AU741101B2 - A method for retrieving data stored on a medium - Google Patents

Description

Regulation 3.2

AUSTRALIA

Patents Act 1990 COMPLETE SPECIFICATION FOR A STANDARD PATENT

(ORIGINAL)

Name of Applicant: DISCOVISION ASSOCIATES of 2355 Main Street, Suite 200, Irvine, California 92714, United States of America Actual Inventor(s): Address for Service: DAVIES COLLISON CAVE, Patent Attorneys, of 1 Little Collins Street, Melbourne, Victoria 3000, Australia "A METHOD FOR RETRIEVING DATA STORED ON A MEDIUM" Invention Title: The following statement is a full description of this invention, including the best method of performing it known to us: -1 P;\OPER\DBW\17835-95.DV3 30/4/99 2 The present invention relates to a method for detecting transitions in an input signal having a DC component and a method for retrieving data stored on a medium.

Various types of recordable and/or erasable media have been used for many years for data storage purposes. Such media may include, for example, magnetic tapes or disks in systems having a variety of configurations.

Magneto-optical systems exist for recording data on and retrieving data from a magnetic disk. The process of recording in a magneto-optical system typically involves use of a magnetic field to orient the polarity of a generalized 25 area on the disk while a laser pulse heats a localized area, thereby fixing the polarity of the localized area. The localized area with fixed polarity is commonly called a pit.

Some encoding systems use the existence or absence of a pit on the disk to define the recorded data as a or 30 respectively.

When recording data, a binary input data sequence may be converted by digital modulation to a different binary sequence having more desirable properties. A modulator may, for 35 example, convert m data bits to a code word with n modulation o code bits (or "binits"). In most cases, there are more code bits than data bits m n.

0 I P;\OPER\DBW\17835-95.DV3 30/4/99 3 Most if not all disk drive systems use run-length-limited modulation codes, such as RLL 2/7/1/2 or RLL 1/7/2/3 codes. Another family of modulation codes are group-coded recording codes, such as GCR 0/11/8/9 or GCR 0/3/8/9 codes (sometimes abbreviated as GCR The numbers appended to the names of particular codes typically refer to certain encoding constraints, such the relationship between bits and flux reversals, or the minimum and maximum number of contiguous binits possible without flux transitions. For example, a commonly used encoding system for pit-type recording is the RLL 2/7/1/2 code which constrains the recorded information to have a minimum of two and a maximum of seven zeroes between ones. In general, RLL recording provides a relatively high data-to-pit ratio but may not, however, in many circumstances allow for high data storage densities because amplitude and timing margins deteriorate very rapidly as frequency is increased.

A GCR 0/3/8/9 code, on the other hand, not only requires nine flux reversals for every eight data bits but further requires a minimum of no zeroes and a maximum of three zeroes between ones.

The density ratio of a given recording system is often r expressed according to the equation x (d where m *and n have the definitions provided above, and d is defined as the minimum number of zeroes occurring between ones. Thus, the RLL 2/7/1/2 code has, according to the above equation, a density ratio of 1.5, while the GCR 0/3/8/9 code has a density ratio of 0.89.

For reading data in an MO system, a focused laser beam or other optical device is typically directed at the recording surface of a rotating optical disk such that the laser beam can selectively access one of a plurality of tracks on the recorded surface. The rotation of the laser beam reflected from the recorded surface may be detected by means of Kerr P:\OPERXRAB\2171610 st ORdo-13 Sepmbr, 2001 -4rotation. A change in Kerr rotation of a first type, for example, represents a first binary value. A change in Kerr rotation of a second type represents a second binary value. An output signal is generated from the first and second binary values occurring at specified clock intervals.

Although there has been a continual demand for disk systems capable of storing increasingly higher data densities, the ability to achieve high data storage densities has met with several limitations. As a general matter, the reasonable upper limit for data density is determined in part by reliability requirements, the optical wavelength of the laser diode, the quality of the optical module, hardware cost, and operating speed. Maximum data densities are also affected by the ability to reject various forms of noise, interference, and distortion. For example, the denser that data is packed, the more intersymbol interference •go• will prevent accurate recovery of data. Moreover, because the technology for many S.o intermediate and high performance optical disk drives has been limited by downward compatibility constraints to older models, signal processing techniques have not advanced as rapidly as they might otherwise have.

When attempting to recover stored data, existing read channels of magneto-optical and other types of disk drives commonly suffer from a number of problems due to the 20 unintended buildup of DC components in the read signal. One cause of DC buildup results ifrom the recording of unsymmetrical data patterns over a number of bytes or data segments. A symmetrical data pattern may be considered as one having an average DC component of zero over a region of interest. Because sequences of recorded bits may be essentially random in many modulation codes, however, localized regions of recorded data having particular patterns of l's and O's will produce an unsymmetrical read signal having unwanted DC components. Because the data patterns vary over time, the level of DC buildup will also vary, causing P:\OPER\DBW\17835-95.DV3 30/4/99 5 wander of the DC baseline, reduction of threshold detection margins, and greater susceptibility to noise and other interference.

Undesired DC buildup is also caused by variance in pit size due to thermal effects on the writing laser or the storage medium. As the writing laser heats up, for example, the spot size may increase leading to wider pits. When the recorded pits are read, variations in pit size will cause an unsymmetrical input signal having DC components. Variation in pit size not only causes undesired DC buildup but also causes the relative locations of the data to appear shifted in time, reducing the timing margin and leading to possible reading errors.

Various attempts have been made to overcome the described problems. For example, various tape drive systems commonly use a DC-free code such as a 0/3/8/10 code, otherwise referred to simply as an 8/10 code. Because an 8/10 code requires stored bits to yield 8 data bits, however, it is only efficient which is a drawback when attempting to record high data densities.

eoeoe: Another method for handling DC buildup involves the use 25 of double differentiation. This method typically involves detection of the peaks of a first derivative of the input signal by detecting zero-crossings of the second derivative of the input signal. Thus, the DC components are effectively filtered out. One drawback of this method is that differentiation or double differentiation can cause undesirable noise effects. A second drawback is that the method may decrease the timing margin to unacceptably low levels by as much as 50 percent).

In another method for addressing DC buildup, the data to be stored is randomized prior to recording such that none of the data patterns repeat over a data sector. However, this P:\OPER\RABU]71610 1I OR.doc-13 Sopt-eb 2(X -6method may not acceptable by ISO standards and may lack downward compatibility with previous disk drive systems. As a further drawback to this method, de-randomizing the data may be complex.

Yet another method for controlling DC buildup involves the use of so-called resync bytes between data segments. This method generally involves the examination and manipulation of data before it is recorded in order to minimize DC buildup upon readback.

Before recording, two consecutive data segments are examined to determine if the patterns of l's and O's are such as to cause positive DC, negative DC, or no DC components when read back. If, for example, two consecutive data segments have the same DC polarity, one of the data segments is inverted prior to being recorded on the medium. In order to stay oo •within the constraints of the particular encoding system, however, a resync byte between the segments may need to be written so that the pattern of contiguous bits and of flux reversals is proper. A drawback of such a method is that it will not necessarily reduce all DC buildup, and time constants must be determined such that the predictable DC buildup °will not affect performance. Further, the method requires additional overhead including the examination of data segments to determine their relative polarity.

It would therefore be advantageous to have a method and system for reading stored S 20 data from a medium and a method and system for detecting transitions in an input signal i having a DC component without suffering the undesirable effects of DC buildup, without creating unacceptable levels of noise or significantly reducing timing margins, without the requirement of large amounts of overhead or de-randomizing algorithms, and while providing high data storage efficiency, or at least provide a useful alternative.

In accordance with the present invention there is provided a method for detecting transitions in an input signal having a DC component, said method comprising the steps of: generating a threshold signal from said input signal; P:\OPER\DBW\17835-9S.DV3 30/4/99 7 comparing said input signal to said threshold signal to thereby generate an output signal; and adjusting said threshold signal in response to said output signal.

The present invention also provides a method for retrieving data stored on a medium, said method comprising the steps of: reading said stored data to thereby generate a playback signal; partially integrating said playback signal; generating a threshold signal which varies with a DC component of said partially integrated signal; and generating an output signal indicative of said stored data by comparing said partially integrated signal with said threshold signal.

