JPH08306029A - Magnetic recording media - Google Patents

Magnetic recording media

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Publication number
JPH08306029A
JPH08306029A JP12944395A JP12944395A JPH08306029A JP H08306029 A JPH08306029 A JP H08306029A JP 12944395 A JP12944395 A JP 12944395A JP 12944395 A JP12944395 A JP 12944395A JP H08306029 A JPH08306029 A JP H08306029A
Authority
JP
Japan
Prior art keywords
layer
magnetic
underlayer
ratio
recording medium
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.)
Withdrawn
Application number
JP12944395A
Other languages
Japanese (ja)
Inventor
Takeshi Maro
毅 麿
Kazunori Adachi
和慶 安達
Akito Sakamoto
章人 酒本
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.)
Maxell Ltd
Original Assignee
Hitachi Maxell Ltd
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 Hitachi Maxell Ltd filed Critical Hitachi Maxell Ltd
Priority to JP12944395A priority Critical patent/JPH08306029A/en
Publication of JPH08306029A publication Critical patent/JPH08306029A/en
Withdrawn legal-status Critical Current

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  • Magnetic Record Carriers (AREA)

Abstract

PURPOSE: To obtain a magnetic recording medium ensuring low modulation noise and having a superior S-N ratio by regulating the ratio of the average grain diameter of magnetic grains constituting a magnetic layer to that of grains constituting an underlayer to a prescribed value. CONSTITUTION: An SiO2 , layer 2, a Cr layer 31, a Co75 Cr10 Pt15 alloy layer 41, an amorphous carbon film 5 and a lubricative layer 6 are formed on an amorphous olefin resin substrate 1 to obtain the objective magnetic disk. The SiO2 layer 2 is a layer for increasing the mechanical strength of the surface of the substrate 1. The Cr layer 31 is an underlayer and this underlayer 31 is columnar. The CoCrPt layer 41 covers the tops of the columnar crystals of the Cr underlayer 31. The ratio (Y/X) of the average grain diameter Y of magnetic grains constituting the magnetic layer 41 to that X of grains constituting the underlayer 31 is 0.4-0.9. The resultant medium ensures low modulation noise and has a superior S-N ratio, and high density recording is performed by using this medium.

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、磁気記録媒体に関し、
さらに詳細には合金薄膜を磁性層とする高密度磁気記録
媒体に関する。
BACKGROUND OF THE INVENTION 1. Field of the Invention The present invention relates to a magnetic recording medium,
More specifically, it relates to a high-density magnetic recording medium having an alloy thin film as a magnetic layer.

【0002】[0002]

【従来の技術】近年の情報量の増加及び情報化機器の小
型化に伴ない、磁気記録の分野でも益々高記録密度記録
が可能な磁気記録媒体が求められている。このような要
望に応えるべく、合金薄膜を磁性層とした媒体が開発さ
れ、従来の塗布型媒体に代わって市場において主流とな
りつつある。合金薄膜媒体は、メッキ法またはスパッタ
法で作製することができるため、磁性層の厚さを塗布型
媒体の厚さの約1/20〜1/10にすることができ
る。これにより、微小磁区の反磁界が小さくなり、高記
録密度でも出力が劣化しないという利点を有する。
2. Description of the Related Art With the recent increase in the amount of information and the miniaturization of information-oriented devices, there is a demand for a magnetic recording medium capable of recording with even higher recording density in the field of magnetic recording. In order to meet such demands, a medium having an alloy thin film as a magnetic layer has been developed and is becoming the mainstream in the market in place of the conventional coating type medium. Since the alloy thin film medium can be manufactured by the plating method or the sputtering method, the thickness of the magnetic layer can be set to about 1/20 to 1/10 of the thickness of the coating medium. This has the advantage that the demagnetizing field of the minute magnetic domains is reduced and the output does not deteriorate even at high recording density.

