PERPENDICULAR MAGNETIC RECORDING MEDIUM AND METHOD OF PRODUCING SAME

Abstract: A perpendicular magnetic recordng medium is fabri­ cated based on R₂₁₋₆₀(Fe 1-y Co y ) z M₀₋₁₀ wherein z is balance and at least 70 at % of R is Nd and/or Pr, the balance of R being one or more of other rare earth elements, and wherein y is less than 0.5 by atomic ratio. M is at least one of various additional metal elements. The Curie temperature Tc is between 70 to 250°C; the saturation magnetization Ms is about 450 emu/cc or more; the uniaxial perpendicular magnetic anisotropy constant Ku of 2.5 x 10⁶ erg/cc or more is attained. Kerr rotation angle is 0.3 degree or more, which provides a magneto-optic recording medium. Since light rare earth elements having the collinear alignment of magnetic moment with Fe are used as a key element, it is possible to fabricate uniform perpendicular magnetic anisotropy thin films in a mass production scale at a low cost.

Description: PERPENDICULAR MAGNETIC RECORDING MEDIUM AND METHOD OF PRODUCING SAME The present invention relates generally to a perpendicular magnetic recording medium and, particularly, a magneto-optic recording medium, and a method of producing the same. In the following, the term "rare earth" denotes "rare earth element", and the term "recording medium" herein is used in a broadest sense. There exists a strong demand for higher-speed and higher-density non-volatile recording media, as compared with the conventional memory devices such as ferrite cores, magnetic tapes or discs, etc., with increasing scale and decreasing size in computer systems. To satisfy the above-mentioned demand, magneto-optical thin film recording media have recently been highlighted owing to the availability for storage devices of great capacity and high density. In usual, a laser beam is used as the light source, being allowed to be incident upon the thin film surface in the direction perpendicular thereto. A great number of microscopic magnetic domains are magnetized minutely and separately below the Curie temperature when no laser beam is incident thereupon, but demagnetized above the Curie temperature when the laser beam is incident thereupon, because of a rise in temperature on the thin film. As ferromagnetic thin films provided with an easy axis for magnetization in the direction perpendicular to the thin film plane, conventionally, there have been known polycrystalline metal thin films such as MnBi, M.nCuBi, CoCr, etc., monocrystalline compound thin films represented by GIG (Ga-Fe garnet) and rare earth - transition metal amorphous thin films such as Gd-Co, Gd-Fe, Tb-Fe, Dy-Fe, etc. The present invention relates, in particular, to rare earth - transition metal amorphous metal ,thin films. The amorphous metal thin films are suitable for a magneto-optic recording material, because in contrast to pollycrystalline thin films there exist no crystal grain boundaries which will cause noise, and additionally there exists an advantage such that a wide thin film can readily be produced. In order to use the rare earth - transition metal amorphous metal alloy film as a magneto-optic recording medium of a high memory density, it is required that the easy axis for magnetization thereof is perpendicular to the film plane. This necessary condition, the perpendicular magnetic anisotropy is not always induced at any cases in the above amorphous metal alloys, but the easy axis for magnetization shows rather a tendency to be arranged in the direction parallel to the film plane depending upon an effect produced by an occurrence of a demagnetizing field. Therefore, in order to obtain a perpendicular magnetic film, it is necessary to provide a uniaxial anisotropic magnetic energy enough to overcome the above demagnetizing field. The magnitude of perpendicular magnetic anisotropy in a thin film can be represented on the basis of a value of uniaxial magnetic anisotropy constant Ku. It has been generally considered that, in order to realize a perpendicular magnetic anisotropic film, the relationship of Ku > 2to52 should be satisfied, where Ms denotes the saturation magnetization, and Tcu is definea as Ku = K1 +21CMs2. In this specification, the term "perpennicular magnetic aflisotropy" embraces at least ones that satisfy above conditions. In the perpendicular magnetic recorcing medium, since a high recording density is generally reguired, it is very important that tte saturation magnetization Ms is great enough to stably maintain microscopic magnetic domains and additionally that the uniaxial magnetic anisotropy constant Ku is sufficiently large. Further, since a laser beam is usually used as the writing power source, it is required that the Curie temperature Tc is sufficiently low, e.g., approximately ranging from 100 to 2000C; the