The present invention also provides a method for retrieving data stored on a medium, said method comprising the steps of: reading the stored data to thereby generate a signal; partially integrating said signal; 5oo555 generating a threshold signal corresponding to an approximate midpoint of said partially integrated signal; and 25 generating an output signal indicative of said stored S"data by comparing said partially integrated signal with said threshold signal.

A preferred embodiment of the present invention is hereinafter described, by way of example only, with reference to the accompanying drawings, wherein: FIG. 1 is a block diagram showing an optical data storage and retrieval system; FIG. 2 is a series of sample waveforms associated with a GCR format; FIGS. 3A and 3B are waveform diagrams of a symmetrical and unsymmetrical input signal, respectively; P;\OPER\DBW\17835-95.DV3 30/4/99 -8- FIG. 4 is a block diagram of a read channel; FIG. 5A is a more detailed block diagram of various stages of a read channel; FIG. 5B(i) is a block diagram of the relationship between FIGS. 5B(ii) and FIGS. 5B(ii) and 5B(iii) form a circuit diagram of a partial integrator stage; FIGS. 6A-6E are frequency response diagrams of various stages of a read channel; FIG. 6F is a plot of group delay for a combination of stages in a read channel; FIG. 6G is a waveform diagram showing signal waveforms at various stages in the read channel; FIG. 7 is a block diagram of a peak detection and tracking circuit; FIG. 8 is a schematic diagram of the peak detection and tracking circuit of FIG. 7; FIG. 9 is a waveform diagram showing tracking by a threshold signal of the DC envelope of an input signal; FIGS. 10A-10D are diagrams showing exemplary waveforms at various points in a read channel; FIG. 11 is a series of waveforms showing uniform laser "pulsing under a pulsed GCR format and non-uniform laser pulsing under an RLL 2,7 format; 25 FIG. 12 is a series of waveforms showing laser pulsing S"for various data patterns adjusted by the write compensation circuit; FIG. 13 is a schematic diagram showing the write compensation circuit; FIG. 14 is a series of waveforms showing laser pulsing for amplitude asymmetry correction; and FIG. 15 is a schematic block diagram of an optical data storage and retrieval system incorporating downward compatibility.

Although the present invention is applicable to many different data storage and retrieval systems, the following P:\OPER\DBW\17835-95.DV3 30/4/99 9description of the preferred embodiment will focus primarily on magneto-optical systems. In so doing, there is no intent to limit the scope of the invention solely to devices which are magneto-optical in nature.

A block diagram of an exemplary magneto-optical system is shown in Fig. 1. The system may have a read mode and a write mode. During the write mode, a data source 10 transmits data to an encoder 12. The encoder 12 converts the data into binary code bits. The binary code bits are transmitted to a laser pulse generator 14, where the code bits may be converted to energizing pulses for turning a laser 16 on and off. In one embodiment, for example, a code bit of indicates that the laser will be pulsed on for a fixed duration independent of the code bit pattern, while a code bit of indicates that the laser will not be pulsed at that interval. Depending on the particular laser and type of optical medium being used, performance may be enhanced by adjusting the relative occurrence of the laser pulse or extending the otherwise uniform pulse duration. In response to being pulsed, the laser 16 heats localized areas of an optical medium 18, thereby S"exposing the localized areas of the optical medium 18 to a S"magnetic flux that fixes the polarity of the magnetic material on the optical medium 18. The localized areas, commonly called o* e 25 "pits", store the encoded data in magnetic form until erased.

During the read mode, a laser beam or other light source "is reflected off the surface of the optical medium 18. The reflected laser beam has a polarization dependent upon the polarity of the magnetic surface of the optical medium 18. The reflected laser beam is provided to an optical reader which sends an input signal or read signal to a waveform processor 22 for conditioning the input signal and recovering the encoded data. The output of the waveform processor 22 may be provided to a decoder 24. The decoder 24 translates the encoded data back to its original form and sends the decoded data to a data output port 26 for transmission or other 0 P:\OPER\DBW\17835-95.DV3 30/4/99 10 processing as desired.

Figure 2 depicts in more detail the process of data storage and retrieval using a GCR 8/9 code format. For a GCR 8/9 code, a cell 28 is defined as one channel bit. Each clock period 42 corresponds to a channel bit; thus, cells 30 through 41 each correspond to one clock period 42 of clock waveform As an example of clock speeds, for a optical disk rotating at 2,400 revolutions per minute with a storage capacity of 256 Mbytes, clock period 42 will typically be 63 nanoseconds or a clock frequency of 15.879 Mhz. GCR input waveform 47 is the encoded data output from the encoder 12 (see Fig. The GCR input waveform 47 corresponds to a representative channel sequence "010001110101". The laser pulse generator 14 uses the GCR data waveform 47 to derive the pulse GCR waveform 65 (which in Figure 2 has not been adjusted in time or duration to reflect performance enhancement for specific data patterns). Generally, the GCR pulses 67 through 78 occur at clock periods when the GCR data waveform 47 is high. The pulse GCR waveform 65 is provided to the laser 16.

The magnetization of the optical medium reverses polarity as the laser is pulsed on and off by utilizing a non- "return-to-zero ("NRZII) driving signal to energize a magnetic recording head). The laser pulses resulting from GCR pulses 68, 69, 70, etc., create a pattern of recorded pits 80 on optical medium 18. Thus, recorded pits 82 through 88 correspond to pulses 68, 69, 70, 71, 73, 76, and 77, respectively.

Successive recorded pits 82 through 85 may merge together to effectively create an elongated pit. The elongated pit has a leading edge corresponding to the leading edge of the first recorded pit 82 and a trailing edge corresponding to the trailing edge of last recorded pit Reading the recorded pits with an optical device such as a laser results in the generation of a playback signal 90. The

C,

P:\OPER\DBW\17835-95.DV3 30/4/99 11 playback signal 90 is low in the absence of any recorded pits.

At the leading edge of a pit 86, playback signal 90 will rise and remain high until the trailing edge of the pit 86 is reached, at which point the playback signal 90 will decay and remain low until the next pit 87.

The above described process may be referred to as pulse width modulation because the width of the pulses in playback signal 90 indicate the distance between 1-bits. Thus, the edges of the recorded pits 80 which define the length of the pulses in playback signal 90 contain the pertinent data information. If the playback signal is differentiated, the signal peaks 111 through 116 of the first derivative signal 110 will correspond to the edges of the recorded pits 80. (The signal peaks of the first derivative playback signal 110 in Fig. 2 are shown slightly offset from the edges of the recorded pits 80 because an ideal playback signal 90 is shown). In order to recover the pit edge information from the first derivative signal 110, it is necessary to detect the signal peaks 111 through 116. Such a process is described in detail further herein.

i. "In contrast, most if not all existing RLL 2/7 code systems are used in conjunction with pulse position modulation In PPM systems, each pit represents a while the absence of a pit represents a The distance between pits represents the distance between 1-bits. The center of each pit corresponds to the location of the data. In order to find the pit centers, the playback signal is differentiated and the 30 zero-crossings of the first derivative are detected. Such a technique may be contrasted with PWM systems, described above, in which the signal peaks of the first derivative contain the pertinent pulse width information.

It is nevertheless possible to utilize PWM instead of PPM with an RLL system such as an RLL 2/7 code system. Each channel bit may correspond to a clock period of a clock P:\OPER\DBW\17835-95.DV3 30/4/99 12 waveform. As with the GCR system described earlier using PWM, a may be represented by a transition in the input waveform. Thus, the RLL 2/7 input waveform may remain in the same state while a occurs, but changes from high-to-low or low-to-high when a occurs.

In both RLL and GCR codes, as well as other codes, when data patterns are read, the input signal generated from the optical reader 20 is often not symmetrical. When an unsymmetrical signal is AC-coupled between circuits, the average DC value shifts away from the peak-to-peak midpoint.

The unintended shifting away from the midpoint may result in a shift in the apparent position of the data, adversely affect the ability to determine accurately the locations of data, and reduce timing margins or render the recorded data unrecoverable.

This phenomenon may be explained with reference to Figs.