【0003】[0003]

【発明が解決しようとする課題】しかしながら、合金薄
膜媒体では、塗布型媒体とは異なり、微小磁区の分離が
十分でないため、書き込み周波数近傍でのノイズ(変調
ノイズ)が増大するという欠点がある。図1に従来の合
金薄膜媒体の微小磁区により形成された異なる磁化の境
界近傍の拡大図を示す。図1に示すように異なる磁化が
向かい合う磁化境界部は、媒体の幅方向に沿って鋸波状
となるために、再生時には変調ノイズとして現れる。こ
のため、現行の合金薄膜媒体をさらに高記録密度化する
場合には、不十分な磁化の区分に基づく変調ノイズを低
下することが要求される。
However, unlike the coating type medium, the alloy thin film medium has a drawback that the noise (modulation noise) in the vicinity of the writing frequency increases because the separation of the fine magnetic domains is not sufficient. FIG. 1 shows an enlarged view of the vicinity of the boundary of different magnetizations formed by minute magnetic domains of a conventional alloy thin film medium. As shown in FIG. 1, the magnetization boundary portion where different magnetizations face each other has a sawtooth shape along the width direction of the medium, and therefore appears as modulation noise during reproduction. Therefore, in order to further increase the recording density of the current alloy thin film medium, it is required to reduce the modulation noise due to insufficient magnetization division.

【0004】本発明は、上記従来技術の合金薄膜媒体が
持つ変調ノイズを低下し、高密度記録が可能な磁気記録
媒体を提供することを目的とする。
It is an object of the present invention to provide a magnetic recording medium capable of high density recording by reducing the modulation noise of the above-mentioned prior art alloy thin film medium.

【0005】[0005]

【課題を解決するための手段】本発明者は、粒若しくは
柱状構造を有する下地層上に磁性層を成長させる際に、
下地層の粒若しくは柱状晶を十分に大きく成長させその
上に微小な磁性粒からなる磁性層を形成するさせること
により、信号強度を損なうことなくノイズを低下するこ
とができることを見い出した。すなわち、本発明に従え
ば、基体上に下地層及び磁性層を積層した磁気記録媒体
において、上記下地層を構成する粒子の平均粒径Xに対
する上記磁性層を構成する磁性粒子の平均粒径Yの比Y
/Xが、0.4≦Y/X≦0.9であることを特徴とす
る上記磁気記録媒体が提供される。
The present inventors have found that when a magnetic layer is grown on an underlayer having a grain or columnar structure,
It has been found that the noise can be reduced without deteriorating the signal strength by growing sufficiently large grains or columnar crystals of the underlayer and forming a magnetic layer made of fine magnetic grains on the grains. That is, according to the present invention, in a magnetic recording medium in which an underlayer and a magnetic layer are laminated on a substrate, the average particle size Y of the magnetic particles forming the magnetic layer is larger than the average particle size X of the particles forming the underlayer. Ratio of
There is provided the above magnetic recording medium, wherein / X is 0.4 ≦ Y / X ≦ 0.9.

【0006】かかる比Y/Xに従って下地層の粒径より
も小さい粒径の磁性層を設けることによって、磁気記録
媒体の変調ノイズを有効に低減することができる。Y/
Xが0.4未満である場合またはY/Xが0.9を超え
ると、S/N比が低下するため好ましくない。特に、Y
/Xが0.4未満である場合には熱ゆらぎの問題が生じ
るため好ましくない。
The modulation noise of the magnetic recording medium can be effectively reduced by providing the magnetic layer having a grain size smaller than that of the underlayer according to the ratio Y / X. Y /
When X is less than 0.4 or when Y / X exceeds 0.9, the S / N ratio decreases, which is not preferable. Especially Y
When / X is less than 0.4, there is a problem of thermal fluctuation, which is not preferable.