crystallization temperature Tcry is sufficiently higher than the Curie temperature Tc; and the difference in temperature between both is at least about 50 C, and preferably, about 100"C or more. By the way, the most well-known combination of rare earth elements and transition metals as the perpendicular magnetic anisotropic metal alloy thin film is that of heavy rare earth elements and iron. The typical examples are Tb-Fe, Gd-Fe, Dy-Fe, Gu-Tb-Fe, Tb-Dy-Fe, etc. In the case of Tb-Fe, for instance, the magnetic characteristics are such that the Curie temperature Tc is 140 to 250"C; the Kerr rotation angle ik is approximately 0.3 degrees; the saturation magnetization Ms is 50 to 100 emu/cc, and the uniaxial perpendicular magnetic anisotropy constant Ku is 0.1 to 1 x 106 erg/cc. In the above metal alloy thin film, however, since the heavy rare earth elements such as Tb, Dy, Gd, etc. to be included therein are scarce in the resources and exist a little in the crust of the earth, and very complicated element separating processes are reguired, thus the material cost is very high. Additionally, it is difficult to fabricate a great amount of uniform products on a large nass production scale, because the atomic magnetic moments of heavy rare earth elements and iron are to be combined with each other in an antiparallel fashion, and therefore the saturation magnetization Ms and the Curie temperature Tc depend greatly upon the compositional proportion of the elements. In contrast thereto, light rare earth elements such as Nd, Pr, etc. more abundantly exist in the crust of the earth as compared with the heavy rare earth elements. Therefore, if the rare earth - iron alloy thin film of the perpendicular magnetic anisotropy can be fabricated by employing light rare earth elements, it is possible to completely overcome the above serious problems with respect to the resources. So far, light rare earth - iron amorphous metal alloy have been studied as follows: J.J. Croat has reported ribbon alloys composed of around PeO 60Ndo 40 or Fe0.60Pr0,40 formed by melt-quenching and has discussed a possibility for permanent magnets, because a high coercive force had been obtained, Appl. Phys. Lett. 39 (4) , 15th August, 1981. These ribbon alloys formed by the melt-quenching technique, however, are not uniform throughout the alloy and, stillmore, not anisotropic but rather essentially isotropic. Furthermore, the thickness of the ribbon was 33 to 208 Fm, which was far less from that required for a recording medium. Recently, K. Tsutumi et al have reported that a thin film composed of Fe61 5Nò34Ti4 5 and formed Cy sputtering has perpendicular magnetic anisotropy, Japan J. Appl. Phys. 23 (1984) , Page L 169 to L 171. However, the characteristics are such that: Ms is 430 emu/cc and Ku is 2 x 106 erg/cc. Further, with respect to Fe-Nd sputtered thin films in cluding no Ti, only thin films of in-plane anisotropy have been reported although the forming conditions are not clear. In summary, in the case of amorphous anisotro pic thin films composed of light rare earth elements and iron, so far it has been considered that it is impossible to provide perpendicular magnetic anisotropy energy strong enough to overcome the effect by the demagnetitzing field thereof because of its high saturation magnetization. With these problems in mind, therefore, it is a primary object of the present invention to provide a per pendicular magnetic recording medium (particularly a magneto optic recording medium)based on light rare earth elements and iron This object is solved by the perpendicular magne tic recording media according to claims 1 to 5. A further object is to provide methods for pro ducing such a perpendicular magnetic recording medium. This object is solved by the processes according to claims 28 and 31. Further advantageous features are evident from the subclaims. The invention provides rare earth - transition metal amorphous alloy thin films provided with perpendi cular magnetic anisotropy, which are useful in magnetically (or further megneto-optically) recording data in a high memory density. The invention also provides a perpendicular magnetic recording medium (and, particularly, magneto-optic recording medium) having excellent stable perpendicular magnetic recording properties, preferably while reducing the material cost and eliminating complicated fabricating processes so as to well be applicable to a large scale mass production process. Other objects and advantages will become apparent in the entire disclosure. The present invention provides a perpendicular magnetic recording medium(and particularly, magneto-optic recording medium) having a composition with the key elements of iron and rare earth element(s), or additionally Co thereto, the rare earth