3A and 3B. Figure 3A shows an ideal input signal S, derived from a symmetrical data pattern. Normally, transitions between 1's and O's in the data are detected at the midpoint between high and low peaks of the input signal. It may be observed in Fig. 3A that the areas A, and A 2 above and below the peak-topeak midpoint Mp, of the input signal S, are equal, and the transitions between 1's and O's correspond precisely (in an ideal system) to the crossings of the input, signal S, and the peak-to-peak midpoint Figure 3B, in contrast, shows an input signal S 2 derived from an unsymmetrical data pattern. It may be observed that the area A above the peak-to-peak midpoint MP2 is greater than the are A 2 below the graph. The input signal S 2 therefore has a DC component that shifts the DC baseline DCBASE above the peak-to-peak midpoint MP 2 When an attempt is made to locate transitions between 1's and O's by determining the zero-crossings of the input signal S 2 errors may be made because the DC level is not identical to the peak-to-peak P:\OPER\DBW\17835-95.DV3 30/4/99 13 midpoint MP 2 The DC level does not stay constant but rises and falls depending on the nature of the input signal. The larger the DC buildup, the more the detected transitions will stray from the true transition points. Thus, DC buildup can cause timing margins to shrink or the data to be unrecoverable.

Fig. 4 is a block diagram of a read channel 200 in accordance with one embodiment of the present invention for mitigating the effects of DC buildup. The read channel 200 roughly corresponds to the waveform processor 22 of Fig. i.

The read channel 200 comprises a pre-amplification stage 202, a differentiation stage 204, an equalization stage 206, a partial integration stage 208, and a data generation stage 210. The operation of the read channel 200 will be explained with reference to a more detailed block diagram shown in Fig.

the waveform diagrams shown in Figs. 10A-10D, and various other figures as will be referenced from time to time herein.

When the optical medium is scanned for data, the preamplification stage 202 amplifies the input signal to an appropriate level. The pre-amplification stage 202 may S"comprise a pre-amplifier 203 as is well known in the art. The eeo.

pre-amplifier 203 may alternatively be located elsewhere such as within the optical reader 20. An exemplary amplified Splayback signal 220 is depicted in Fig. The output of the pre-amplification stage 202, as shown in Fig. 5A, is provided to the differentiation stage 204. The 30 differentiation stage 204 may comprise a differential amplifier 212 such as a video differential amplifier configured with a capacitor 213 in a manner well known in the art. A representative frequency response diagram of the differentiation stage 204 is shown in Fig. 6A. The differentiation stage 204 effectively increases the relative magnitudes of the high frequency components of the amplified playback signal 220. An exemplary waveform of the output of P:\OPER\DBW\17835-95.DV3 30/4/99 14 the differentiation stage 204 is shown in Fig. The differentiation stage 204 is followed by an equalization stage 206 as shown in Fig. 5A. The equalization stage 206 provides additional filtering so as to modify the overall channel transfer function and provide more reliable data detection. The equalization stage 206 shapes the differentiated input signal so as to even out the amplitudes of high and low frequency components and generate a smoother signal for later processing. Equalizing filters often modify the noise spectrum as well as the signal. Thus, an improvement in the shape of the differentiated input signal a reduction in distortion) is usually accompanied by a degradation in the signal-to-noise ratio. Consequently, design of the equalization stage 206 involves a compromise between attempting to minimize noise and providing a distortion-free signal at an acceptable hardware cost. In general, equalizer design depends on the amount of intersymbol interference to be compensated, the modulation code, the data recovery technique to be used, the signal-to-noise ratio, and the noise spectrum shape.

"A substantial portion of linear intersymbol interference 00.0 when reading stored data in a magneto-optical recording system is caused by limited bandwidth of the analog read channel and S"roll-off of input signal amplitude with increased storage density. Accordingly, the equalization stage 206 may comprise one or more linear filters which modify the read channel "transfer function so as to provide more reliable data detection. Normally, the equalization stage is implemented as OOe part of the read channel, but, under certain conditions, part of the equalization filtering can be implemented as part of *..the write channel as well.

For purposes of analysis, the playback signal can be considered as a series of bipolar rectangular pulses having unit amplitude and a duration T. Alternatively, the playback P:\OPER\DBW\17835-95.DV3 30/4/99 15 signal may be considered as a series of bidirectional step functions at each flux reversal location, where the step amplitude matches the pulse amplitude. When an input signal is applied to the equalization stage 206, clocking information as well as pulse polarity for each clock cell or binit may be derived from the output signal of the equalization stage 206.

The clocking and polarity information may be derived, in theory, by use of an ideal waveform restoration equalizer, which produces an output signal having mid-binit and binit boundary values similar to those of the input signal. The zero crossings of the output signal occur at binit boundaries in order to regenerate a clock accurately. If the zero-crossing time and direction are known, both clock and data can be extracted from the signal zero crossings.

In one embodiment, the equalization stage 206 comprises an equalizer selected from a class of waveform restoration equalizers. Generally, a waveform restoration equalizer generates a signal comprising a binary sequence resembling the input or playback waveform. The corners of the otherwise rectangular pulses of the resultant signal are rounded because signal harmonics are attenuated in the channel. The resultant oooeo signal may also exhibit some output signal amplitude variation.

*go* S"An equalizer which produces a minimum bandwidth output signal is an ideal low pass filter with response of unity to the minimum cutoff frequency and no response at higher frequencies. Although such an ideal low pass filter is not physically realizable, the Nyquist theorem on vestigial 9...i symmetry suggests that the sharp cutoff minimum bandwidth filter can be modified and still retain output pulse zero crossing at all mid-binit cell times. To achieve this result, the high frequency roll-off of the equalized channel is preferably symmetrical and locates the half-amplitude point at the minimum bandwidth filter cutoff frequency.

P:\OPER\DBW\17835-95.DV3 30/4/99 16 One type of roll-off characteristic that may be exhibited by a filter in the equalization stage 206 is a raised cosine roll-off, leading to the name raised cosine equalizer. A raised cosine roll-off transfer function is approximately realizable, and has an improved response over the minimum bandwidth filter. The output pulses have a zero value at times nT, but the sidelobe damped oscillation amplitude is reduced.

The output zero crossings of the raised cosine filter are more consistent than those of the minimum bandwidth filter, and linear phase characteristics are more easily achieved with a gradual roll-off, such as with the relatively gradual roll-off of the raised cosine filter. These advantages, however, are typically obtained at the expense of increased bandwidth. The ratio of bandwidth extension to the minimum bandwidth, fm, is sometimes referred to as the of the raised cosine channel.

Thus, in the case of a modulation code with d 0, a 0 is the minimum bandwidth but represents an unrealizable rectangular transfer function, while a 1 represents a filter using twice the minimum bandwidth.

The impulse transfer function of the raised cosine equalization channel (including the analog channel plus equalizer, but excluding the input filter) may be given as follows: H(f) 1, for 0 f (1 a) fm H(f) 1/2 {1 cos (1 a) fm)/(2 a f for (1 a) fm f (1 a) fm H(f) 0, for f (1 a) fm where E(f) k f is the phase, and k is a constant. The above family may be referred to as a waveform restoration equalizers. The a 1 channel has the property of having nulls at half-binit intervals as well as at full binit intervals.

Such a channel results in a signal having no intersymbol P:\OPER\DBW\17835-95.DV3 30/4/99 17 interference at mid-binit or binit boundary times, which are signal zero crossing and sample times, thus allowing accurate clock and data recovery. For such a full bandwidth equalizer, the roll-off starts at zero frequency and extends to the cutoff frequency fc- Raised cosine equalizers are capable of correcting extensive amounts of linear intersymbol interference given adequate signal-to-noise ratio. A large amount of high frequency boost is usually required to compensate for MO-media loss and optical short wavelength low resolution. An equalizer bandwidth equal to at least twice the minimum bandwidth is preferred for elimination of linear intersymbol interference, assuming a physically realizable channel operating on a modulation code with d 0. A bandwidth of such a width generally results in reduction of the signal-to-noise ratio.

The equalizer bandwidth is selected so as to achieve the optimum compromise between interference distortion and noise.

