JPH07320324A - Magneto-optical recording medium and reproducing method thereof - Google Patents

Magneto-optical recording medium and reproducing method thereof

Info

Publication number
JPH07320324A
JPH07320324A JP10680594A JP10680594A JPH07320324A JP H07320324 A JPH07320324 A JP H07320324A JP 10680594 A JP10680594 A JP 10680594A JP 10680594 A JP10680594 A JP 10680594A JP H07320324 A JPH07320324 A JP H07320324A
Authority
JP
Japan
Prior art keywords
magneto
light
layer
reflective layer
semi
Prior art date
Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
Pending
Application number
JP10680594A
Other languages
Japanese (ja)
Inventor
Haruki Tokumaru
春樹 徳丸
Kiyotaka Arai
清敬 新井
Yoshimi Shimamori
巧美 島守
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
Mitsubishi Chemical Corp
Japan Broadcasting Corp
Original Assignee
Mitsubishi Chemical Corp
Nippon Hoso Kyokai NHK
Japan Broadcasting Corp
Priority date (The priority date is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the date listed.)
Filing date
Publication date
Application filed by Mitsubishi Chemical Corp, Nippon Hoso Kyokai NHK, Japan Broadcasting Corp filed Critical Mitsubishi Chemical Corp
Priority to JP10680594A priority Critical patent/JPH07320324A/en
Publication of JPH07320324A publication Critical patent/JPH07320324A/en
Pending legal-status Critical Current

Links

Abstract

(57)【要約】 【目的】 本発明の目的は、光磁気記録媒体において十
分な反射率を確保しながら大きなカー回転角を得ること
であり、更にはカー回転角が極大となるような光干渉層
膜厚でも十分な反射率を得ることが出来る光磁気記録媒
体を提供することにある。 【構成】 基体上に少なくとも磁性層と該磁性層よりも
光源に近い側に光源からの光の一部を反射し他を透過す
る半反射層と、磁性層より光源から遠い側に光源からの
光を反射する反射層をそれぞれ有する光磁気記録媒体に
おいて、該半反射層がAu、Ag、Cuの中から選ばれ
る1元素あるいは2元素以上を主体とする薄膜からなる
ことを特徴とする光磁気記録媒体。
(57) [Summary] [Object] It is an object of the present invention to obtain a large Kerr rotation angle while ensuring a sufficient reflectance in a magneto-optical recording medium. An object of the present invention is to provide a magneto-optical recording medium that can obtain a sufficient reflectance even with the thickness of the interference layer. A magnetic layer and a semi-reflective layer that reflects a part of light from the light source on the side closer to the light source than the magnetic layer and transmits the light on the other side on the substrate, and a semi-reflective layer on the side farther from the light source than the magnetic layer. In a magneto-optical recording medium each having a reflective layer that reflects light, the semi-reflective layer is a thin film mainly composed of one element or two or more elements selected from Au, Ag and Cu. recoding media.

Description

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

【0001】[0001]

【産業上の利用分野】本発明は光磁気ディスク、光磁気
テープ等の熱磁気記録による信号記録と磁気光学効果を
利用した信号再生を行う光磁気記録媒体およびそれを用
いた信号再生方法に関するものである。
BACKGROUND OF THE INVENTION 1. Field of the Invention The present invention relates to a magneto-optical recording medium such as magneto-optical disk and magneto-optical tape for recording signals by thermo-magnetic recording and reproducing signals utilizing magneto-optical effect, and a signal reproducing method using the same. Is.

【0002】[0002]

【従来の技術】従来の光磁気記録媒体は、基体上に反射
層、磁性層、透明な1層もしくは2層の光干渉層を有す
る構造を持つ。光磁気記録媒体の信号品質は光の反射率
と磁気カー回転角が大きいほど高くなるため、従来の媒
体では磁性層を光干渉層や反射層で挟むことにより光を
媒体内で多重反射させてカー回転角を高めている。
2. Description of the Related Art A conventional magneto-optical recording medium has a structure having a reflective layer, a magnetic layer, and one or two transparent optical interference layers on a substrate. The signal quality of a magneto-optical recording medium increases as the light reflectance and the magnetic Kerr rotation angle increase.Therefore, in a conventional medium, the magnetic layer is sandwiched between optical interference layers and reflective layers to cause multiple reflection of light in the medium. The car rotation angle is increased.

【0003】この時、光の干渉効果により反射率が低下
するが、信号品質に対する寄与は反射率よりもむしろカ
ー回転角の方が大きいので、トータルとしては信号品質
が向上することになる。信号再生時のノイズは通常、媒
体の反射率によって決定されるショットノイズで制限さ
れる。
At this time, the reflectance decreases due to the interference effect of light, but since the Kerr rotation angle contributes more to the signal quality than the reflectance, the signal quality is improved as a whole. Noise during signal reproduction is usually limited by shot noise determined by the reflectance of the medium.