element(s) being mainly of neodymium Nd and/or praseodymium Pr. In a first aspect of the present invention, the perpendicular magnetic recording medium consists essentially of 21 to 60 (preferably 31 to 60) atomic percent rare earth elements R and the balance of iron Fe wherein 70-100 atomic percent of the R being neodymium Nd and/or praseodymium Pr the balance of the R being one or more selected from the group consisting of yttrium Y, lanthanum La, cerium Ce, samarium Sm, gadolinium Gd, terbium Tb, dysprosium Dy, holmium Ho, erbium Er and ytterbium Yb. In the following, the symbol "R" refers to the rare earth elements hereinabove specified, however, the rare earth elements R may not be pure elements and may contain other rare earth elements other than those specified above in small amounts. In a second aspect of the present invention, the perpendicular magnetic recording medium having the composition of the first aspect wherein cobalt Co of less than 50 (preferably less than 30) atomic percent of the entire Fe is substituted for Fe. In a third aspect of the present invention, the perpendicular magnetic recording medium additionally comprises not exceeding 10 atomic percent of at least one additional element M selected from the group consisting of nickel Ni, zirconium Zr, niobium Nb, vanadium V, tantalum Ta, chromium Cr, molybdenum Mo, tungsten W, manganese Mn, bismuth Bi, aluminium Al, solicon Si, lead Pb, germanium Ge, tin Sn, antimony Sb and hafnium Hf. In a fourth aspect of the preset invention,the composition can be expressed by a formula: R(Fe,Co)M, which includes 21 to 60 atomic percent rare earth elements R,0 to 10 atomic percent additional element(s) M and the balance of Fe and Co, wherein Co amounts to less than 50 atomic percent of the sum of Fe and Co to be counted as the balance and wherein 70-100 atomic percent of the entire R consists of Nd and/or Pr(Nd, Pr), the balance of R being one or more of Y, La, Ce, Sm, Gd, Tb, Dyr Ho, Er and Yb; and wherein, here, Ti is counted as M in the case where Co is present. In the following, "t" or "at %" denotes atomic percent, if not otherwise specified. Furthermore, the method of fabricating the perpendicular magnetic recording medium according to the present invention comprises, in a process for producing a thin film on a substrate by a metal gas deposition technique, the steps of: maintaining a substrate at a temperature between 1800C and a temperature lower than the crystallization temperatures Tcry of said compositions, and forming a perpendicular magnetic anisotropic thin film of a defined composition on the substrate by the metal gas deposition technique; preferably up to a film thickness from about 0.3 to about 3 ,pom. Here, the composition includes those mentioned in the preceding aspects. In a still further aspect of the present invention, the Kerr rotation angle ek is significantly increased by oxidization in the film surface or by SiO coating on the film surface, while a combination thereof is useful, too. In the perpendicular magnetic or magneto-optic recording medium according to the present invention, it is possible to obtain an amorphous metal alloy thin film of perpendicular magnetic anisotropy provided with characteristics such that the Curie temperature Tc is from 70 to 250"C; the saturation magnetization Ms is about 450 emu/cc or more; the uniaxial perpendicular magnetic anisotropy constant Ku is at least 1 x 106 erg/cc and up to 2.5 to 7 x 106 erg/cc or more, the Kerr rotation angle ek is about 0.3 - 0.55 degree or more; that is, which are each equivalent or superior to those of heavy rare earth - iron amorphous thin films, in spite of the fact that iron and light rare earth elements such as Nd and/or Pr are used which are relatively abundant in resources and less expensive The perpendicular magnetic anisotropy constant Ku of at least 1 x 106 ers/cc provides a perpendicular magnetic recording medium which can be written or read at least through a magnetic head. With the high Kerr rotation angle the perpendicular magnetic thin film can be written or read mgneto-optically. As is discussed previously, it fias been generally consicered that the condition Ku > 2tolls2 should be satisfied for the perpendicular magnetic film. In the present invention, however, the magnetic domain is very finely divided, wherein the demagnetizing field is less than the apparent demagnetizing field resulting in a perpendicular magnetic film even without satisfying said condition. It appears that Ku > 0.6 x 2gums2 is roughly sufficient. As to whether or not a perpendicular magnetic film occurs, we can know by measuring the magnetization curves in both directions perpendicular (1) and parallel (//) to the film plane as shown in Fig. 3. Further, the Curie temperature Tc and the