【0007】上記本発明の磁気記録媒体において、下地
層を構成する粒子は、一般に粒若しくは柱状晶の形態で
あり、その平均粒径XはX≧15nmであることが好ま
しい。下地層の平均粒径Xが15nm未満であると、下
地層の粒若しくは柱状晶の結晶性が低下するため、その
上に磁性層が成長しにくくなるとともに、成長した磁性
層の結晶配向が悪化して信号強度が小さくなる。磁性層
の粒径Yの範囲としては、上記磁性層の粒径Yと下地層
の粒径XとのY/X比及び前記下地層Xの粒径範囲の下
限により定まる。
In the above-mentioned magnetic recording medium of the present invention, the particles forming the underlayer are generally in the form of particles or columnar crystals, and the average particle size X is preferably X ≧ 15 nm. If the average grain size X of the underlayer is less than 15 nm, the crystallinity of the grains or columnar crystals of the underlayer is lowered, so that it becomes difficult for the magnetic layer to grow thereon, and the crystal orientation of the grown magnetic layer deteriorates. As a result, the signal strength decreases. The range of the grain size Y of the magnetic layer is determined by the Y / X ratio between the grain size Y of the magnetic layer and the grain size X of the underlayer and the lower limit of the grain range of the underlayer X.

【0008】上記構造の磁気記録媒体は、スパッタ法に
より形成することができ、非磁性基板上に下地層を低ス
パッタガス圧及び高基板温度の条件下、上層の磁性層を
高スパッタガス圧及び下地層形成時より低い基板温度条
件下で形成することができ、負のバイアス電圧を印加し
たり、スパッタガスの酸素、窒素ガスを添加してもよ
い。これらの方法を単独または組み合わせて形成するこ
ともできる。上記磁性層と下地層の平均粒径の比Y/X
は、スパッタガス流量及びガス圧等を適宜調整すること
によって本発明の範囲にすることができる。
The magnetic recording medium having the above structure can be formed by a sputtering method. An underlayer is formed on a non-magnetic substrate under conditions of low sputtering gas pressure and high substrate temperature, and an upper magnetic layer is formed under high sputtering gas pressure. It can be formed under a substrate temperature condition lower than that at the time of forming the underlayer, and a negative bias voltage may be applied or oxygen or nitrogen gas as a sputtering gas may be added. These methods may be used alone or in combination. Ratio Y / X of the average particle size of the magnetic layer and the underlayer
Can be within the scope of the present invention by appropriately adjusting the flow rate and gas pressure of the sputtering gas.

【0009】下地層に用いられる材料としては、例え
ば、Cr,CrTi,CrW,CrTa,CrAl,C
rAg等のCr系合金、Ti,Ti−Taが挙げられる
が、特にこれらに限定されず磁気記録媒体の下地層に使
用できる種々の材料を用い得る。磁性材料として、例え
ば、CoCr,CoCrTa,CoCrPt,CoCr
PtTa,CoPt,CoPd,CoCrPtSi,C
oCrPtB等のCo系合金、CoやFeをSiO2
同時にスパッタし、Co,Fe粒子を分散させた複合材
料等が挙げられるが、特にこれらに限定されない。磁性
層はCoNi系合金以外の材料から構成されていてもよ
い。これら下地層及び磁性層は、上記のようにスパッタ
法や真空蒸着法等で容易に形成することができる。
The material used for the underlayer is, for example, Cr, CrTi, CrW, CrTa, CrAl, C.
Examples thereof include Cr-based alloys such as rAg, Ti and Ti-Ta, but various materials that can be used for the underlayer of the magnetic recording medium are not particularly limited to these. As the magnetic material, for example, CoCr, CoCrTa, CoCrPt, CoCr
PtTa, CoPt, CoPd, CoCrPtSi, C
Examples thereof include Co-based alloys such as oCrPtB, composite materials in which Co and Fe are sputtered at the same time as SiO 2 , and Co and Fe particles are dispersed, but are not particularly limited thereto. The magnetic layer may be made of a material other than the CoNi-based alloy. The underlayer and the magnetic layer can be easily formed by the sputtering method, the vacuum deposition method or the like as described above.

【0010】本発明の磁気記録媒体に用いられる基体と
しては、例えば、Al,NiPメッキしたAl、ガラ
ス、セラミックス、カーボン、高分子材料、例えば、ポ
リカーボネート、アモルファスポリオレフィン、エポキ
シ、ポリアミド、ポリイミド、ポリエチレンテレフタレ
ート、ナイロン等を用いることができる。
The substrate used in the magnetic recording medium of the present invention is, for example, Al, NiP-plated Al, glass, ceramics, carbon, a polymeric material such as polycarbonate, amorphous polyolefin, epoxy, polyamide, polyimide, polyethylene terephthalate. , Nylon, etc. can be used.