【0004】従って、反射率が低下するとショットノイ
ズが低下することになるが、ショットノイズが極端に小
さくなると、システムノイズと呼ばれる機器全体のノイ
ズが信号再生時のノイズを支配するようになり、ショッ
トノイズ限界の信号検出ができなくなる。また、反射率
が極端に小さくなると、光スポットのフォーカスサー
ボ、トラッキングサーボにも支障をきたす。
Therefore, when the reflectance decreases, the shot noise also decreases. However, when the shot noise becomes extremely small, the noise of the entire device called system noise dominates the noise during signal reproduction, and the shot noise The noise limit signal cannot be detected. Further, if the reflectance becomes extremely small, it also interferes with the focus servo and tracking servo of the light spot.

【0005】媒体の反射率は光干渉層の膜厚に依存して
大きく変化し、反射率が極小となる光干渉層の膜厚付近
(干渉点と呼ぶこととする)で、カー回転角は極大とな
る。この反射率が極小となる光干渉層膜厚を選べば、光
干渉層の膜厚変動に対する反射率変動を最小に抑えるこ
とになるため、媒体の製造マージンを大きくすることが
できる。
The reflectivity of the medium greatly changes depending on the film thickness of the optical interference layer, and the Kerr rotation angle is around the film thickness of the optical interference layer where the reflectivity is minimal (hereinafter referred to as an interference point). It becomes maximum. By selecting a film thickness of the optical interference layer that minimizes the reflectance, the fluctuation of the reflectance with respect to the fluctuation of the thickness of the optical interference layer is suppressed to the minimum, so that the manufacturing margin of the medium can be increased.

【0006】しかしながら、従来の媒体では光干渉層の
厚みを干渉点に選ぶと反射率が小さくなりすぎるという
問題が生じる。よって、従来の媒体では極端にカー回転
角を大きくせず反射率が20%程度となるように光干渉
層膜厚が設計されており、磁性層のもつ性能を十分に引
き出しているとは言えない。
However, in the conventional medium, when the thickness of the optical interference layer is selected as the interference point, the reflectance becomes too small. Therefore, in the conventional medium, the film thickness of the optical interference layer is designed so that the Kerr rotation angle is not extremely increased and the reflectance is about 20%, and it can be said that the performance of the magnetic layer is sufficiently brought out. Absent.

【0007】[0007]

【発明が解決しようとする課題】光磁気記録媒体の記録
密度は現状よりも更に向上することが望まれており、記
録再生用レーザー光の短波長化は最も有力な手法であ
る。従って、今後光磁気記録媒体に対して用いられるレ
ーザーは短波長化する傾向が続くと考えられる。
It is desired that the recording density of the magneto-optical recording medium be further improved from the current state, and shortening the wavelength of the recording / reproducing laser beam is the most effective method. Therefore, it is considered that the laser used for the magneto-optical recording medium will continue to have a shorter wavelength in the future.

【0008】光の波長が短くなると磁性層の反射率その
ものが低下するうえに、光干渉層の屈折率は一般的に増
大するので、干渉点での反射率の低下は現在よりも更に
顕著になる。よって、先に述べたようにショットノイズ
限界の再生を行ったり、十分なサーボ信号を得るために
は光干渉層膜厚を干渉点から大幅にずらすことによりカ
ー回転角を犠牲にして反射率を確保することが必要にな
る。
When the wavelength of light becomes shorter, the reflectance of the magnetic layer itself lowers and the refractive index of the light interference layer generally increases, so that the reflectance at the interference point lowers more remarkably than at present. Become. Therefore, as described above, in order to perform reproduction at the shot noise limit or to obtain a sufficient servo signal, the Kerr rotation angle is sacrificed and the reflectance is sacrificed by significantly shifting the film thickness of the optical interference layer from the interference point. It is necessary to secure it.

【0009】透明基板を通して光磁気記録媒体の信号を
再生する場合、基板の複屈折が信号品質を低下させる。
基板の複屈折が大きい場合は、層構成を逆にして基板の
反対側から基板を通さずに信号を再生しなければならな
い。この場合、空気から直接光干渉層に光が入射するこ
とになり、干渉点での反射率低下が著しくなる。
When the signal of the magneto-optical recording medium is reproduced through the transparent substrate, the birefringence of the substrate deteriorates the signal quality.
When the birefringence of the substrate is large, the layer structure must be reversed to reproduce the signal from the opposite side of the substrate without passing through the substrate. In this case, light is directly incident on the light interference layer from the air, and the reflectance at the interference point is significantly reduced.

【0010】よって、基板を介さずに信号を再生する場
合にも光干渉層膜厚を干渉点から大きくずらして反射率
を確保する必要がある。本発明の解決しようとする課題
は、光磁気記録媒体において十分な反射率を確保しなが
ら大きなカー回転角を得ることであり、更にはカー回転
角が極大となるような光干渉層膜厚でも十分な反射率を
得ることである。
Therefore, even when the signal is reproduced without passing through the substrate, it is necessary to largely shift the film thickness of the optical interference layer from the interference point to secure the reflectance. The problem to be solved by the present invention is to obtain a large Kerr rotation angle while ensuring a sufficient reflectance in a magneto-optical recording medium, and even with an optical interference layer film thickness that maximizes the Kerr rotation angle. It is to obtain sufficient reflectance.