Kerr rotation angle ek can be increased up to 0.5 degree or more by substituting Co for a part of Fe. Stillmore, in the present invention, wherein the magnetic moments of each atom are combined in collinearly parallel to each other on the basis of combination of Nd, Pr and iron, it is possible to obtain a saturation magnetization Ms higher than that in heavy rare earth - iron films, so that the- precision of recording/reading data can be further improved. By the same token, as shown in Fig. 2, the saturation magnetization Ms or Curie temperature Tc are less dependent upon the compositional proportion so that a more uniform thin film can be easily obtained. Purthermore, in the magnetic or thermomagnetic writing, it is possible to reduce the magnitude of magnetic field to be applied to the film from the outside, because the leak magnetic flux car; be utilizes due to the higher saturation magnetization. stillmore significant improvement in the increase in the Kerr rotation angle ek can be obtained by oxidizing the film surface or coating by Sic, or a combination thereof based on tile thin film hereinabove mentioned. The large Kerr rotation angle provides a higher S/N ratio. The features and advantages of the perpendicularly magnetizable recording medium and the method of fabricating the same according to the present invention will be more clearly appreciated from the following description taken in conjunction with the accompanying drawings in which: Fig. 1 is a graph showing the relationship between temperature T and magnetization M in an embodiment of Fe100-xNdx by applying a magnetic field of 10 kOe (0.8 x 106 A/m) as a function of Nd content x; Fig. 2 is graphs showing the relationship between Nd content x and Curie temperature Tc, crystallization temperature Tcry and the relationship between Nd content x and saturation magnetization Ms at 77K (-196 C) and 300K (27 C) in Fe100 xNdx; ; Figs. 3 (a) and (b) are graphs showing various magnetization curves in Fe 100xNdy at 77K (-196 C) and 300K (27 C) tor- each Nd content x of 35 and 40; Fig. 4 is graph showing the relationship between substrate temperature Ts and perpendicular magnetic anisotropy constant Ku in z Fes5Nd35 system; C. Fig. 5 is X-rcy difi-raction patterns in Fes5Nd35 at different substrate temperatures Ts of 212 C, 287 C and 335 C; Fig. 6 is a graph showing the relationship between film thickness D and perpendicular magnetic anisotropy constant Ku in Fe65Nd35; Fig. 7 is a graph showing the relationship between argon pressure P within the vessel and perpendicular magnetic anisotropy constant Ku in Fe65Nd35; ; Fig. 8 is a graph showing the relationship between Nd content x and perpendicular magnetic anisotropy constant Ku in Fe 100-x Nd Fig. 9 (1) is a graph showing the relationship between magnetization torque L and angle Q at torque measurement under magnetic field of l5kOe (1.2 x 106 A/m) at various temperatures from 4.2 to 300K (-269 to 27 C) in Fe60Nd40; Fig. 9 (2) is a graph showing the relationship between magnetization torque L and the angle e under various magnetic fields from 3 to 20kOe (0.24 to 1.6 x 106 A/rn) at three different temperatures of 4.2K (-269 C), 77R (-196"C) and 300K (27 C) in Fes0Nd40; ; Fig. 10 is a graph showing the relationship between temperature T an hysteresis loss W within a magnetic field of 15 kOe in Fe65Nd35 and Fe60I40; Fig. 11 is a graph showing the Curie temperature Tc, crystallization temperature Tcry, magnetic anisotropy transition tmperature T1, and coercivity Hc, as a function of the relative Co concentration y (versus Fe in (Fe yCOy)60ND40 Fig. 12 is a graph showing the deventience of Kerr rotation angle ek (uegree) upon wavelength of light (nm) of Nd35Fe65 and (Fel-y Coy)60Nd40; ; Fig. 13 is a graph showing Kerr rotation angle leki of a sputtered thin film of (Fe1yCoy)60Nd40 as a function of a relative Co concentration y; Fig. 14 is a graph showing saturation magnetization Ms and perpendicular magnetic anisotropy constant Ru of (Fe1yCoy)60Nd40 as a function of the relative Co concentration; Fig. 15 is a graph showing Kerr rotation angle leki (degree) and coercivity Hc, and increase thereof due to oxidization in the film surface of Fel00 xNdx; ; Fig. 16 is a graph showing temperature - depending change in the perpendicular magnetic anisotropy constant Ku (107 erg/cc) of Fe100xNdx ( = 30, 35, 38i 40, 50); Fig. 17 is a high resolution electron micrograph of a 15 nm thick Fe60Nd40 film deposited on a substrate at 220 C; Fig. 18 is a graph showing Kerr rotation angle ek vs wavelength A for Fe XPrx (x=20-50) films and Fig. 19 is a graph showing Kerr rotation angle ek (degree) of Fel00-xPrx films as a function of Pr concentration x (at %) at different wavelength #=633 and 500nm. The perpendicular magnetic, particularly, magneto-optic