In some instances, it may be desirable to narrow the bandwidth by using an a 1 transfer function in order to improve noise at the expense of added distortion in the form of clock ooooo S•jitter.

Another waveform-restoration equalizer is known as the ee S" 25 cosine 3 response equalizer. The impulse transfer function of a full bandwidth f channel is as follows: H(f) coso for 0 f fc H(f) 0 for f fc Like the a equalizer family, there are numerous f equalizers.

Full bandwidth 3 equalizers have a cutoff frequency of fc, and consequently reduce clock jitter due to the relatively small amount of interference at binit boundaries. Techniques are known in the art for optimizing these types of equalizing filters to achieve the minimum probability of error in various P:\OPER\DBW\17835-95.DV3 30/4/99 18 types of noise conditions.

Use of a equalizers generally results in a narrower bandwidth, thereby reducing noise at the expense of clock jitter or horizontal eye opening. Use of a equalizer generally results in signal-to-noise ratio improvement by reducing high frequency boost without reducing the bandwidth.

The choice of 3 equalizer may reduce the vertical eye opening or an effective amplitude reduction. The a 1 and 2 equalizer channels are identical from the standpoint of eye pattern, both types of channels having a relatively wide open eye pattern.

A preferred equalizer channel bandwidth for codes with d 0 does not necessarily depend on the minimum recorded pulse width, Tr, as might be expected, but rather on the binit width, Tm. This is because the data-recovery circuits are generally required to distinguish between pulses that differ by as little as one binit width, and time resolution is a function of signal bandwidth. The codes (where k represents the maximum number of contiguous binits without flux reversals) require a nominal bandwidth BWNOM 1/Tm fc so as to eliminate interference at the center and edge of each binit, provided that intersymbol interference at binit S" 25 boundaries is absent.

For codes with d 0, interference can be essentially "eliminated at binit edges with a reduced bandwidth of BW 1/ (2*Tm) fc/2. In such a case, all binit read pulses then have unit amplitude at a flux reversal, and the read-pulse tails cross zero at flux transitions. The narrower bandwidth BW results in output signal zero crossings at a point of no *...interference, without considering binit centers, but the bandwidth reduction is typically obtained with an increase in detection ambiguity in the presence of channel impairments.

The narrower bandwidth BW may also result in a reduction of the signal zero-crossing slope, leading to a potential P:\OPER\DBW\17835-95.DV3 30/4/99 19 increase in detection sensitivity with respect to noise, disk speed variations, analog channel differences, or improper equalization. For example, a half-bandwidth 2 equalization channel with a (1,k)2/3 rate modulation code may result in a signal having no intersymbol interference at the signal zero crossings, but some amplitude variation between zero crossings. The bandwidth is less than the bandwidth for nonreturn to zero ("NRZI") modulation, even though more information is recorded than with NRZI modulation bandwidth 0.75 and bit rate 1.33 relative to NRZI). The reduced bandwidth makes up for the modulation code rate loss.

The a 1 and P waveform restoration equalizers may permit output zero crossings to occur at the equivalent of input pulse edges. Data detection can then be obtained by hard-limiting the equalized signal, generally resulting in an output signal resembling the original playback signal.

However, this result occurs only if the equalizer response extends to DC, which is typically not the case for a magnetooptical channel. Low frequency loss in the MO channel causes drift up and down of the DC baseline, resulting in output •binits which are lengthened or shortened according to the degree of amplitude offset at zero-crossing detector. This problem can be reduced by the use of either a DC-free S" 25 modulation code or, preferably, DC restoration as described herein. In order to achieve the desired low frequency response for a waveform-restoration equalizer, the low frequency signals may have to be amplified significantly, which can seriously degrade signal-to-noise ratio under some conditions.

If low frequency noise is present in significant amounts, waveform-restoration equalization techniques may not be very satisfactory unless a modulation code with no DC and little low-frequency content or DC restoration circuits are used.

In a preferred embodiment, the equalization stage 206 may comprise a programmable filter and equalizer 207 located on an integrated chip. Such integrated chips are presently available P:\OPER\DBW\17835-95.DV3 30/4/99 20 from various manufacturers. The filter and equalizer 207 may be of an equi-ripple variety and have relatively constant group delay up to a frequency equal to about twice the cutoff frequency. A representative frequency response diagram of the equalization stage 204 is shown in Fig. 6B, and an exemplary output waveform is shown in Fig. After the signal has been processed by the equalization stage 206, the signal peaks of the waveform in Fig. contain accurate information regarding the position of the read data. The signal peaks can be detected by taking another derivative, but doing so may be detrimental to the system's signal-to-noise ratio and will likely cause undesired jitter.

A preferred embodiment of the invention described herein provides an accurate means for detecting the signal peaks without taking a second derivative, by using partial integration and a novel data generation circuit.

After the signal has been processed by the equalization stage 206, it is provided to a partial integrator stage 208 for further shaping of the waveform. As illustrated in Fig.

5A, the partial integrator stage 208 may comprise an amplifier stage 229, a bandpass filter stage 230, an integrator and low pass filter stage 232, and a subtracter and low pass filter S" 25 stage 234. The amplifier stage 229 receives the output of the equalization stage 206 and provides a signal to the bandpass filter stage 230 and the integrator and low pass filter stage 232. The integrator and low pass filter stage 232 preferably attenuates a selected range of high frequency components. A representative frequency response 260 of the integrator and low pass filter stage 232 and a representative frequency response 261 of the bandpass filter stage 230 are depicted in Fig. 6C.

The output of the bandpass filter stage 230 is thereafter subtracted from the output of the integrator and low pass filter stage 232 and filtered by the low pass filter stage P\OPER\RABU171610 Is ORdoc-13 Seplember, 200! -21 234. A graph of the total frequency response of the partial integrator stage 208, including the low pass filter 234, is shown in Fig. 6D. An exemplary output waveform of the partial integrator stage 208 is shown in Fig. 10 OD.

A detailed circuit diagram of a particular embodiment of a partial integrator stage is illustrated in Fig. 5B. In Fig. 5B, a differential input 238, 239 is received, such as from the equalization stage 206. The differential input 238, 239 is provided to differential amplifier 240, configured as shown, which differentially sums its inputs. Differential amplifier 240 essentially corresponds to amplifier stage 229 shown in Fig. An output 249 from the differential amplifier 240 is connected to a pair of current generators 241 and 242. The first current generator 241 comprises a resistor R77 and a ooo* ,,PNP transistor Q61, configured as shown in Fig. 5B. The second current generator 242 oo also comprises a resistor R78 and a PNP transistor Q11, configured as shown in Fig. An output from current generator 241 is connected to a bandpass filter 243. The bandpass filter 243 comprises an inductor L3, a capacitor C72 and a resistor configured in parallel as shown in Fig. 5B. The bandpass filter 243 essentially corresponds to bandpass filter stage 230 of Fig. 5. An output from the other current generator 242 is connected to an integrator 244. The integrator 244 comprises a capacitor C81 and a resistor R66, configured in parallel as shown in Fig. An output from the integrator 244 is connected through a resistor R55 to a NPN transistor Q31. Transistor Q31 is configured as an emitter-follower, providing isolation with respect to the output of the integrator 244, and acting as a voltage source. The emitter of transistor Q31 is connected to a low pass filter 245. The low pass filter 245 comprises an P:\OPER\AB\2 171610 Is[ OR.dc-13 September, 2001 -22inductor L6, a capacitor C66 and a resistor R49, configured as shown in Fig. 5B. The integrator 244, emitter-follower including transistor Q31, and low pass filter 245 essentially correspond to the integrator and low pass filter stage 232 shown in Fig. 5A. The frequency response of the integrator 244 essentially corresponds to the frequency response 260 shown in Fig. 6C, while the frequency response of the low pass filter 245 essentially corresponds to the frequency response 261 shown in Fig. 6C.