【0011】[0011]

【課題を解決するための手段】本発明者らは、上記課題
を解決すべく鋭意検討した結果、光磁気記録媒体の磁性
層よりも光源に近い側に光源からの光の一部を反射し他
を透過する半反射層を設け、該半反射膜をAu、Ag、
Cuの中から選ばれる1元素あるいは2元素以上を主体
とする薄膜で構成することにより、比較的大きな反射率
を確保しつつ大きなカー回転角を有する光磁気記録媒体
を提供できることを見い出した。
As a result of intensive studies to solve the above problems, the inventors of the present invention have reflected a part of the light from the light source on the side closer to the light source than the magnetic layer of the magneto-optical recording medium. A semi-reflective layer that transmits the other light is provided, and the semi-reflective film is made of Au, Ag,
It has been found that it is possible to provide a magneto-optical recording medium having a large Kerr rotation angle while ensuring a relatively large reflectance by forming a thin film mainly containing one element or two or more elements selected from Cu.

【0012】本発明の要旨は、基体上に少なくとも磁性
層と該磁性層よりも光源に近い側に光源からの光の一部
を反射し他を透過する半反射層と、磁性層より光源から
遠い側に光源からの光を反射する反射層をそれぞれ有す
る光磁気記録媒体において、該半反射層がAu、Ag、
Cuの中から選ばれる1元素あるいは2元素以上を主体
とする薄膜からなることを特徴とする光磁気記録媒体お
よび、その媒体を用い、磁性層からの光を半反射層から
の光でホモダイン検波することを特徴とする光磁気記録
信号の再生方法である。
The gist of the present invention is to provide at least a magnetic layer on a substrate, a semi-reflective layer that reflects a part of the light from the light source and transmits the other to the side closer to the light source than the magnetic layer, and from the magnetic layer to the light source. In a magneto-optical recording medium each having a reflective layer for reflecting light from a light source on the far side, the semi-reflective layer is Au, Ag,
A magneto-optical recording medium comprising a thin film mainly composed of one element or two or more elements selected from Cu, and homodyne detection of light from a magnetic layer by light from a semi-reflective layer using the medium. The method for reproducing a magneto-optical recording signal is characterized by the following.

【0013】以下に本発明を詳細に説明する。本発明に
用いられる基体としてはガラス基板、ポリカーボネート
等のプラスチック基板、PET等のプラスチックフィル
ム等が挙げられる。ポリカーボネート等の複屈折の小さ
な基体を用いる場合は基体を通して磁性層に光を入射す
る層構成とするのが望ましく、PETフィルム等の複屈
折の大きな基体を用いる場合は基体を通さず基体の反対
側から磁性層に光を入射する層構成が望ましい。
The present invention will be described in detail below. Examples of the substrate used in the present invention include a glass substrate, a plastic substrate such as polycarbonate, and a plastic film such as PET. When using a substrate with a small birefringence such as polycarbonate, it is desirable to have a layer structure in which light is incident on the magnetic layer through the substrate. Therefore, a layer structure in which light is incident on the magnetic layer is desirable.

【0014】本発明に用いられる磁性層としてはTbF
eCo等の希土類−遷移金属非晶質合金薄膜、Co/P
t等の人工格子薄膜等が挙げられる。磁性層の特性とし
ては垂直磁気異方性が大きく垂直磁化膜となること、磁
気光学効果が大きいこと、キュリー温度が170〜30
0℃程度でレーザーでの熱磁気記録に適していることが
望まれる。
The magnetic layer used in the present invention is TbF.
Rare earth-transition metal amorphous alloy thin film such as eCo, Co / P
An artificial lattice thin film such as t can be used. As the characteristics of the magnetic layer, the perpendicular magnetic anisotropy is large and the film becomes a perpendicular magnetization film, the magneto-optical effect is large, and the Curie temperature is 170 to 30.
It is desired to be suitable for thermomagnetic recording with a laser at about 0 ° C.

【0015】磁性層の膜厚は薄すぎると十分な磁気光学
効果が得られず、厚すぎると記録感度が低下するため、
15nm〜50nm程度が好ましい。磁性層よりも光源
に近い側に光源からの光の一部を反射し他を透過する半
反射層を設けるのが本発明において特徴的である。この
半反射層は光源からの光を反射することである程度の反
射率を確保する。
If the film thickness of the magnetic layer is too thin, a sufficient magneto-optical effect cannot be obtained, and if it is too thick, the recording sensitivity decreases.
It is preferably about 15 nm to 50 nm. The present invention is characterized in that a semi-reflective layer that reflects a part of the light from the light source and transmits the other is provided on the side closer to the light source than the magnetic layer. This semi-reflective layer ensures a certain degree of reflectance by reflecting the light from the light source.

【0016】それと同時に光の一部を透過させるが、こ
の透過光は磁性層、反射層、および光干渉層で多重反射
を起こしカー回転角が増大する。半反射層はカー回転角
が増大した光を再び逆向きに透過させ、受光素子に到達
させる。半反射層としては光を十分に透過する様な薄い
膜厚でも比較的大きな反射率を得ることが重要であり、
Au、Ag、Cuの中から選ばれる1元素あるいは2元
素以上を主体とする薄膜がそのような条件を満たす。
At the same time, a part of the light is transmitted, but this transmitted light causes multiple reflection in the magnetic layer, the reflection layer, and the light interference layer to increase the Kerr rotation angle. The semi-reflective layer transmits the light having the increased Kerr rotation angle in the opposite direction again and reaches the light receiving element. As a semi-reflective layer, it is important to obtain a relatively large reflectance even with a thin film thickness that sufficiently transmits light,
A thin film mainly containing one element or two or more elements selected from Au, Ag and Cu satisfies such a condition.

