The present invention generally relates to optical scanning devices for storing information onto a disc-shaped storage medium or reading information from such disc-shaped storage medium, where the disc is rotated and a write/read head is moved radially with respect to the rotating disc. More particularly, the invention relates to an optical disc drive comprising rotating means, defining a rotating axis for an optical disc, and optical scanning means, for scanning said optical disc with a light beam.
The present invention is applicable in the case of optical or magneto-optical disc systems. Hereinafter, the wording “optical disc system” will be used, but it is to be understood that this wording is intended to also cover magneto-optical disc systems.
It is commonly known that an optical storage disc comprises at least one track of storage space where information (such as images, data, music, . . . ) may be stored. Optical storage discs may be of a read-only type, where information is recorded during manufacture and can only be read by a user, or of a writable type, where information may be stored by a user. For writing information in the storage space of the optical storage disc or for reading information from the disc, an optical disc drive comprises, on the one hand, rotating means for receiving and rotating the optical disc and, on the other hand, optical means for generating an optical beam, typically a laser beam, and scanning the storage track with said laser beam. The rotating means are for example a motor, which drives a hub engaging a central portion of the optical disc. For optically scanning the rotating disc, the optical disc drive comprises for instance at least a light beam generator device (typically a laser diode), an objective lens, for focusing the light beam in a focal spot on the information layer of the disc, and an optical detector, for receiving the reflected light reflected from the disc and generating an electrical detector output signal. Since the technology of optical discs in general, the way in which information can be stored in an optical disc and the way in which optical data can be read from an optical disc are commonly known, it is not necessary here to describe this technology in more detail.
In an ideal case, the information layer of the disc is assumed to be perpendicular to the optical axis of the apparatus, so that the returning beam, i.e. the light reflected from the disc, is co-axial and counter propagates to the incoming light. In the case where the disc has a warped surface, the propagation axis of the reflected light is no longer co-axial to the axis of the incoming light, and a tilt effect, consisting in a deviation of the returning beam from the co-axial propagation of the ideal case, is observed. Such a disc-tilt is known to degrade the performance of optical disc-drives and has to be detected and compensated. Nevertheless, since the incoming light is focused to a tiny spot on the information layer of the disc, this deviation from co-axial propagation is very small and a tilt detector based on this principle of detection of said deviation is very difficult to implement.
It has then been proposed to amplify the deviation of the returning beam, for instance by adding aberrations to the incoming beam and therefore causing the spot size on the information layer to increase. For instance, when the disc is accessed with infra-red light (wavelength=about 790 nm), the larger amount of spherical aberration (said aberration being due to the fact that, in a radiation beam, the rays in the central part of the beam and the rays of the periphery of the beam have different focal points when they are focused on the disc) causes the spot size on the information layer of the disc to increase compared to the situation where the disc is accessed with red light (wavelength=about 660 nm). An example of such a situation is described in the Japanese patent JP2000076679, where disc-tilt is measured from the position of a spot with a light source having a wavelength different from the wavelength used for reading out the information on the disc. It turns out, however, that, when such a method is applied, the size of the spot on the optical detector is now too large compared to the size of the standard four-quadrant detector conventionally used in optical disc drive apparatuses: no significant difference in the signals from the quadrants of the detector can be measured, and hence no tilt error signal can be derived.
It is therefore the object of the invention to provide an optical disc drive avoiding this drawback.
To this end, the invention relates to an optical disc drive as defined in the introductory paragraph of the description and in which the optical scanning means themselves comprise at least:
This structure allows to generate on the detector a spot small enough in order to be able to measure significant differences between the signals of the detector and therefore to derive a noticeable tilt error signal.
Preferably, the diffractive structure is attached to one surface of a servo-lens positioned just before the optical detector. However, it may also be attached to one surface of an objective lens used as focusing means, or to a separate plate.
In an advantageous implementation, the diffractive structure consists of a series of ring-shaped prisms, but it can also be approximated by a step-wise structure.
The invention will now be described, by way of example only, in a more detailed manner and with reference to the accompanying drawings, in which:
An example of an optical disc drive, suitable for storing information on or reading information from an optical disc 1, is schematically illustrated in
The disc drive further comprises a platform 9, which is displaceable in the radial direction of the disc 1 with respect to the sledge 7, and which is displaceably mounted with respect to the sledge 7 by mounting means not shown for the sake of clarity. A radial platform actuator 10 is provided for radially displacing the platform 9 with respect to the sledge 7. Radial sledge actuators and radial platform actuators are known per se, and as the design and operation of such radial platform actuator are not the subject of the present invention, it is not necessary here to discuss them in great detail.
