhesion. In the same manner as in the above embodiment, a signal waveform having only a reference interference fringe obtained by a film thickness measurement performed in advance on a film-free measurement object using the same optical system including the same Wollaston prism is measured by actual film thickness measurement. The influence is reduced or completely eliminated by subtracting from the signal waveform having the film thickness interference fringe obtained by the above. Further, similarly to the averaging process by the CCD camera, the above influence can be reduced by arranging a plurality of line sensors and measuring at the same time, and averaging each output waveform. Needless to say, these effects can be further eliminated by combining them. In addition, if scanning of the line sensor is performed a plurality of times at staggered times, random noise and fixed noise can be simultaneously removed.

【0018】[0018]

【発明の効果】上記した説明により明らかなように、本
発明による干渉膜厚計によれば、予め目的とする膜のな
い状態でその表面から反射したP偏光波面とS偏光波面
との交線にて生じる基準干渉縞の波形を記憶させ、測定
された干渉縞の波形からこの基準干渉縞の波形を減じ、
上面からの反射波面と下面からの反射波面との膜厚干渉
縞のみを基準干渉縞のあった位置の両側に残し、これら
の干渉縞のピーク位置間隔を測定すれば、1μm以下の
薄膜であってもその膜厚を容易に、かつ正確に測定でき
る。このとき、例えばウォーラストンプリズムを用いた
場合、その頂角を小さくして上面からの反射波面同士及
び下面からの反射波面同士の基準干渉縞と、上面及び下
面からの反射波面の膜厚干渉縞との間隔を広げると更に
良い。また、上記複屈折性プリズムに傷、ごみ等があっ
ても上記減算処理によりその影響が軽減され、または完
全に除去される。従って、取扱い、メンテナンスが容易
になり、維持コストが低廉化する。更に、多数のライン
で干渉縞間隔を計測し、これの平均値をとるようにすれ
ば、統計的には100本のラインで計測した場合、σは
1/10になるので1桁精度向上が期待でき、即ち分解
能を向上できる。
As is apparent from the above description, according to the interference film thickness meter according to the present invention, the intersection of the P-polarized wave front and the S-polarized wave front reflected from the surface in the absence of the target film in advance. The waveform of the reference interference fringe generated in is stored, and the waveform of the reference interference fringe is subtracted from the measured interference fringe waveform .
Only the film thickness interference fringes of the reflected wavefront from the upper surface and the reflected wavefront from the lower surface are left on both sides of the position where the reference interference fringes existed, and when the peak position interval of these interference fringes is measured, the thin film is 1 μm or less. However, the thickness can be easily and accurately measured. At this time, for example, when a Wollaston prism is used, the apex angle is reduced and the reference interference fringes between the reflected wavefronts from the upper surface and between the reflected wavefronts from the lower surface, and the thickness interference fringes of the reflected wavefronts from the upper and lower surfaces are reduced. It is even better to increase the distance between them. Further, even if the birefringent prism has a flaw, dust or the like, the influence thereof is reduced or completely removed by the subtraction processing. Accordingly, handling and maintenance are facilitated, and maintenance costs are reduced. Furthermore, if the fringe intervals are measured on a large number of lines and the average value is taken, σ becomes 1/10 statistically when 100 lines are measured. This can be expected, that is, the resolution can be improved.

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

【図1】本発明が適用された干渉膜厚計の光学素子及び
処理ブロックの関係を示す図。
FIG. 1 is a diagram showing a relationship between an optical element and a processing block of an interference film thickness meter to which the present invention is applied.

【図2】CCDカメラの画像イメージを示す図。FIG. 2 is a diagram showing an image image of a CCD camera.

【図3】(a)〜(d)はウォーラストンプリズムによ
り生じた干渉縞を含む像をCCDカメラにより受光した
際の信号波形を処理する手順を示す図。
FIGS. 3A to 3D are diagrams illustrating a procedure for processing a signal waveform when an image including interference fringes generated by a Wollaston prism is received by a CCD camera.