【0011】以下、本発明を実施例により詳細に説明す
るが、本発明はそれらに限定されるものではない。
Hereinafter, the present invention will be described in detail with reference to Examples, but the present invention is not limited thereto.

【0012】[0012]

【実施例】【Example】

実施例1 本実施例では、連続スパッタ装置を用いて、SiO2
Cr/CoCrPt/カーボンの4層からなる記録層を
基体の両面に積層した磁気ディスクを作製する。図3に
示したような、基板の両面に同時スパッタできる連続ス
パッタ装置を用いてアモルファスポリオレフィン基板上
に4層記録膜を成膜した。このスパッタ装置は、予備排
気室7、SiO2 成膜室8、Cr成膜室9、CoCrP
t成膜室10及びカーボン成膜室11がこの順序でゲー
トバルブ13を通じて連結されている。成膜中はゲート
バルブ13を閉めることにより、各成膜室は隣設する成
膜室から隔離される。各成膜室にはそれぞれクライオポ
ンプ12が装着されており、スパッタ雰囲気ガスとして
アルゴンガス及びその混合ガスが流入される。アモルフ
ァスポリオレフィン基板は、専用のトレーで各成膜室に
順次搬送される。SiO2 成膜室にはSiターゲット、
Cr成膜室にはCrターゲット、CoCrPt成膜室に
はCo75Cr10Pt15合金ターゲット、カーボン成膜室
にはカーボンターゲットが、各2枚、基板通過位置を挟
んで互いに対向するように取り付けられており、この2
枚のターゲット間を基板を通過させることにより同時に
両面に成膜が行われる。このスパッタ装置に基板を入れ
る前、全成膜室を到達真空度が1×10-5Paとなるま
で排気しておいた。
Example 1 In this example, a continuous sputtering apparatus was used to obtain SiO 2 /
A magnetic disk is manufactured in which four recording layers of Cr / CoCrPt / carbon are laminated on both sides of a substrate. A four-layer recording film was formed on an amorphous polyolefin substrate using a continuous sputtering apparatus capable of simultaneously sputtering both surfaces of the substrate as shown in FIG. This sputtering apparatus includes a preliminary exhaust chamber 7, a SiO 2 film forming chamber 8, a Cr film forming chamber 9, and CoCrP.
The t film forming chamber 10 and the carbon film forming chamber 11 are connected in this order through the gate valve 13. By closing the gate valve 13 during film formation, each film formation chamber is isolated from the adjacent film formation chamber. A cryopump 12 is attached to each film forming chamber, and argon gas and a mixed gas thereof are introduced as a sputtering atmosphere gas. The amorphous polyolefin substrate is sequentially transferred to each film forming chamber by a dedicated tray. Si target in the SiO 2 film forming chamber,
A Cr target is set in the Cr film forming chamber, a Co 75 Cr 10 Pt 15 alloy target is set in the CoCrPt film forming chamber, and two carbon targets are installed in the carbon film forming chamber so that they face each other across the substrate passing position. This is 2
A film is formed on both surfaces at the same time by passing the substrate between the targets. Before the substrate was put into this sputtering apparatus, all the film forming chambers were evacuated until the ultimate vacuum reached 1 × 10 −5 Pa.