【0017】反射層の膜厚は厚すぎると光が透過しなく
なり、また逆に薄すぎると反射率が不十分となり問題が
ある。膜厚としては5〜40nmの範囲が好ましく、1
0〜30nmがより好ましい。光源の波長が600nm
〜800nm程度の場合は、半反射層を構成する薄膜の
主体がAu、Ag、Cuの中のいずれでも、あるいはそ
の中のどの2元素以上の組合せでも特に問題がない。
If the thickness of the reflective layer is too thick, light cannot be transmitted, and if it is too thin, the reflectance becomes insufficient, which causes a problem. The film thickness is preferably in the range of 5 to 40 nm, and 1
0-30 nm is more preferable. The wavelength of the light source is 600 nm
In the case of about 800 nm, there is no particular problem even if the main constituent of the thin film forming the semi-reflective layer is Au, Ag, or Cu, or any combination of two or more elements therein.

【0018】しかし、波長が600nm未満の短波長に
なると、Au、Cu、あるいはそれらの合金を主体とす
る薄膜を半反射層としても半反射層としての効果が十分
でなくなる。よって、600nm未満の短波長光源に対
応した光磁気記録媒体を作製する場合は、半反射層をA
gを主体とする薄膜とするのが好ましい。
However, when the wavelength becomes a short wavelength of less than 600 nm, the effect as a semi-reflective layer becomes insufficient even if the thin film mainly composed of Au, Cu or an alloy thereof is used as the semi-reflective layer. Therefore, when manufacturing a magneto-optical recording medium compatible with a short wavelength light source of less than 600 nm, the semi-reflective layer is
It is preferable to use a thin film mainly composed of g.

【0019】Auは耐食性に優れるため、単体で半反射
層を構成できるのに対して、AgやCuはAuに比べて
耐食性に劣るため、単体で半反射層を構成することは困
難である。従って、Ag、Cu、あるいはそれらの合金
を主体とする薄膜で半反射層を構成する場合は耐食性を
向上させるために、次に挙げる元素群の中から1元素以
上を半反射層に添加するのが好ましい。
Since Au is excellent in corrosion resistance, it is possible to form the semi-reflective layer by itself, whereas Ag and Cu are inferior in corrosion resistance to Au, so it is difficult to form the semi-reflective layer by itself. Therefore, when the semi-reflective layer is composed of a thin film mainly composed of Ag, Cu, or an alloy thereof, in order to improve the corrosion resistance, one or more elements from the following element groups should be added to the semi-reflective layer. Is preferred.

【0020】耐食性を向上させる元素としてはAu、P
t、Pd、Rh、Mo、Ta、Tiが効果的であり、添
加濃度としては0.5原子%以上10原子%以下程度が
適当である。また、Au、Ag、Cuはいずれも熱伝導
度が高いため、これらを半反射層として用いると、磁性
層の熱が半反射層に逃げることになり、記録感度の低下
を引き起こす。
As elements for improving the corrosion resistance, Au and P
t, Pd, Rh, Mo, Ta, and Ti are effective, and the addition concentration is preferably 0.5 atomic% or more and 10 atomic% or less. Further, since Au, Ag, and Cu all have high thermal conductivity, when these are used as the semi-reflective layer, the heat of the magnetic layer escapes to the semi-reflective layer, causing a decrease in recording sensitivity.

【0021】従って、記録感度の向上を望む場合は、熱
伝導度を低減するために半反射層に次に挙げる元素を添
加するのが好ましい。熱伝導度を低減させる元素として
はTi、V、Cr、Mn、Fe、Co、Ni、Zr、N
b、Mo、Ta、W、Hf、Biが挙げられる。本発明
では磁性層に対して半反射層と反対側に反射層を設け
る。
Therefore, when it is desired to improve the recording sensitivity, it is preferable to add the following elements to the semi-reflective layer in order to reduce the thermal conductivity. The elements that reduce the thermal conductivity are Ti, V, Cr, Mn, Fe, Co, Ni, Zr and N.
b, Mo, Ta, W, Hf and Bi are mentioned. In the present invention, the reflective layer is provided on the side opposite to the semi-reflective layer with respect to the magnetic layer.

【0022】即ち、半反射層と反射層で磁性層を挟む構
成とする。半反射層と磁性層の間、磁性層と反射層の間
のいずれか、あるいは両方に誘電体等からなる光干渉層
を設けてもよい。反射層は半反射層と磁性層を透過して
きた光源からの光を反射して、再び磁性層に戻す役割を
担う。
That is, the magnetic layer is sandwiched between the semi-reflective layer and the reflective layer. An optical interference layer made of a dielectric or the like may be provided between the semi-reflective layer and the magnetic layer, between the magnetic layer and the reflective layer, or both. The reflective layer plays a role of reflecting light from the light source that has passed through the semi-reflective layer and the magnetic layer and returning it to the magnetic layer.