【図4】(a)は従来の干渉膜厚計による膜厚測定の原
理を説明するための図、(b)は従来の干渉膜厚計によ
り薄膜の膜厚を測定した際の問題点を示す(a)と同様
な図。
FIG. 4 (a) is a diagram for explaining the principle of film thickness measurement using a conventional interference film thickness meter, and FIG. 4 (b) shows a problem when a thin film thickness is measured using a conventional interference film thickness meter. The figure similar to (a) shown.

【符号の説明】[Explanation of symbols]

1 投光装置 2 ハーフミラー 3 対物レンズ 4 結像レンズ 5 偏光フィルタ 6 ウォーラストンプリズム 7 偏光フィルタ 8 リレーレンズ 9 CCDカメラ 10 増幅器・フィルタブロック 11 ビデオモニタ 12 画像取り込みブロック 13 コンピュータ DESCRIPTION OF SYMBOLS 1 Projector 2 Half mirror 3 Objective lens 4 Imaging lens 5 Polarizing filter 6 Wollaston prism 7 Polarizing filter 8 Relay lens 9 CCD camera 10 Amplifier / filter block 11 Video monitor 12 Image capturing block 13 Computer

Claims (1)

(57)【特許請求の範囲】(57) [Claims] 【請求項1】 基板上に直接若しくは別の膜を介して
形成された膜に照明光を照射し、該膜の上面及び下面か
らの反射光を複屈折性プリズムによりP偏光波とS偏光
波とに分け、それぞれ別方向に傾けて、それらの波面の
交線にて生じる膜厚干渉縞の間隔を計測して膜厚を測定
する干渉膜厚計に於て、予め前記目的の膜のない状態でその表面から反射したP
偏光波面とS偏光波面との交線にて生じる 基準干渉縞の
みの波形を記憶する手段と、 受光手段にて前記膜厚干渉縞を含む像を結像させ、前記
基準干渉縞の波形を前記受光手段にて結像させた像の干
渉縞波形から減じる手段と、 前記基準干渉縞の波形を減じた後の一対の干渉縞の波形
のピーク位置の間隔から前記膜の膜厚を求める手段とを
有することを特徴とする干渉膜厚計。
An illumination light is applied to a film formed directly on a substrate or through another film, and reflected light from the upper and lower surfaces of the film is converted into a P-polarized wave and an S-polarized wave by a birefringent prism. In the interference film thickness meter for measuring the film thickness by measuring the interval of the film thickness interference fringes generated at the intersection of their wavefronts by tilting them in different directions, the target film is not included in advance. P reflected from the surface in the state
Means for storing only the waveform of the reference interference fringes generated at the intersection of the polarization wavefront and the S-polarization wavefront; and forming an image including the film thickness interference fringes by a light receiving means, and changing the waveform of the reference interference fringes to Means for subtracting from the interference fringe waveform of the image formed by the light receiving means, and means for determining the film thickness of the film from the interval between the peak positions of the pair of interference fringe waveforms after subtracting the waveform of the reference interference fringe. An interference film thickness meter comprising:
JP24858294A 1994-09-16 1994-09-16 Interference film thickness meter Expired - Fee Related JP2875746B2 (en)

Priority Applications (1)

Application Number Priority Date Filing Date Title
JP24858294A JP2875746B2 (en) 1994-09-16 1994-09-16 Interference film thickness meter

Applications Claiming Priority (1)

Application Number Priority Date Filing Date Title
JP24858294A JP2875746B2 (en) 1994-09-16 1994-09-16 Interference film thickness meter

Publications (2)

Publication Number Publication Date
JPH0886619A JPH0886619A (en) 1996-04-02
JP2875746B2 true JP2875746B2 (en) 1999-03-31

Family

ID=17180274

Family Applications (1)

Application Number Title Priority Date Filing Date
JP24858294A Expired - Fee Related JP2875746B2 (en) 1994-09-16 1994-09-16 Interference film thickness meter

Country Status (1)

Country Link
JP (1) JP2875746B2 (en)

Families Citing this family (1)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
JP4833662B2 (en) * 2005-12-28 2011-12-07 株式会社ミツトヨ Non-contact displacement measuring device, edge detection method thereof, and edge detection program

Also Published As

Publication number Publication date
JPH0886619A (en) 1996-04-02

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