An output from the low pass filter 245 and an output from the bandpass filter 243 are coupled to a differential amplifier 246, configured as shown in Fig. 5B. Differential amplifier 246 differentially sums its inputs, and provides a differential output to another low pass filter 247. The differential amplifier 246 and low pass filter 247 correspond essentially to the subtractor and low pass filter stage 234 shown in Fig. Exemplary waveforms for the circuit of Fig. 5B are shown in Fig. 6G. Figure 6G shows first an exemplary input waveform 256 as may be provided to differential amplifier 240 from, equalizer 206. The next waveform 257 in Fig. 6G corresponds to an output from the bandpass filter 243 in response to the Fig. 5B circuit receiving input waveform 256. The next waveform 258 in Fig. 6G corresponds to an output from the low pass filter 245 in response to the Fig. 5B circuit receiving input waveform 256. Waveform 258 shows the effect of operation of the integrator 244. The function of low pass filter 245 is essentially to provide a delay so as to align the output of the bandpass filter 243 and the integrator 244 in time at the input of differential amplifier 246. Low pass filter 245 thereby matches the delays along each input leg of the differential amplifier 246 prior to differential summing.

The final waveform 259 in Fig. 6G corresponds to an output from the second low pass filter 247, after the signals PAOPERNRABU171610 [M ORd-13 Sqnsmbe, 2001 23 output from the bandpass filter 243 and low pass filter 245 have been combined and filtered. Waveform 259 typically exhibits considerably improved resolution over the original playback signal read from the magnetic medium.

It should be noted that the partial integration functions described with respect to Figs. 5A and 5B are carried out using differential amplifiers differential amplifiers 240 and 246), thereby providing common mode rejection or, equivalently, rejection of the DC component of the input signal 238, 239. Another feature of the embodiments shown in Figs. 5A and 5B is the relatively favorable frequency response characteristics exhibited by the partial integration stage. In particular, by combining an integrated signal with a high pass filtered signal at subtractor and low pass filter block 214 or differential amplifier 246), noise is removed from the differentiated and equalized playback signal, but while maintaining relatively rapid response time due in part to the high pass frequency boost .iprovided by the bandpass filter.

A primary function of the combination of the differentiation stage 204, the equalization stage 206, and the partial integration stage 208 is to shape the playback signal 220 in an appropriate manner for facilitating data recovery. As can be seen by comparing Figs. 10 OA and 10 OD, the resultant signal shown in Fig. 10 OD is similar to the playback signal S 20 220 of Fig. 10A (from which it was derived) but differs therefrom in that the amplitudes of its high and low frequency components have been equalized and sharp noise-like characteristics removed. A graph of the total frequency response for the combination of the differentiation stage 204, the equalization stage 206, and the partial integration stage 208 is shown in Fig. 6E. A graph of the total group delay response for the same chain of elements is shown in Fig. 6F.

It may be noted that tape drive systems presently exist utilizing equalization and integration of a playback signal in P:\OPER\DBW\17835-95.DV3 30/4/99 24 order to facilitate data recovery. However, to a large degree such systems do not suffer from the problems of DC buildup because they typically utilize DC-free codes. As mentioned previously, DC-free codes have the disadvantage of being relatively low in density ratio and henceinefficient. The present invention in various embodiments allows for the use of more efficient coding systems by providing means for eliminating the effects of DC buildup without necessarily using a DC-free code.

The output of the partial integrator stage 208 the waveform in Fig. 10D) is provided to a data generation stage 210. A block diagram of the data generation stage 210 is shown in FIG. 7. The data generation stage 210 comprises a positive peak detector 300, a negative peak detector 302, a voltage divider 304, a comparator 306, and a dual edge circuit 308.

The operation of the circuit show in FIG. 7 may be explained with reference to Fig. 9. In Fig. 9, it is assumed that a recorded bit sequence 320 has been read and eventually caused to be generated, in the manner as previously described, a preprocessed signal 322 from the partial integrator stage 208.

It should be noted that the preprocessed signal 322 and .o various other waveforms described herein have been idealized somewhat for purposes of illustration, and those skilled in the art will appreciate that the actual waveforms may vary in shape and size from those depicted in Fig. 9 and elsewhere.

The preprocessed signal 322 is fed to the positive peak detector 300 and the negative peak detector 302 which measure and track the positive and negative peaks, respectively, of the preprocessed signal 322. The positive peak output signal 330 of the positive peak detector 300 and the negative peak output signal 332 of the negative peak detector 302 are depicted in Fig. 9. The positive peak output signal 330 and the negative peak output signal 332 are averaged by a voltage divider 304, which is comprised of a pair of resistors 340 and 341. The output of voltage divider 304 is utilized as a P:\OPER\DB\17835-95.DV3 30/4/99 25 threshold signal 334 and represents the approximate peak-topeak midpoint of the preprocessed signal 332. The output of the voltage divider 304 is provided to a comparator 306 which compares the divided voltage with the preprocessed signal 332.

The comparator 306 changes states when the preprocessed signal 332 crosses the threshold signal 334, indicating a transition in the read data from a 1 to 0 or a 0 to i. The output of comparator 306 is shown as output data waveform 362 in Fig. 9.

As explained in more detail below, the output data waveform 362 is fed back to the positive peak detector 300 and negative peak detector 302 to allow tracking of the DC envelope. The output of the comparator 306 is also provided to a dual edge circuit 350 which generates a unipolar pulse of fixed duration each time the comparator 306 changes states.

The output of the dual edge circuit 350 provides clocking and data information from which recovery of the recorded data may be had in a straightforward manner. For example, in a pulse-width modulation technique such as the GCR 8/9 modulation code described previously, each data pulse output from the dual edge circuit 350 represents a transition in flux a recorded 1-bit), while the lack of data pulse at oee.

clock intervals would represent the lack of transition in flux a recorded 0-bit). The sequence of recorded bits can thereafter be decoded by decoder 24 (shown in Fig. 1) by methods well known in the art to determine the original data.

In order to properly track the envelope caused by the DC portion of the preprocessed signal 322, a preferred embodiment feeds back duty cycle information from the output signal 362 to the peak detectors. Thus, the output of the comparator 306 is fed back to the positive peak detector 300 and the negative peak detector 302. This process may be explained further by reference to Fig. 8 which depicts a more detailed circuit diagram of the data generator stage 210. As shown in Fig. 8, the preprocessed signal 322 is provided to the base of transistors Q2 and Q5. Transistor Q2 is associated with the P \OPER\DBW\17835-95.DV3 30/4/99 26 positive peak detector 300, and transistor Q5 is associated with the negative peak detector 302. Because the positive peak detector 300 and negative peak detector 302 operate in an analogous fashion, the duty cycle feedback operation will be explained only with reference to the positive peak detector 300, while those skilled in the art will understand by perusal of Fig. 8 and the description below the analogous operation of negative peak detector 302.

Transistor Q2 charges a capacitor C1 when the amplitude of the preprocessed signal 322 exceeds the stored voltage of the capacitor C1 (plus the forward bias voltage of the transistor Q2). In Fig. 9, it can be seen that the positive peak output signal 330 charges rapidly to the peak of the signal 332. The output signal 362, through feedback, maintains the positive charge on the capacitor C1 when the output signal 362 is high and allows the capacitor C1 to discharge when the output signal 362 is low. Thus, if the output signal 362 is high, the positive charge on capacitor C1 is maintained by transistor Q1 through resistor R2. Preferably, resistors R1 and R2 are selected to be the same value so that charge is oo oi S"added to the capacitor through resistor R2 at the same rate oo that it is discharged through resistor R1, thus maintaining as constant the net charge on capacitor Cl. If, on the other 25 hand, the output signal 362 is low, then transistor Q1 is turned off and capacitor C1 is allowed to discharge though resistor R1. The values of capacitor C1 and resistor R1 are preferably selected such that the time constant is slightly faster than the speed of expected of DC buildup so that the capacitor C1 can track the change in DC level as it occurs.

The output of capacitor C1 is provided to the base of *-...transistor Q3. The voltage level of the emitter of Q3 is a bias voltage level above the output of capacitor C1. Current is drawn through resistor R3 which allows the emitter of transistor Q3 to follow the voltage of the capacitor C1 (offset by the emitter-base bias voltage). Thus, the emitter P:\OPER\DBW\17835-95.DV3 30/4/99 27 of transistor Q3 yields positive peak output signal 330. It should be noted that transistors Q1 and Q2 are NPN type transistors while Q3 is a PNP type resistor. Thus, the NPN-PNP configuration largely cancels out adverse thermal effects that may be experienced with transistors Q1, Q2 and Q3 and also cancels out the bias voltages associated with their operation.