【0023】従って、反射層としてはそれに接する層、
即ち磁性層あるいは光干渉層に対する反射率が高いのが
望ましく、Al、Au、Ag、Cuを主体とする薄膜で
構成するのが好ましい。波長が600nm未満では、A
uおよびCuの磁性層あるいは光干渉層にたいする反射
率が低下するため、反射層として用いるのは適当でな
い。
Therefore, the reflective layer is a layer in contact with it,
That is, it is desirable that the reflectance with respect to the magnetic layer or the optical interference layer is high, and it is preferable that the thin film is mainly composed of Al, Au, Ag, and Cu. If the wavelength is less than 600 nm, A
It is not suitable for use as a reflective layer because the reflectance of the magnetic layer or optical interference layer of u and Cu decreases.

【0024】波長が600nm未満の場合にはAlある
いはAgを主体とする薄膜を反射層として用いるのが好
ましい。半反射層と同様、耐食性を向上させるため、あ
るいは熱伝導度を低減するために、先に述べたような元
素を反射層に添加してもよい。反射層の厚みとしては5
0nm程度が一般的である。
When the wavelength is less than 600 nm, it is preferable to use a thin film mainly composed of Al or Ag as the reflective layer. Similar to the semi-reflective layer, the above-mentioned elements may be added to the reflective layer in order to improve the corrosion resistance or reduce the thermal conductivity. The thickness of the reflective layer is 5
Generally about 0 nm.

【0025】光干渉層はその界面で反射した光とその界
面を透過して別な界面で反射してきた光の位相差を変化
させる役割を担い、その位相差によって反射率等が変化
することになる。光干渉層は光を透過するため、使用す
る光源の波長で吸収係数が小さいことが望まれ、一般的
には窒化珪素等の透明な誘電体が用いられる。
The optical interference layer plays a role of changing the phase difference between the light reflected at the interface and the light transmitted through the interface and reflected at another interface, and the reflectance and the like change depending on the phase difference. Become. Since the light interference layer transmits light, it is desired that the absorption coefficient is small at the wavelength of the light source used, and a transparent dielectric such as silicon nitride is generally used.

【0026】光干渉層の屈折率は干渉効果を支配し、屈
折率が大きいほど干渉効果が大きくなる。一般的には屈
折率が2.2程度のものが光干渉層として用いられてい
る。本発明の光磁気記録信号の再生方法は磁性層に達し
て戻ってくる光を半反射層で反射されて戻ってくる光で
ホモダイン検波することを特徴とする。
The refractive index of the light interference layer dominates the interference effect, and the larger the refractive index, the greater the interference effect. Generally, a material having a refractive index of about 2.2 is used as an optical interference layer. The method of reproducing a magneto-optical recording signal of the present invention is characterized in that homodyne detection is performed on light returning to the magnetic layer and reflected by the semi-reflective layer.

【0027】磁性層まで達して戻ってきた光と半反射層
で反射された光の位相差は媒体上のどの位置でも一定に
保たれなければならないが、本発明においては磁性層と
半反射層の間の層、即ち光干渉層の厚みが大きく変化し
なければ位相差はほぼ一定に保たれる。
The phase difference between the light reaching the magnetic layer and returning to the magnetic layer and the light reflected by the semi-reflective layer must be kept constant at any position on the medium, but in the present invention, the magnetic layer and the semi-reflective layer are used. If the thickness of the layer between them, that is, the thickness of the optical interference layer does not change significantly, the phase difference is kept substantially constant.

【0028】[0028]

【実施例】以下に、実施例を挙げて本発明を具体的に説
明するが、本発明はその要旨を越えない限り、以下の実
施例に限定されるものではない。 実施例1 厚さ1.2mmのポリカーボネートディスク基体上にま
ず半反射層として厚さ17nmのAu膜をスパッタ法で
設けた。
EXAMPLES The present invention will be specifically described below with reference to examples, but the present invention is not limited to the following examples as long as the gist thereof is not exceeded. Example 1 First, an Au film having a thickness of 17 nm was provided as a semi-reflective layer on a polycarbonate disk substrate having a thickness of 1.2 mm by a sputtering method.

【0029】更に、光干渉層として厚さ120nmの酸
化タンタル膜を、磁性層として厚さ25nmのTbFe
Co非晶質合金膜を、再び光干渉層として厚さ40nm
の酸化タンタル膜を、それぞれスパッタ法によって設け
た。最後に反射層として厚さ50nmのAl膜をスパッ
タ法により設けて光磁気記録媒体とした。
Further, a tantalum oxide film having a thickness of 120 nm is used as an optical interference layer, and TbFe having a thickness of 25 nm is used as a magnetic layer.
The Co amorphous alloy film is again used as an optical interference layer having a thickness of 40 nm.
The tantalum oxide film of was formed by the sputtering method. Finally, an Al film having a thickness of 50 nm was provided as a reflective layer by a sputtering method to obtain a magneto-optical recording medium.

