The present invention relates to an apparatus, or a drive, having an optical head for reading data stored in an optical carrier, comprising:
a light source for illuminating said carrier,
an optical mounting for directing the reflected light from said carrier to a detection branch.
This apparatus finds many applications, notably for data carriers constituted by optical discs. Often the data stored in the disc provide output signals which are poor in quality and need processing for improving their readability.
The invention proposes an above-mentioned apparatus in which measures are taken to improve the output quality of the output signal.
According to the invention, such an apparatus having an optical head for reading data stored in an optical carrier comprises:
a light source or master source for illuminating said carrier,
an optical mounting for directing the reflected light from said carrier to a detection branch in which a non-linear optical element is placed, the type of this non-linear element being chosen for improving the signal to noise ratio of the detected information.
The invention also proposes a method of reading an optical data carrier, comprising the steps of:
injecting into a slave laser the light coming from a master light source after reflection at a data carrier,
providing detection means for detecting the light coming from the data carrier by using a non-linear optical element providing an improvement of the signal to noise ratio of the detected information.
The idea of the invention is to use optical means for obtaining a better signal. The non-linear optical devices that the invention recommends are disclosed in the patent documents GB 2 118 765 and U.S. Pat. No. 4,748,630. The measures provided by the invention improve the signal-to noise ratio without using usual electronic circuits.
These and other aspects of the invention are apparent from and will be elucidated, by way of non-limitative example, with reference to the embodiment(s) described hereinafter.
According to an aspect of the invention, a non-linear optical element 80 is provided in the detection branch A non-linear optical element can be defined by a typical response curve, giving the output power of the element as a function of the input power. An example is given in
The typical output intensity Pout as a function of the input intensity Pin is shown in this
A first embodiment shown in
Another method is to use the threshold condition of the laser 100. For small amounts of light reflected from the disc, the slave laser will operate below its lasing threshold and a negligible amount of light is emitted. As the amount of reflected light increases the slave laser is forced to operate above the threshold, with the consequence that the output power increases substantially. The emitted optical power is very low when the electric current is below the threshold value. The output-power ratio between the HI level and the LO level is determined by the total number of modes in which spontaneous emission is generated. The typical value of this ratio is 106-107. This embodiment is shown in
(a) the wavelength λ1 of the light injected into the slave laser is very close to the wavelength λ2 of the (free-running) slave laser, i.e. λ1≈λ2, and
(b) the wavelength of the light injected into the slave laser is much shorter than the emission wavelength of the slave laser, i.e. λ1<<λ2.
To understand the difference, the gain G and the absorption ABS of a semiconductor laser operating above threshold is considered as a function of energy EN, see
For the case where λ1≈λ2, the injected wavelength, λ1, falls within the positive-gain region of the slave laser. Here the master laser and the slave laser are of the same type with nearly the same emission wavelengths. In this situation, injection of light corresponds to a reduction of the optical losses of the laser cavity, assuming that the slave laser, in free-running mode, is operating just below threshold. The result of the injected light is to force the laser above the threshold at the injected wavelength. If λ1<<λ2, the light injected into the slave laser is absorbed and transformed into electron-hole pairs. The effect of the extra generated electron-hole pairs is similar to an increased injection current level. Hence, in this way the laser can also be forced to operate above threshold.
Yet another implementation is to use transverse mode switching induced by injection of light reflected from the information carrier. Without (or with only a small amount of) injected light, the slave laser operates in the free-running transverse mode, see
Instead of using an edge-emitter semiconductor laser, it is also possible to use a VCSEL in the detection branch. In this situation the master laser shown in
In a practical situation the slave laser is pulsed through current modulation. Just below threshold the slave laser is very sensitive to injection from the master laser.
For the situation where the non-linear optical element exhibits hysteresis, the response function shown in
If the bias level is chosen close to threshold so that slave laser has laser action in the TM state, but does not lase when it is in the TE state, the integrated monitoring photodiode (MPD) may be used for bit detection. The MPD has a large bandwidth (several GHz) and is well suited for detecting whether the laser is lasing or not.
Advantages
The typical optical read-out power on the disc in an optical disc drive is approximately 0.5 mW. Increasing the read-out power above this value would erase information written on RW media. Realistic reflection coefficients for +RW discs are 0.15 (unwritten), and 0 (written) giving an average reflection coefficient of 0.075. This means that the typical currents induced in the detector (assuming a conversion gain of 0.2 A/W) are:
i=0.5 mW×0.075×0.2 A/W≈8 μA
The contribution from the detector noise to the total noise is given by:
where <i> is the average current on the detector, ωC the capacitive resistance of the detector, kBT the energy equivalent to the temperature T, and f the frequency bandwidth of the detector. For high-speed applications it is necessary to increase the frequency bandwidth of the detector, which means that the contribution from the detector noise increases correspondingly.
In BLU-RAY (BD) players, the dominant noise sources are laser noise (RIN) and detector noise (as given by the expression for ΔV/V).
The RIN increases linearly with the frequency f. The RIN should, however, be compared with the detector-noise power, (ΔV/V)2, which increases with f2. For 1× BD the RIN is the dominant noise term. The detector noise becomes dominant at higher speeds.
As was mentioned above, the non-linear optical element placed in the detection branch incorporates its own laser (either an edge emitter or a VCSEL). It assumed that, when the output from the NOE is high, the emitted optical power is ˜0.5 mW. This light falls on the detector and induces the current:
i=0.5 mW×0.2 A/W≈100 μA
Compared with the situation without a non-linear optical element (NOE) the current gain is 100/8˜12.5 which corresponds to 22 dB. For this case the introduction of the NOE reduces the detector noise contribution by 22 dB. This would then allow for an increased frequency bandwidth.
The presented idea hence offers a possibility to decrease the contribution from detector noise (which is the dominant noise term for high-speed applications) in, for example, BD players.
Another advantage of using a non-linear optical element for readout is the reduced sensitivity to media noise. As was described above, bits are detected when the reflected light from the disc crosses a threshold value. This means that reflectivity variations inherent in the disc-material do not play an important role as long as the variations are not so large that the threshold value is crossed.
Furthermore, since the detection of bits is reduced to a detection of transitions between two states (HI and LOW)n, this means that the slicer implemented in the current disc drives would be redundant. The purpose of the slicer is to detect the DC level around which the reflected light from the disc is modulated (this DC level is not necessarily constant but may show fluctuations). However, the DC level is constant for the non-linear optical element, see
The dynamic range, i.e. the reflectivity difference between marks and empty space, depends on the type of disc, for example, +RW discs have a different dynamic range from ROM discs. Again, since the detection of information is reduced to a threshold transition, readout with a non-linear optical element offers an increased compatibility robustness.
In contrast to low-power diode lasers, high-power diode lasers operating around 405 nm are known to be noisy. Laser noise is very likely to be reduced as a consequence of the injection of less noisy light from the low-power diode laser.
Some references are cited for illustrating this disclosure.
Number | Date | Country | Kind |
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03290226.4 | Jan 2003 | EP | regional |
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/IB04/00186 | 1/21/2004 | WO | 7/26/2005 |