【0013】予備排気室7内のトレーに基板を設置した
後、真空度が1×10-4Paとなるまで予備排気室7を
排気した。次に、トレーをSiO2 成膜室8に移しアモ
ルフォスポリオレフィン基板上に高周波反応性スパッタ
によりSiO2 を100nm成膜した。このときの成膜
条件は、Ar流量50sccm、O2 流量20scc
m、ガス圧0.5Pa、投入電力3Kwとした。次い
で、次のCr成膜室9にトレーを搬送し、Cr層を、直
流スパッタにより100nm成膜した。このときの成膜
条件は、Ar50sccm、ガス圧0.4Pa、投入電
力を3Kw、基板設定温度を50℃とした。この温度で
もスパッタ時の基板最高温度は100℃であり、基板が
溶融するというような問題は起こらなかった。このトレ
ーを次のCoCrPt成膜室10に送り、CoCrPt
膜を30nmの膜厚で直流スパッタにより成膜した。こ
のときのスパッタ条件は、Arガス流量100scc
m、ガス圧0.8Pa投入電力3Kwとした。CoCr
Pt膜の成膜時には、基板加熱は行なわなかった。スパ
ッタ時の最高温度は、50℃であった。最後に、カーボ
ン成膜室11内にトレーを移し、カーボン保護膜を10
nmの膜厚で直流スパッタ法により成膜した。この時の
成膜条件は、Arガス流量50sccm、ガス圧0.4
Pa、投入電力3Kwとした。次いで、積層された基板
を装置から取り出し、最上層のカーボン保護膜の上にパ
ーフルオロポリエーテル系の潤滑剤を両面にディプ法で
塗布した。
After the substrate was placed on the tray in the preliminary evacuation chamber 7, the preliminary evacuation chamber 7 was evacuated until the degree of vacuum reached 1 × 10 -4 Pa. Next was 100nm deposited SiO 2 by RF reactive sputtering in Cupid Foss polyolefin substrate transferred tray SiO 2 film formation chamber 8. The film forming conditions at this time are Ar flow rate 50 sccm and O 2 flow rate 20 sccc.
m, gas pressure 0.5 Pa, and input power 3 Kw. Next, the tray was transported to the next Cr film forming chamber 9, and a Cr layer was formed to 100 nm by DC sputtering. The film forming conditions at this time were Ar 50 sccm, gas pressure 0.4 Pa, input power 3 Kw, and substrate setting temperature 50 ° C. Even at this temperature, the maximum temperature of the substrate during sputtering was 100 ° C., and the problem of melting the substrate did not occur. This tray is sent to the next CoCrPt film forming chamber 10,
A film having a thickness of 30 nm was formed by DC sputtering. The sputtering conditions at this time are Ar gas flow rate 100 scc
m, gas pressure 0.8 Pa, input power 3 Kw. CoCr
The substrate was not heated when the Pt film was formed. The maximum temperature during sputtering was 50 ° C. Finally, the tray is moved into the carbon film forming chamber 11 and the carbon protective film 10 is removed.
A film having a thickness of nm was formed by the DC sputtering method. The film forming conditions at this time are Ar gas flow rate of 50 sccm and gas pressure of 0.4.
Pa and input power 3 Kw. Then, the laminated substrates were taken out of the apparatus, and a perfluoropolyether-based lubricant was applied to both surfaces of the uppermost carbon protective film by a dip method.

【0014】こうして得られた本実施例の4層構成の磁
気ディスクの概略断面図を図2に示す。この磁気ディス
クは、アモルファスポリオレフィン樹脂基体上1にSi
2層2,Cr層3,Co75Cr10Pt15合金層4、非
晶質カーボン膜5及び潤滑材層6が形成されている。S
iO2 層2は、基板の表面の機械的強度を上げるための
層であり、その上に形成するCr層3が本発明における
下地層に該当する。
FIG. 2 is a schematic sectional view of the magnetic disk having a four-layer structure of the present embodiment obtained in this way. This magnetic disk consists of an amorphous polyolefin resin substrate 1 with Si
An O 2 layer 2, a Cr layer 3, a Co 75 Cr 10 Pt 15 alloy layer 4, an amorphous carbon film 5 and a lubricant layer 6 are formed. S
The iO 2 layer 2 is a layer for increasing the mechanical strength of the surface of the substrate, and the Cr layer 3 formed thereon corresponds to the underlayer in the present invention.