The disc drive further comprises, for scanning the tracks (not shown) of the disc 1 by means of an optical beam, an optical device 20 which is described later. It also comprises a pivot platform actuator 11, arranged for pivoting the platform 9 with respect to the sledge 7 (such pivot platform actuators are known per se and therefore not discussed in great detail), and a control unit 12 having the following outputs: a first output 12a connected to a control input of the motor 3, a second output 12b coupled to a control input of the radial sledge actuator 8, a third output 12c coupled to a control input of the radial platform actuator 10, a fourth output 12d coupled to a control input of an axial platform actuator 13, and a fifth output 12e coupled to a control input of the pivot platform actuator 11. The control unit 12 is designed to generate at said outputs 12a to 12e control signals SCM, SCS, SCpr, SCpa and SCPp respectively for controlling the motor 3, the sledge actuator 8, the radial platform actuator 10, the axial platform actuator 13 and the pivot platform actuator 11. The control unit 12 has also a read signal input 12f for receiving a read signal SR from an optical detector described in the following paragraphs.
The optical scanning device 20 will now be described. According to a preferred embodiment of the invention illustrated in
After its reflection on said information layer, the converging beam 29 forms a reflected beam which returns on the same optical path. This backward radiation is further transmitted through the polarized beam-splitter 24 and passes through a servo-lens 40 which transforms said returning beam into a converging beam 41 falling on an optical detector such as a servo-detector 42. The semi-transparent mirror 23 is constructed with optical elements that allow to separate the emitted beam and the returning one and to supply the latter to the optical elements (40,42) that follow said mirror.
In order to obtain a measure of the amount of radial and tangential tilt of the disc 1, a second light source 51, typically a laser with a second wavelength different from said first wavelength (in this example 780 nm), is temporarily switched on for producing a second light beam. By definition, the two wavelengths are considered as different when the absolute difference between them is more than 10 nm. The polarized light emitted by said light source 51 is reflected by the polarized beam-splitter 24 and the mirror 25, and then passed through the collimator lens 26 and focused by the objective lens 27. A second backward beam obtained after reflection of said second beam on the information layer is then received by the servo-detector 42. Since the wavelength of the second light beam is different from that of said first light beam, the spot on the information layer of said first disc is now aberrated. As a result the size of the spot on the detector of this second beam becomes larger than the size of the detector.
According to the invention, it is proposed, in order to overcome the problem of the size of the spot on the servo-detector, to attach to one surface of one of the lenses located on the path of the backward beam or on a separate plate, between the focusing point on the information layer and the servo-detector, a diffractive structure implemented as described hereinunder. By doing so, the size of the spot on the servo-detector is reduced when accessing said first disc with the light emitted by the second light source.
An example of this diffractive structure is shown in
h2=λ2/(n2−1) (1)
where λ2 is the wavelength of the light emitted by the second light source 51 and n2 is the refractive index of the prism material at the wavelength λ2. As shown in
An important feature of the diffractive structure is that it should not influence the returning light of said first light beam when this light is used to access said first disc. A blazed grating however also diffracts the first light beam significantly into the first diffraction order. In order to prevent this, instead of a blazed grating a binary grating must be used. In a binary grating, each blaze is approximated by a step-wise structure (see
h1=λ1/(n1−1) (2)
where λ1 is the wavelength of the light emitted by the first light source and n1 is the refractive index of the grating material at the wavelength λ1. Here, for exemplary purposes, the refractive index of the grating material for both λ1 and λ2 is assumed to be 1.65. For the situation shown in
The diffracting structure used, according to the invention, to reduce the size of the spot from the second light source on the servo-detector is either attached to the servo-lens or to the objective lens or on a separate plate. In the first case, the diffractive structure (such as illustrated in
The simulated normalized radial-tilt error-signal obtained is shown in
In the second case, the diffractive structure may be attached to the objective lens. The radius and the corresponding pitch for each ring are then given in the following table 2, together with the numerical aperture (NA) belonging to the radius:
In order not to influence the returning light from the second light source when accessing a second disc having said second cover layer, the diffractive structure is confined to the region defined by 0.5<NA<0.65, where it acts as a weak positive lens for the light emitted by the second light source. Due to the lens effect, the rays are re-focused on the servo-detector (it may be noted that the diffractive structure has an overall aspheric shape in order to fit onto the aspheric surface of the objective lens). As described above, the grating structure may be approximated by a phase-step profile, so that the light from the first light source is not affected when passing through the region 0.5<NA<0.65. The normalised radial-tilt error-signal obtained with this modified objective lens is shown in
It must be understood that the invention thus defined is not limited to the above-mentioned implementations. Whilst in the above described embodiment the first wavelength is smaller than the second wavelength, it is possible that the first wavelength may also be larger than the second wavelength. Also, whilst in the above-described embodiment, explicit reference is made to a detector with four quadrants, it appears that the principle can be applied to a detector having at least two or even six and more segments. Although the embodiment described above indicates a situation where the beam from the second light source used for the tilt measurement is confined to a numerical aperture which is smaller than the numerical aperture of the beam from the first light source, it is appreciated that a similar principle to the one given above can be applied to the opposite situation.
Number | Date | Country | Kind |
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02293262.8 | Dec 2002 | EP | regional |
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/IB03/06213 | 12/22/2003 | WO | 6/24/2005 |