The negative peak detector 302 operates in an analogous fashion to the positive peak detector 300 and is therefore not explained in greater detail. The emitter of transistor Q6 yields negative peak output signal 332.

As described previously, positive peak output signal 330 and negative peak output signal 332 are averaged by a voltage divider 304 comprised of pair of resistors R4 as shown in Fig.

8 to form threshold signal 334. The threshold signal 334 therefore constitutes the approximate midpoint of the peak-topeak value of the preprocessed signal 322 tracks the DC envelope of the preprocessed signal 322 through duty cycle feedback compensation.

Although the duty cycle feedback has been shown in the preferred embodiment as originating from the output of the comparator 306, it may be observed that other feedback paths may also be utilized. For example, a similar feedback path may be taken from the output of dual edge circuit 308 if a flip/flop or other memory element is placed at the output of the dual edge circuit 308. Also, other means for measuring duty cycle and adjusting the threshold signal to track the DC envelope may be utilized.

A preferred technique such as described generally in Figs. 4 and 5 includes the step of differentiation of the playback signal prior to partial integration, followed thereafter by the step of DC tracking. The preferred method is particularly suitable for systems having a playback signal with relatively poor resolution, and may be advantageously P:\OPER\DBW\1783-95.DV3 30/4/99 28 applied, for example, to reading information stored in a GCR format. In one aspect of the preferred method, the initial step of differentiation reduces the low frequency component from the incoming playback signal. In another aspect of the preferred method, the partial integration stage results in restoration or partial restoration of the playback signal while providing rapid response due to the high pass boost from the bandpass filter stage). The preferred method may be contrasted with a method in which integration of the playback signal is carried out initially prior to differentiation), which may lead to an increased size of DC component and a correspondingly more difficult time in tracking the DC component.

Fig. 11 depicts the differences between the laser pulsing in GCR 8/9 and RLL 2,7 code formats. In GCR 8/9, a cell 28 is defined as a code word corresponding to a data bit. For GCR 8/9, a cell is equal to one data bit. Thus, cells 30 through 41 each correspond to one clock period42 of clock waveform 45. For a optical disk rotating at 2,400 revolutions per minute (RPM) with a storage capacity of 256 MBYTES clock period 42 will typically be 63 nanoseconds or a clock frequency of 15.879 Mhz. GCR data waveform 47 is the encoded data output from the encoder 12. A representative data sequence is depicted in Fig. 11. The code data sequence 011110100110 is shown in GCR data 50 through 61 where GCR data is a GCR data 51 is a GCR data 52 is a and so forth for GCR data 53 through 61. Pulse GCR waveform 65 is the output from laser pulse means 14 inputted into pulse laser 16.

Pulse GCR waveform 65 as shown has not been adjusted in time or duration to reflect performance enhancement for specific data patterns. Pulse GCR 67 through 78 reflect no pulse when the corresponding GCR data 47 is and reflects a pulse when GCR data 47 is a For example, pulse GCR 67 has no pulse because GCR data 50 is a Conversely, pulse GCR 68, 69, and 71 show a laser pulse because GCR data 51 through 54 are a respectively, and similarly for pulse GCR 72 through 78.

P:\OPER\DBW\17835-95.DV3 30/4/99 29 Under the depicted uniform scenario, pulse GCR pulsewidth 79 is uniform for pulse GCR 68, 69, 70, 71, 73, 76 and 77. For the preferred embodiment this pulsewidth is 35 nanoseconds.

Each laser pulse corresponding to pulse GCR waveform creates a recorded pit 80 on optical medium 18. Recorded pit 82 corresponds to pulse GCR 68. Recorded pit 83 corresponds to pulse GCR 69. Similarly, recorded pits 84 through 88 corresponds to pulse GCR 70, 71, 73, 76 and 77, respectively.

Because of thermal dissipation and spot size on the optical medium 18, the recorded pits 80 are wider in time than pulse GCR 65. Successive recorded pits 80 merge together to effectively create a larger recorded pit. Thus the elongated recorded pit has a leading edge corresponding to the first recorded pit and a trailing edge corresponding to the last recorded pit. For example, the pit created by recorded pits 82 through 85 has a leading edge from recorded pit 82 and a trailing edge from pit 85. Under the GCR 8/9 data format, a rising edge corresponds to a while a trailing edge O. 20 corresponds to a Hence, for data pattern "11110" as shown by GCR data 51 through 55, a rising edge occurs for the first as shown by recorded pit 82 and, at the end of the GCR oo data 54, a trailing edge occurs as shown by recorded pit because GCR data 55 is a Playback signal 90 will be low when recorded pit 80 shows no pits. At the leading edge of a pit, playback signal 90 will rise and remain high until the trailing edge of the pit is reached. The signal will go low and remain low until the next pit. For example, playback signal 91 is low because GCR data 47, which is a did not create a pit. At the front edge of recorded pit 82, playback signal 90 has a leading edge as some shown in playback signal 92. Playback signal 90 will then remain unchanged until a trailing edge occurs on a recorded pit. For example, because recorded pits 83 and 84 show no trailing edge, playback signal 93 and 94 remains high. The signal remains high during playback signal 95 because of P \OPER\DBW\17835-95lV3 30/4/99 30 recorded pit 85. However, because GCR data 55 is a recorded pit 85 creates a trailing edge. Thus, playback signal 56 decays. The signal will decay to 0 until a recorded pit occurs creating a rising edge. Thus, with the occurrence of recorded pit 86, which corresponds to GCR data 56 being a playback signal 97 because there is no immediate successor to recorded pit 86 when GCR data 57 is a playback signal 98 decays. Playback signal 99 remains low because there is no recorded pit when GCR data 58 is a With GCR data 59 and 60 being recorded pits 87 and 88 overlap creating one larger pit. Thus, playback signal 100 rises and playback signal 101 remains high. Playback signal 102 falls at the trailing edge of recorded pit 88 when GCR data 61 is a "0" For RLL 2,7 a cell consists of two data bits which corresponds to two clock periods 121 of 2F clock waveform 120.

For a 256 MBYTE disk, an RLL 2,7 encoding format will require a 2F clock pulse width 121 of 35.4 nanoseconds or a clock frequency of 28.23 Mhz. The calculation of this value is straightforward. In order to maintain the same disk density, the GCR 8/9 and RLL 2,7 encoding formats must contain the same amount of information in the same recording time. Because two code bits are required per data bit, the RLL 2,7 format requires a clock frequency twice that of the data bits of the .00 GCR data. The GCR data format records nine bits of code bits per eight bits of data. Thus, the GCR data bit clock is nineeights of the clock period 42. Thus, for a GCR clock period 42 S0 of 63 nanoseconds, the RLL 2,'7 pulse width 121 must be 35.4 nanoseconds in order to maintain the same disk density.

The RLL 2,7 data waveform 122 reflects two code bits per cell. For example, RLL 2,7 data 124 shows a data pattern "00" while RLL 2,7 data 125 shows a data pattern In this data format, a represents a transition in data. Thus, 2,7 data 125 goes high when the occurs in the data pattern.

Similarly, RLL 2,7 data 126 goes low when the occurs in the data pattern. While a occurs RLL 2,7 data 122 remains P:\OPER\DBW\17835-95.DV3 30/4/99 31 in the same state. Pulsed 2,7 waveform 137 reflects the pulsing of laser 16 corresponding to RLL 2,7 data 122. Thus, for 2,7 data 125 and 126, during the period when that signal is high, pulsed 2,7 waveform 140 and 141 is high. Because of the thermal elongation of the pit, pulsed 2,7 waveform 141 goes low prior in time to RLL 2,7 data 126. For longer data patterns of the pulsing must remain on. For example, during the data pattern "10001" as shown in RLL 2,7 data 128 and 129, pulsed 2,7 waveform 143 and 144 remains high longer than pulsed 2,7 waveform 140 and 141. For data patterns of successive the pulsed 2,7 waveform 137 can be pulsed as separate pulses. For example, for the data pattern "1000001" RLL 2,7 data 132, 133 and 134 can be pulsed in two separate pulses as shown in pulse 2,7 147, 148 and 149.