【0015】得られた磁気ディスクの断面を透過型顕微
鏡で観察したところ、図4に示すように、下地層31は
柱状であり、CoCrPt層41はCr下地層の各柱状
結晶の上面を覆っていることがわかった。
When the cross section of the obtained magnetic disk was observed with a transmission microscope, the underlayer 31 was columnar and the CoCrPt layer 41 covered the upper surface of each columnar crystal of the Cr underlayer as shown in FIG. I found out that

【0016】実施例2 CoCrPt膜の性膜条件をArガス流量200scc
m、ガス圧1.6Paとした以外は、実施例1と同様に
して磁気ディスクを作製した。
Example 2 The CoCrPt film was formed under the following conditions: Ar gas flow rate 200 scc
A magnetic disk was produced in the same manner as in Example 1 except that m and gas pressure were set to 1.6 Pa.

【0017】実施例3 CoCrPt膜の性膜条件をArガス流量300scc
m、ガス圧2.4Paとした以外は、実施例1と同様に
して磁気ディスクを作製した。
Example 3 The condition of the CoCrPt film was set to an Ar gas flow rate of 300 sccc.
A magnetic disk was produced in the same manner as in Example 1 except that m and gas pressure were set to 2.4 Pa.

【0018】実施例4 CoCrPt膜の成膜条件をArガス流量400scc
m、ガス圧3.2Paとした以外は、実施例1と同様に
して磁気ディスクを作製した。
Example 4 The CoCrPt film was formed under the Ar gas flow rate of 400 sccc.
A magnetic disk was produced in the same manner as in Example 1 except that m and gas pressure were 3.2 Pa.

【0019】比較例1 CoCrPt膜の成膜条件をArガス流量50scc
m、ガス圧0.4Paとした以外は、実施例1と同様に
磁気ディスクを作製した。この比較例1の磁気ディスク
は従来使用されている磁気ディスクと同様のものであ
る。
Comparative Example 1 The CoCrPt film was formed under the Ar gas flow rate of 50 scc.
A magnetic disk was produced in the same manner as in Example 1 except that m and gas pressure were 0.4 Pa. The magnetic disk of Comparative Example 1 is the same as the conventionally used magnetic disk.

【0020】比較例2 CoCrPt膜の性膜条件をArガス流量500scc
m、ガス圧4Paとした以外は、実施例1と同様にして
磁気ディスクを作製した。
Comparative Example 2 The CoCrPt film was formed under the following conditions: Ar gas flow rate 500 sccc.
A magnetic disk was produced in the same manner as in Example 1 except that m and gas pressure were 4 Pa.

【0021】実施例1〜4及び比較例1〜2で得られた
磁気ディスクについて、サンプル信号を記録した後、S
/N比を測定した。また、各磁気ディスクについて、下
地層及び磁性層の結晶粒の平均粒径を調べた。S/N比
は、トラック幅8μm、ギャップ長0.4μmのMIG
ヘッドを用いて、線速7m/S、ヘッドの浮上量0.1
μm、線記録密度50kfciでサンプル信号の記録を
行ったあと、トラック幅5μm、ギャップ長0.2μm
の薄膜ヘッドを用いて、線速7m/S、ヘッドの浮上量
0.1μmで再生し、その再生信号をスペクトラムアナ
ライザに取り込んで調べた。下地層及び磁性膜の結晶粒
の平均粒径は、上記例で得られたディスクについてミク
ロトームを用いて断面の超薄切片を作製し、それらを透
過型顕微鏡で観察し、各100個のサンプルから平均値
を求めた。結果を表1に示す。各ディスクの断面を顕微
鏡観察すると、下地層は、どの磁気ディスクも実施例1
で得られた磁気ディスクと同様に図4に示したような柱
状構造であり、その上に磁性粒子が成長する構造である
ことがわかった。
After recording a sample signal on the magnetic disks obtained in Examples 1 to 4 and Comparative Examples 1 and 2, S was recorded.
The / N ratio was measured. Further, for each magnetic disk, the average grain size of the crystal grains of the underlayer and the magnetic layer was examined. The S / N ratio is MIG with a track width of 8 μm and a gap length of 0.4 μm.
Using the head, linear velocity 7 m / S, head flying height 0.1
After recording a sample signal with a line recording density of 50 μm and a linear recording density of 50 kfci, the track width is 5 μm and the gap length is 0.2 μm.
Was reproduced at a linear velocity of 7 m / S and the flying height of the head was 0.1 μm, and the reproduced signal was taken into a spectrum analyzer for examination. The average grain size of the crystal grains of the underlayer and the magnetic film was obtained by making ultra-thin sections of a section of the disc obtained in the above example using a microtome and observing them with a transmission microscope. The average value was calculated. The results are shown in Table 1. When the cross section of each disk is observed with a microscope, the underlayer is the magnetic disk of Example 1
It was found that the magnetic disk had a columnar structure as shown in FIG. 4 similarly to the magnetic disk obtained in the above, and had magnetic particles grown on it.