【0030】半反射層の直後に設けた光干渉層は波長7
80nmでカー回転角が最大となるよう120nmとし
た。分光光度計により反射率を、偏波面変調法によりカ
ー回転角をそれぞれ測定した。測定波長は780nmと
した。この実施例のように、基体を透過させて光を入射
させる構成の光磁気記録媒体の場合、基体表面でも反射
が起こるが、この反射光は実際の信号には寄与しないの
で、反射率およびカー回転角に対する基体表面での反射
光の寄与を計算により除いて反射率とカー回転角を求め
た。表1に結果を示す。
The light interference layer provided immediately after the semi-reflective layer has a wavelength of 7
It was set to 120 nm so that the Kerr rotation angle became maximum at 80 nm. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method. The measurement wavelength was 780 nm. In the case of a magneto-optical recording medium having a structure in which light is transmitted through a substrate as in this embodiment, reflection also occurs on the surface of the substrate, but since this reflected light does not contribute to the actual signal, the reflectance and the curve The reflectance and Kerr rotation angle were obtained by removing the contribution of the reflected light on the substrate surface to the rotation angle by calculation. The results are shown in Table 1.

【0031】比較例1 半反射層を設けない以外は実施例1と同様の方法でディ
スクを作製し、光磁気記録媒体とした。但し、基体上に
直接設ける光干渉層の厚みは波長780nmでカー回転
角が最大になるよう60nmとした。分光光度計により
反射率を、偏波面変調法によりカー回転角をそれぞれ測
定した。測定波長は780nmとした。この比較例のよ
うに、基体を透過させて光を入射させる構成の光磁気記
録媒体の場合、基体表面でも反射が起こるが、この反射
光は実際の信号には寄与しないので、反射率およびカー
回転角に対する基体表面での反射光の寄与を計算により
除いて反射率とカー回転角を求めた。表1に結果を示
す。
Comparative Example 1 A disk was prepared in the same manner as in Example 1 except that the semi-reflective layer was not provided, and used as a magneto-optical recording medium. However, the thickness of the optical interference layer provided directly on the substrate was set to 60 nm so that the Kerr rotation angle was maximized at a wavelength of 780 nm. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method. The measurement wavelength was 780 nm. In the case of a magneto-optical recording medium having a structure in which light is made incident through a substrate as in this comparative example, reflection also occurs at the substrate surface, but this reflected light does not contribute to the actual signal, so the reflectance and curve The reflectance and Kerr rotation angle were obtained by removing the contribution of the reflected light on the substrate surface to the rotation angle by calculation. The results are shown in Table 1.

【0032】比較例2 半反射層をAl膜6nmとした以外は実施例1と同様の
方法でディスクを作製し、光磁気記録媒体とした。半反
射層の直後に設ける光干渉層は波長780nmでカー回
転角が最大となるよう120nmとした。分光光度計に
より反射率を、偏波面変調法によりカー回転角をそれぞ
れ測定した。
Comparative Example 2 A disk was prepared in the same manner as in Example 1 except that the semi-reflective layer was an Al film having a thickness of 6 nm to obtain a magneto-optical recording medium. The light interference layer provided immediately after the semi-reflective layer was set to 120 nm so that the Kerr rotation angle was maximized at a wavelength of 780 nm. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method.

【0033】測定波長は780nmとした。この比較例
のように、基体を透過させて光を入射させる構成の光磁
気記録媒体の場合、基体表面でも反射が起こるが、この
反射光は実際の信号には寄与しないので、反射率および
カー回転角に対する基体表面での反射光の寄与を計算に
より除いて反射率とカー回転角を求めた。表1に結果を
示す。
The measuring wavelength was 780 nm. In the case of a magneto-optical recording medium having a structure in which light is made incident through a substrate as in this comparative example, reflection also occurs at the substrate surface, but this reflected light does not contribute to the actual signal, so the reflectance and curve The reflectance and Kerr rotation angle were obtained by removing the contribution of the reflected light on the substrate surface to the rotation angle by calculation. The results are shown in Table 1.

【0034】実施例2 半反射層をAg膜19nmとした以外は実施例1と同様
の方法でディスクを作製し、光磁気記録媒体とした。但
し、半反射層の直後に設ける光干渉層は波長450nm
でカー回転角が最大となるよう52nmとした。分光光
度計により反射率を、偏波面変調法によりカー回転角を
それぞれ測定した。
Example 2 A disk was prepared in the same manner as in Example 1 except that the semi-reflective layer was an Ag film having a thickness of 19 nm, and was used as a magneto-optical recording medium. However, the light interference layer provided immediately after the semi-reflective layer has a wavelength of 450 nm.
Therefore, the Kerr rotation angle was set to 52 nm so as to be maximum. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method.

【0035】測定波長は450nmとした。この実施例
のように、基体を透過させて光を入射させる構成の光磁
気記録媒体の場合、基体表面でも反射が起こるが、この
反射光は実際の信号には寄与しないので、反射率および
カー回転角に対する基体表面での反射光の寄与を計算に
より除いて反射率とカー回転角を求めた。表1に結果を
示す。
The measurement wavelength was 450 nm. In the case of a magneto-optical recording medium having a structure in which light is transmitted through a substrate as in this embodiment, reflection also occurs on the surface of the substrate, but since this reflected light does not contribute to the actual signal, the reflectance and the curve The reflectance and Kerr rotation angle were obtained by removing the contribution of the reflected light on the substrate surface to the rotation angle by calculation. The results are shown in Table 1.