As with the GCR 8/9 format, recorded pit 160 shows thermal elongation. For example, recorded pit 162 is wider in time than the pulse from pulsed 2,7 waveform 140 and 141; similarly for recorded pit 163. Physical limitations of existing lasers and optical disks prevent recorded pit 163 from being recorded in two successive pulses at 2F clock 120 frequency. Thus, for these intermediate size pits, the thermal accumulation distortion effects will be greater than in either recorded pit 162 or the combined recorded pits 164 and 165.

Again, playback signal 167 depicted by playback signal 168 through 174 goes high on leading edges of recorded pits 160, and remains constant during the presence or absence of pits.

The pulsed GCR code can be improved by correcting predictable position shifts. Fig. 12 shows the timing diagram for the write compensation of the laser pulse generator 14.

Experimental testing showed that recording early when the laser 16 is off for two bits or greater enhances performance.

Clock waveform 176 is the code bit clock used for clocking data 177, 203 and 229 which show the worst case data patterns for enhancement. Other patterns can be corrected but will suffer in signal amplitude. Data 180 through 184 corresponds P:\OPER\DBW\17835-95.V3 30/4/99 32 to the data sequence "10100". The uncompensated pulse waveform 188 through 192 corresponds to this data pattern without write compensation. Uncompensated pulse waveform 189 and 191 occur in the second half of the clock period. After write compensation, the output of laser pulse generator 14 corresponds to compensated pulse waveform 195 where compensated pulse waveforms 197 and 198 remains unchanged and a shortened off-period for compensated pulse waveform 199 provides an earlier compensated pulse waveform 200. During compensated pulse 201, laser 16 remains off for a longer duration than uncompensated pulse 192. Similarly for data 206 through 209 corresponding to data pattern "1100" uncompensated pulse waveform 211 would be off for uncompensated pulse waveform 213 followed by two pulses uncompensated pulse waveforms 214 and 216. Again, the write compensation circuit adjusts compensated pulse wave form 220 so that compensated pulse waveform 225 will occur closer in time to compensated pulse waveform 223 so that compensated pulse waveform 224 is shorter than uncompensated pulse waveform 215. Finally, data 231 through 235, corresponding to the data pattern "00100" has uncompensated pulse waveform 237 occurring at uncompensated pulse waveform 240. Write compensation would move compensated pulse waveform 243 earlier in time to compensated pulse waveform 246.

Fig. 13 shows the schematic diagram of the write compensation circuit which comprises data pattern monitor 248, write compensation pattern detector 249 and delay circuit 269.

Data pattern monitor 248 is a serial shift register that sequentially clocks encoded data from encoding means 12. The last six clocked in data bits are sent to write compensation pattern detector 249 where they are analyzed for determining whether to pulse the laser earlier than normal.

Data pattern monitor 248 consists of data sequence D flip flops 250 through 256. Encoded data is input into the D port of data sequence D flip flop 250 whose Q output WDl becomes P;\OPER\DBW\17835-9S.DV3 30/4/99 33 the input of the D port of data sequence D flip flop 251. This clocking continues through data sequence D flip-flops 252 through 256 whose Q output WD7 is the data sequence delayed by seven clock periods from when it was first input into data pattern monitor 248. The Q outputs WDI, WD2, WD3, WD4, and of data sequence D flip flops 250 through 255, respectively, represent the last six of the last seven data bits inputted into a data pattern monitor 248. These six bits are sent to a write compensation pattern detector 249 where they are compared to predetermined data patterns; and, if they match, an enable write signal is sent to a delay circuit 269 to indicate that the laser pulse is to occur earlier than normal.

The first data pattern is detected by inverting the Q data WDI, WD2, WD3, and WD4 from data sequence D flip flops 250, 251, 253 and 254 through data inverters 260, 261, 262 and 263, respectively. The output of these inverters is AND'd with the output from data sequence D flip flop 252 in detect AND gate 264. Thus when a sequence "00100" occurs, the output of detect AND gate 264 goes high indicating that a detect of the data pattern occurred. Similarly, the second data pattern is detected by inverting the Q output WD2, WD2, and WD4 from data sequence D flip flops 250, 251, and 253 through the data inverters 282, 283, and 284 respectively and ANDing with the outputs WD4 and WD6 of data sequence D flip flops 252 and 254 in detect AND gate 286. Thus, a data pattern of "010100" will trigger a high from detect AND gate 286 indicating a detect.

The third data sequence is detected by inverting the Q output WDI and WD2 from data sequence D flip flops 250 and 251 through data inverters 287 and 288 and ANDing with the Q output QWD3 and WD4 of data sequence Dflip flops 252 and 253 in data detect AND gate 286. Thus the data pattern of "1100" will trigger a detect from detect AND gate 289 indicating the presence of the data. The data pattern detect output of detect AND gates 264, 286 and 289 is OR'd in detected pattern OR gate 266 whose output goes high when one of the three data patterns is detected. The detected pattern output is clocked in enable P:\oPER\DBW\17835-95.DV3 30/4/99 34 write D flip flop 268 where Q output, enable write signal, is then sent to delay circuit 269.

Delay circuit 269 takes the clocked data output WD4 of data sequence D flip flop 253 and simultaneously inputs it into delay line 276 and not delay select AND gate 274. The delayed output of delay line 276 is inputted into delay select AND gate 272. the enable write signal from write compensation pattern detector 249 will enable either delay select AND gate 272 or not delay select AND gate 274. When the enable write signal is low which indicates that one of the three data patterns has not occurred, it is inverted by enable write inverter 270. This allows the delayed data from delay line 276 to be clocked. On the other hand, if enable write is high, which indicates that one of the three data patterns has occurred, then the not delay select AND gate 274 allows the transmission of the data from data sequence D flip flop 253 which is undelayed. The output from delay select AND 272 and not delay select AND gate 274 is OR'd in data OR gate 278 where it is outputted from delay circuit 269. Although prior discussions about the write compensation circuit or timing indicated that for the three data patterns, the write pulse would occur 10 nanoseconds for all data but the three data o. patterns. The delay of delay circuit 276 is set between 8 to 12 nanoseconds for the frequency of the preferred embodiment.

ae When recording lower frequency data patterns, the resultant magneto-optical signal has a slower rise time than fall time. This causes the final output from the waveform processor 22 to have degraded amplitude on positive peaks which can be corrected by recording with higher effective power at the leading edge of the data pattern. For the preferred embodiment, the data pattern "000111" will trigger a wide write signal during the second of the data pattern thereby pulsing the laser during its normal off period.

In Fig. 14, clock waveform 301 clocks data waveform 303 P;\OPER\DB1i\17835-95.DV3 30/4/99 35 through the laser pulse greater 14 for the data pattern "000111". As depicted by data 305 through 310, the laser pulse generator 14 generates pulse waveform 312 with pulses 314, 315 and 316 when data waveform 303 is a During the second "1" of this data pattern, the laser pulse generator 14 will turn on for the increase power waveform 318 and generate a pulse 320. The output laser pulse waveform 322 results from the OR of pulse 312 and turn on for the increase power waveform 318 that creates laser pulses 323, 324 and 325. Under normal operations, laser pulse 324 would be off during the first half of the clock period. However, under this particular data pattern, keeping the laser on for the laser pulses 323 and 324, effectively increases the power fifty percent during this time period.

In Fig. 15, a host computer 410 which serves as a source and utilizer of digital data is coupled by interface electronics 412 to a data bus 414. As host computer 410 processes data, and it wants to access external memory from time to time, a connection is established through interface electronics 412 to data bus 414. Data bus 414 is coupled to the input of a write encoder 416 and the input of a write encoder 418. Preferably, write encoder 416 encodes data from bus 414 in a low density, i.e. ANSI format and write encoder 418 encodes data from data bus 414 in a higher density format.