【0022】[0022]

【表1】 [Table 1]

【0023】表1からわかるように、本発明の実施例に
より得られた磁気ディスクは、下地層に対する磁性層の
平均粒径比Y/Xが0.4〜0.9の範囲内であり、Y
/Xがこの範囲外の比較例に比べてS/N比が優れてい
ることがわかる。このS/N比の改善は主に磁性粒の粒
径が小さくなり、磁性粒の分離が良くなるために変調ノ
イズが低下するためと考えられる。
As can be seen from Table 1, the magnetic disks obtained according to the examples of the present invention had an average particle size ratio Y / X of the magnetic layer to the underlayer within the range of 0.4 to 0.9, Y
It can be seen that the S / N ratio is superior to that of the comparative example in which / X is outside this range. It is considered that the improvement of the S / N ratio is mainly because the particle size of the magnetic particles is reduced and the separation of the magnetic particles is improved, thereby lowering the modulation noise.

【0024】下地層を構成する粒子の平均粒径のS/N
比への影響を調べるために、実施例1の条件においてC
r層の成膜条件を、Arガス流量100sccm、ガス
圧0.8Paとした場合及びArガス流量100scc
m、ガス圧0.8Pa、基板温度25℃とした場合につ
いて磁気ディスクを作製した。それぞれ得られた磁気デ
ィスクの下地層を構成粒子の平均粒径は、13nm及び
10nmであり、各S/N比は実施例1の場合に比べて
低かった。従って、下地層粒子の平均粒径を15nm以
上に維持するのが好ましい。
S / N of average particle size of particles constituting the underlayer
In order to investigate the influence on the ratio, C
When the film formation conditions for the r layer are Ar gas flow rate 100 sccm and gas pressure 0.8 Pa, and Ar gas flow rate 100 sccc
m, a gas pressure of 0.8 Pa, and a substrate temperature of 25 ° C., a magnetic disk was produced. The average particle diameter of the constituent particles of the underlayer of the magnetic disk thus obtained was 13 nm and 10 nm, respectively, and the respective S / N ratios were lower than in the case of Example 1. Therefore, it is preferable to maintain the average particle size of the underlayer particles at 15 nm or more.

【0025】[0025]

【発明の効果】本発明の磁気記録媒体は、変調ノイズが
低く、優れたS/N比を有する。本発明の磁気記録媒体
を用いることにより高密度記録が可能になる。
The magnetic recording medium of the present invention has a low modulation noise and an excellent S / N ratio. High density recording is possible by using the magnetic recording medium of the present invention.

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

【図1】従来の合金薄膜記録媒体の部分拡大平面図であ
り、微小磁区により形成された異なる磁化の境界を概念
的に表している。
FIG. 1 is a partially enlarged plan view of a conventional alloy thin film recording medium, conceptually showing boundaries of different magnetizations formed by minute magnetic domains.

【図2】実施例1で得られた本発明の磁気ディスクの概
略断面図である。
2 is a schematic sectional view of the magnetic disk of the present invention obtained in Example 1. FIG.

【図3】実施例で用いた連続スパッタ装置の概略構成図
である。
FIG. 3 is a schematic configuration diagram of a continuous sputtering apparatus used in Examples.