【0036】比較例3 基体上に直接設ける光干渉層の厚みを波長450nmで
カー回転角が最大になるよう38nmとした以外は比較
例1と同様の方法でディスクを作製し光磁気記録媒体と
した。分光光度計により反射率を、偏波面変調法により
カー回転角をそれぞれ測定した。
Comparative Example 3 A disk was prepared in the same manner as in Comparative Example 1 except that the thickness of the optical interference layer provided directly on the substrate was set to 38 nm so that the Kerr rotation angle was maximized at a wavelength of 450 nm and used as a magneto-optical recording medium. did. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method.

【0037】測定波長は450nmとした。この比較例
のように、基体を透過させて光を入射させる構成の光磁
気記録媒体の場合、基体表面でも反射が起こるが、この
反射光は実際の信号には寄与しないので、反射率および
カー回転角に対する基体表面での反射光の寄与を計算に
より除いて反射率とカー回転角を求めた。表1に結果を
示す。
The measurement wavelength was 450 nm. In the case of a magneto-optical recording medium having a structure in which light is made incident through a substrate as in this comparative example, reflection also occurs at the substrate surface, but this reflected light does not contribute to the actual signal, so the reflectance and curve The reflectance and Kerr rotation angle were obtained by removing the contribution of the reflected light on the substrate surface to the rotation angle by calculation. The results are shown in Table 1.

【0038】実施例3 厚さ20μmのPETフィルム基体上にまず反射層とし
て厚さ50nmのAl膜をスパッタ法により形成した。
更に光干渉層として厚さ40nmの酸化タンタル膜を、
磁性層として厚さ25nmのTbFeCo非晶質合金膜
を、再び光干渉層として厚さ116nmの酸化タンタル
膜を、それぞれスパッタ法によって設けた。
Example 3 An Al film having a thickness of 50 nm was first formed as a reflective layer on a PET film substrate having a thickness of 20 μm by a sputtering method.
Furthermore, a 40 nm thick tantalum oxide film is used as an optical interference layer.
A TbFeCo amorphous alloy film having a thickness of 25 nm was provided as a magnetic layer, and a tantalum oxide film having a thickness of 116 nm was provided again as an optical interference layer by a sputtering method.

【0039】最後に半反射層として厚さ14nmのAu
膜をスパッタ法により設けて光磁気記録媒体とした。半
反射層の直前に設ける光干渉層は波長780nmでカー
回転角が最大となるよう116nmとした。分光光度計
により反射率を、偏波面変調法によりカー回転角をそれ
ぞれ測定した。測定波長は780nmとした。表1に結
果を示す。
Finally, as a semi-reflective layer, Au having a thickness of 14 nm is used.
The film was provided by a sputtering method to obtain a magneto-optical recording medium. The light interference layer provided immediately before the semi-reflective layer was set to 116 nm so that the Kerr rotation angle was maximized at a wavelength of 780 nm. The reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method. The measurement wavelength was 780 nm. The results are shown in Table 1.

【0040】比較例4 半反射層を設けないこと以外は実施例3と同様の方法で
光磁気記録媒体を作製した。
Comparative Example 4 A magneto-optical recording medium was prepared in the same manner as in Example 3 except that the semi-reflective layer was not provided.

【0041】最後に設ける光干渉層は波長780nmで
カー回転角が最大となるよう60nmとした。信号品質
を比較するために、分光光度計により反射率を、偏波面
変調法によりカー回転角をそれぞれ測定した。測定波長
は780nmとした。表1に結果を示す。
The final optical interference layer was set to 60 nm to maximize the Kerr rotation angle at a wavelength of 780 nm. In order to compare the signal quality, the reflectance was measured by a spectrophotometer and the Kerr rotation angle was measured by a polarization plane modulation method. The measurement wavelength was 780 nm. The results are shown in Table 1.

【0042】[0042]

【表1】 [Table 1]

【0043】実施例1は十分高い反射率を示すと同時
に、大きなカー回転角を示している。それに対して、比
較例1の場合はカー回転角は大きいが反射率が十分に高
いとは言えないし、比較例2は反射率は高いがカー回転
角は実施例の半分以下である。このことから、高い反射
率を得るには半反射層を設けることが重要であること、
および、高反射率と大きなカー回転角を両立させるため
には半反射膜をAu、Ag、Cuの中から選ばれる1元
素あるいは2元素以上を主体とする薄膜で構成すること
が重要であることが理解できる
Example 1 shows a sufficiently high reflectance and a large Kerr rotation angle. On the other hand, in the case of Comparative Example 1, the Kerr rotation angle is large but the reflectance cannot be said to be sufficiently high. In Comparative Example 2, the reflectance is high but the Kerr rotation angle is half or less of that of the embodiment. From this, it is important to provide a semi-reflective layer in order to obtain high reflectance,
Further, in order to achieve both high reflectance and a large Kerr rotation angle, it is important that the semi-reflective film is composed of a thin film mainly containing one element or two or more elements selected from Au, Ag and Cu. Can understand

【0044】実施例2と比較例3より、短波長領域では
半反射層を設けないと十分な反射率を得ることが困難で
あることが分かり、半反射層は短波長領域で非常に効果
的であることが分かる。実施例3と比較例4より、光干
渉層に直接光を入射する場合も高反射率を得ることが困
難であり、このような場合にも半反射層が特に効果的で
あることが分かる。
From Example 2 and Comparative Example 3, it was found that it is difficult to obtain a sufficient reflectance in the short wavelength region unless the semi-reflective layer is provided, and the semi-reflective layer is very effective in the short wavelength region. It turns out that From Example 3 and Comparative Example 4, it can be seen that it is difficult to obtain high reflectance even when light is directly incident on the light interference layer, and even in such a case, the semi-reflective layer is particularly effective.