The Draft Proposal for 90 MM Rewritable Optical Disk Cartridges for Information Interchange, dated 1 January 1991, which describes the ANSI format, is incorporated herein by reference. The outputs of write encoders 416 and 418 are coupled alternatively through a switch 422 to the write input of a magneto-optical read/write head 420. The read output of head 420 is coupled alternatively through a switch 424 to the inputs of a read decoder 426 and a read decoder 428. Read decoder 426 decodes data in the same format, i.e. ANSI, as write encoder 416 and read decoder 428 decodes data in the same format as write encoder 418. Preferably, the encoding and decoding technique disclosed above is employed to implement P;\OPER\DBW\17835-95.DV3 30/4/99 36 write encoder 418 and read decoder 428. The outputs of encoders 426 and 428 are connected to data bus 414.

Responsive to a mode selection signal, switch control electronics 430 sets the states of switches 422 and 424 into either a first mode or a second mode. In the first mode, write encoder 418 and read decoder 428 are connected between data bus 414 and read/write head 420. In the second mode, write encoder 416 and read decoder 426 are connected between data bus 414 and read/write head 420. Read/write head 420 reads encoded data from and writes encoded data to a 490 millimeter optical disk received by a replaceable optical disk drive 432, which is controlled by disk drive electronics 434. Read/write head 420 is transported radially across the surface of the disk received by disk drive 432 by position control electronics 436.

When a 90 millimeter disk in a high-density format is received by disk drive 432, a mode selection signal sets the system in the first mode. As a result, data from host computer 410 to be stored on the disk, is organized by interface electronics 412 and encoded by write encoder 418, while data read from the disk is decoded by read decoder 428, reorganized by interface electronics 412 and transmitted to host computer 410 for processing.

a. *e When a 90 millimeter disk in the low density ANSI format is received by disk drive 432, a mode selection signal sets the system in the second mode. As a result, data from host computer 410 to be stored on the disk, is organized by interface electronics 412 and encoded by write encoder 416, while data read from the disk is decoded by read decoder 426, reorganized by interface electronics 412 and transmitted to host computer 410 for processing.

Preferably, irrespective of the format used to store data, the mode selection signal is stored on each and every P:\OPERTLAB'2171610 1sORldoc-13 Ssplnbs. 2001 -37disk in one format, the low density ANSI format, and the system defaults to the corresponding mode, e.g. the second mode. The mode selection signal could be recorded in the control track zone in ANSI format. When a disk is installed in disk drive 32, disk drive electronics 34 initially controls position control electronics 36 to read the area of the disk on which the mode selection signal is stored. Read decoder 26 reproduces the mode selection signal, which is applied to switch control electronics 30. If the installed disk has the low density ANSI format, then the system remains in the second mode when the mode selection signal is read. If the installed disk has the high density format, then the system switches to the first format when the mode selection signal is read.

In certain cases, it may be desirable to modify the laser for the first and second modes. For example, different laser frequencies could be used or different laser focussing lens systems could be used for the different modes. In such case, the mode selection signal is also coupled to read/write head 420 to control the conversion between frequencies or optical lens focussing systems, as the case may be.

It is preferable to organize the data stored in both formats to have the same number of bytes per sector, in the case of ANSI, 512 bytes. In such case, the same interface electronics 412 can be used to organize the data stored and retrieved from the disks in both formats.

In accordance with a preferred embodiment of the invention, the same read/write head, position control electronics, optical disk drive, disk drive electronics interface electronics and data bus can be employed to store data on and retrieve data from optical disks in different formats. As a result, downward compatibility from higher density formats that are being developed as the state of the are advances, to the industry standard ANSI format can be realized using the same equipment.

P:\OPER\RAB\2171610 Isl ORdoc13 Septembcr, 2001 -38- It will be appreciated that the various circuits and methods described herein are not limited to magneto-optical systems but may also be useful in systems for reading data on stored tapes and other types of disks as well and, in a more general sense, in any system (whether or not a data storage system) for processing electrical signals in which it is desired to mitigate the effects of DC buildup.

While the invention has been particularly shown and described with reference to certain embodiments, it will be understood by those skilled in the art that various changes in form and detail may be made without departing from the spirit and scope of the invention.

Throughout this specification and the claims which follow, unless the context requires otherwise, the word "comprise", and variations such as "comprises" and "comprising", will be understood to imply the inclusion of a stated integer or step or group of integers or steps but not the exclusion of any other integer or step or group of integers or steps.

The reference to any prior art in this specification is not, and should not be taken as, an acknowledgment or any form of suggestion that that prior art forms part of the 20 common general knowledge in Australia.

Claims (21)

1. A method for detecting transitions in an input signal having a DC component, said method comprising the steps of: generating a threshold signal from said input signal; comparing said input signal to said threshold signal to thereby generate an output signal; and adjusting said threshold signal in response to said output signal.

2. The method according to claim 1 wherein said step of adjusting said threshold signal in response to said output signal causes said threshold signal to track the DC component of said input signal.

3. The method according to claim 1 wherein said input signal includes peaks corresponding to locations of data stored on a medium.

4. The method according to claim 3 wherein said step of generating a threshold signal includes detecting respective .voltage levels of said peaks. *o0o The method according to claim 1 wherein an amount of adjustment to said threshold signal in response to said output signal is proportional to a duty cycle of said output signal. 00 0

6. A method for retrieving data stored on a medium, said method comprising the steps of: *eg0 reading said stored data to thereby generate a playback signal; partially integrating said playback signal; ~generating a threshold signal which varies with a DC component of said partially integrated signal; and generating an output signal indicative of said stored data by comparing said partially integrated signal with said threshold signal. P;\OPER\DBW\17835-95.DV3 30/4/99 40

7. The method according to claim 6 wherein said medium includes a magneto-optical disk.

8. The method according to claim 6 further comprising the step of differentiating said playback signal prior to said partially integrating step.

9. The method according to claim 6 wherein said step of partially integrating comprises: integrating said playback signal; simultaneously with but separately from said integrating, bandpass filtering said playback signal; and taking a difference between said integrated signal and said bandpass filtered signal to thereby generate a difference signal. The method according to claim 9 further comprising the step of low pass filtering said difference signal.

11. The method according to claim 6 wherein said step of generating a threshold signal comprises: detecting a positive peak voltage of said partially 9999 integrated signal; detecting a negative peak voltage of said partially integrated signal; and averaging said positive peak voltage and said negative peak voltage.

12. The method according to claim 11 further comprising the step of adjusting said threshold signal in response to a state of said output signal.

13. The method according to claim 12 wherein said threshold signal is adjusted by decreasing a detected positive peak voltage when said output signal is in one of either a low state or high state, and decreasing a detected negative peak voltage when said output signal is in the other of said low P:\OPER\DBW\17835-95.DV3 30/4/99 41 state or high state.

14. The method according to claim 6 wherein said threshold signal corresponds to an approximate midpoint of said partially integrated signal. A method for retrieving data stored on a medium, said method comprising the steps of: reading the stored data to thereby generate a signal; partially integrating said signal; generating a threshold signal corresponding to an approximate midpoint of said partially integrated signal; and generating an output signal indicative of said stored data by comparing said partially integrated signal with said threshold signal.

16. The method according to claim 15 wherein said medium includes a magneto-optical disk.

17. The method according to claim 15 wherein said step of reading said stored data includes the steps of generating an input signal and differentiating said input signal.

18. The method according to claim 15 wherein said step of partially integrating said signal comprises: integrating said signal; simultaneously with but separately from said integrating, bandpass filtering said signal; and taking a difference between said integrated signal and said bandpass filtered signal.

19. The method according to claim 15 wherein said step of :a":generating a threshold signal includes adjusting said threshold signal in response to said output signal. The method according to claim 19 wherein the adjustment to said threshold signal is proportional to a duty cycle of P:\OPER\RAB2171610 1s ORdoc-13 Scpember. 2001 -42- said output signal.

21. An optical claims 1 to

22. An optical claims 6 to 14. disc system operated according to the method recited in any one of disc system operated according to the method recited in any one of

23. An optical claims 15 to disc system operated according to the method recited in any one of 1 C V C V V

24. A method for detecting transitions in an input signal having a DC component substantially as hereinbefore described with reference to the accompanying drawings.

25. A method for retrieving data stored on a medium substantially as hereinbefore described with reference to the accompanying drawings. DATED this 13 th day of September 2001 DISCOVISION ASSOCIATES By its Patent Attorneys DAVIES COLLISON CAVE