【図4】実施例1で得られた本発明の磁気ディスクの拡
大断面図である。
FIG. 4 is an enlarged cross-sectional view of the magnetic disk of the present invention obtained in Example 1.

【符号の説明】[Explanation of symbols]

1 基板 2 SiO2 層 3 Cr層 4 CoCrPt合金層 5 カーボン層 6 潤滑材層 7 予備排気室 9 Cr成膜室 12 クライオポンプ 13 ゲートバルブ 31 柱状構造の下地層 41 磁性層の磁性粒DESCRIPTION OF SYMBOLS 1 Substrate 2 SiO 2 layer 3 Cr layer 4 CoCrPt alloy layer 5 Carbon layer 6 Lubricant layer 7 Preliminary exhaust chamber 9 Cr deposition chamber 12 Cryopump 13 Gate valve 31 Columnar underlying layer 41 Magnetic particles of magnetic layer

Claims (4)

【特許請求の範囲】[Claims] 【請求項1】 基体上に下地層及び磁性層を積層した磁
気記録媒体において、 上記下地層を構成する粒子の平均粒径Xに対する上記磁
性層を構成する磁性粒子の平均粒径Yの比Y/Xが、
0.4≦Y/X≦0.9であることを特徴とする上記磁
気記録媒体。
1. A magnetic recording medium in which an underlayer and a magnetic layer are laminated on a substrate, and a ratio Y of an average particle size Y of magnetic particles forming the magnetic layer to an average particle size X of particles forming the underlayer. / X is
The magnetic recording medium described above, wherein 0.4 ≦ Y / X ≦ 0.9.
【請求項2】 X≧15nmであることを特徴とする請
求項1の磁気記録媒体。
2. The magnetic recording medium according to claim 1, wherein X ≧ 15 nm.
【請求項3】 下地層がCr,CrTi,CrW,Cr
Ta、Ti,Ti−Taからなる群から選ばれる一種か
ら構成され且つ磁性層がCoCr,CoCrTa,Co
CrPt,CoCrPtTa,CoPt,CoPd,C
oCrPtSi,CoCrPtB,Co粒分散複合材料
及びFi粒分散複合材料からなる群から選ばれる一種か
ら構成されている請求項1または2の磁気記録媒体。
3. The underlayer is Cr, CrTi, CrW, Cr
The magnetic layer is composed of one kind selected from the group consisting of Ta, Ti, and Ti-Ta, and the magnetic layer is CoCr, CoCrTa, Co.
CrPt, CoCrPtTa, CoPt, CoPd, C
3. The magnetic recording medium according to claim 1, which is composed of one kind selected from the group consisting of oCrPtSi, CoCrPtB, Co grain dispersion composite material, and Fi grain dispersion composite material.
【請求項4】 磁性層がCoNi系合金を除く材料から
構成されている請求項1から3のいずれか一項の磁気記
録媒体。
4. The magnetic recording medium according to claim 1, wherein the magnetic layer is made of a material excluding a CoNi-based alloy.
JP12944395A 1995-04-28 1995-04-28 Magnetic recording media Withdrawn JPH08306029A (en)

Priority Applications (1)

Application Number Priority Date Filing Date Title
JP12944395A JPH08306029A (en) 1995-04-28 1995-04-28 Magnetic recording media

Applications Claiming Priority (1)

Application Number Priority Date Filing Date Title
JP12944395A JPH08306029A (en) 1995-04-28 1995-04-28 Magnetic recording media

Publications (1)

Publication Number Publication Date
JPH08306029A true JPH08306029A (en) 1996-11-22

Family

ID=15009603

Family Applications (1)

Application Number Title Priority Date Filing Date
JP12944395A Withdrawn JPH08306029A (en) 1995-04-28 1995-04-28 Magnetic recording media

Country Status (1)

Country Link
JP (1) JPH08306029A (en)

Cited By (1)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US6682833B1 (en) * 1999-03-19 2004-01-27 Fujitsu Limited Magnetic recording medium and production process thereof

Cited By (1)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US6682833B1 (en) * 1999-03-19 2004-01-27 Fujitsu Limited Magnetic recording medium and production process thereof

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