【0045】[0045]

【発明の効果】本発明によればショットノイズ限界の再
生を行うのに十分な反射率と大きなカー回転角を示す光
磁気記録媒体を提供できる。
According to the present invention, it is possible to provide a magneto-optical recording medium exhibiting a reflectance and a large Kerr rotation angle sufficient for reproducing shot noise limit.

───────────────────────────────────────────────────── フロントページの続き (72)発明者 島守 巧美 神奈川県横浜市緑区鴨志田町1000番地 三 菱化成株式会社総合研究所内 ─────────────────────────────────────────────────── ─── Continuation of the front page (72) Inventor Takumi Shimamori Sanboshi Kasei Co., Ltd. Research Institute, 1000, Kamoshida-cho, Midori-ku, Yokohama-shi, Kanagawa

Claims (5)

【特許請求の範囲】[Claims] 【請求項1】 基体上に少なくとも磁性層と該磁性層よ
りも光源に近い側に光源からの光の一部を反射し他を透
過する半反射層と、磁性層より光源から遠い側に光源か
らの光を反射する反射層をそれぞれ有する光磁気記録媒
体において、該半反射層がAu、Ag、Cuの中から選
ばれる1元素あるいは2元素以上を主体とする薄膜から
なることを特徴とする光磁気記録媒体。
1. A magnetic layer at least on a substrate, a semi-reflective layer that reflects a part of light from a light source and transmits the other to a side closer to the light source than the magnetic layer, and a light source farther from the light source than the magnetic layer. In the magneto-optical recording medium, each of which has a reflective layer for reflecting the light from, the semi-reflective layer is composed of a thin film mainly containing one element or two or more elements selected from Au, Ag and Cu. Magneto-optical recording medium.
【請求項2】 半反射層がAgを主体とする薄膜からな
ることを特徴とする請求項1に記載の光磁気記録媒体。
2. The magneto-optical recording medium according to claim 1, wherein the semi-reflective layer is a thin film containing Ag as a main component.
【請求項3】 半反射層の厚みが5nm以上40nm以
下であることを特徴とする請求項1および請求項2に記
載の光磁気記録媒体。
3. The magneto-optical recording medium according to claim 1, wherein the semi-reflective layer has a thickness of 5 nm or more and 40 nm or less.
【請求項4】 請求項1、請求項2および請求項3に記
載の光磁気記録媒体を用い、磁性層まで達して戻ってき
た光を半反射層で反射されて戻ってきた光でホモダイン
検波することを特徴とする光磁気記録信号の再生方法。
4. The magneto-optical recording medium according to claim 1, claim 2 or claim 3, wherein the light returning to the magnetic layer is reflected by the semi-reflective layer and returned by homodyne detection. A method for reproducing a magneto-optical recording signal, comprising:
【請求項5】 情報の記録再生を行う光を基体と逆側か
ら磁性層に入射するのに適した層構成を有することを特
徴とする請求項4に記載光磁気信号の再生方法。
5. The method of reproducing a magneto-optical signal according to claim 4, having a layer structure suitable for allowing light for recording / reproducing information to enter the magnetic layer from the side opposite to the substrate.
JP10680594A 1994-05-20 1994-05-20 Magneto-optical recording medium and reproducing method thereof Pending JPH07320324A (en)

Priority Applications (1)

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Application Number Priority Date Filing Date Title
JP10680594A JPH07320324A (en) 1994-05-20 1994-05-20 Magneto-optical recording medium and reproducing method thereof

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Publication Number Publication Date
JPH07320324A true JPH07320324A (en) 1995-12-08

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Country Link
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Cited By (6)

* Cited by examiner, † Cited by third party
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US7291374B2 (en) 1998-06-22 2007-11-06 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
US7314657B2 (en) 2000-07-21 2008-01-01 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
US7314660B2 (en) 2000-07-21 2008-01-01 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
US7314659B2 (en) 2000-07-21 2008-01-01 Target Technology Company, Llc Metal alloys for the reflective or semi-reflective layer of an optical storage medium
US7316837B2 (en) 2000-07-21 2008-01-08 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
US7374805B2 (en) 2000-07-21 2008-05-20 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium

Cited By (7)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US7291374B2 (en) 1998-06-22 2007-11-06 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
US7384677B2 (en) 1998-06-22 2008-06-10 Target Technology Company, Llc Metal alloys for the reflective or semi-reflective layer of an optical storage medium
US7314657B2 (en) 2000-07-21 2008-01-01 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
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US7314659B2 (en) 2000-07-21 2008-01-01 Target Technology Company, Llc Metal alloys for the reflective or semi-reflective layer of an optical storage medium
US7316837B2 (en) 2000-07-21 2008-01-08 Target Technology Company, Llc Metal alloys for the reflective or the semi-reflective layer of an optical storage medium
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