recording medium and the method of producing the same will be described in further detail with reference to the attached drawings. As already described hereinabove, the composition of the medium of the present invention can be generally expresses by a formula R21-60(Fel-yCoy)balM0-10, wherein y is less than 0.5 by atomic ratio anci 70-100 at % of R consists of Nd and/or Pr. That is to say, 21 to 60 atomic percent rare earth elements R are included in the whole composition; however, 70 atomic percent or more of the entire R is Nd and/or Pr. It is particularly preferred to use Nd. Further, it is also possible to use one or more of other rare earth elements such as Ce, Y, Sm, Dy, Tbv Ho, Gd, La, Er and Yb as the balance of R from the standpoint of easiness in procurement. It is preferred that the balance (Fel yCOy) is at least 40 atomic percent. In the case where at least 21 et % R is contained, the temperature difference of more than 500C between Tcry and Tc and a Ku of at least 1 x 106 erg/cc are obtained, which is gene rally useful as a perpendicular magnetic recording medium which can be recorded through a magnetic head. In the case where 31 atomic percent or more of the rare earth element R is included, it is possible to obtain a stable uniaxial (i.e., perpendicular) magnetic anisotropy constant Su of at least 2.5 x 106 erg/cc in the direction perpendicular to the thin film plane, thus this range is preferred. Where the R content of the composition exceeds 60 atomic percent, the formed thin film is not stable in the anisotropy constant, because active rare earth elements are included excessively. Therefore, the content of R should be between 21 and 60 atomic percent (preferably 31 t or more). More preferred is an R range from 33 to 50 % providing Ku of 3 x 106 erg/cc or more with a desired stability of film, and most preferred is an R range from 35 to 45 t in view of Ku. The dependence of the perpendicular magnetic anisotropy constant Ku upon the content x of rare earth element R is clearly shown in Fig. 8. The balance of the R consists primarily of Fe. However, it is also possible that Co is substituted for less than 50 (preferably less than 30) atomic percent of the entire Fe to be counted as the balance where Co is not contained in order to increase the saturation magnetization Ms, the Curie temperature Tc and the Kerr rotation angle, and further to improve the corrosion resistance of the thin film, without deteriorating the characteristics required for generally perpendicular magnetic or particularly magneto-optic thin films. If Co is substituted for Fe in an amount less than 50 % of Fe, the temperature difference between the crystallization temperature Tcry and the Curie temperature Tc becomes small and Kerr rotation angle ek becomes small, too. Besides, if so, targets for sputtering become brittle resulting in difficulty in production thereof. Thus Co substitution should be less than 50 at % of the entire Fe. So long as the Kerr rotation angle is concerned, a Co substitution amount for Fe from about 8 at % to less than 30 at % is preferred (ek of 0.450 or more ), and a Co substitution amount of about 12 to about 27 at % is most preferred (8k of 0,5" or more). Further, it is also possible to add not exceeding 10 atomic percent of at least one of additional metal elements such as Ni, Zr, Eb, V, Ta, Cr, Mo, W, Mn, Bi, P1, Pb, Sb, Ge, Sn and ef (ref erred to as "addi tional elements M" which further embraces Si) also without deteriorating the magnetic characteristics required for magneto-optic or particularly perpendicular magnetic thin films. It is preferred that the sum of M does not exceed 10 at %. It is also possible to add 10 atomic percent or less of titanium Ti to above compositions. In this case, the Ku can be as high as 3 x 106 ery/cc, provided that the specific process of the present invention is applied. Generally, a protective layer of SiO2 or A1N is provided to improve the corrosion resistance of the thin film. In the present invention, the incorporation of Co and/or some of the additional elements M in the Fe(Nd, Pr) alloy system improves the corrosion resistance of the thin film per se, such M being one or more of Ni, Zr, Nb, V, Ta, Cr, Mo, W, A1, Hf, Ti, Ni and Si. As already explained hereinabove, since a laser beam is used as the writing power source in magneto-optically writing data onto the thin film, the Curie temperature Tc should be low and the crystallization temperature Tcry should be high, and the difference between the two should be great. Fig. 1 shows these temperature characteristics in Fe100Nd (x= 18,30,35,38 and 40). Fig. 1 indicates that the Curie temperature Tc is from 350 to 400K (77 to 127 C), which is roughly equivalent to that (about 70"C) of Dy-Fe or that (about 140"C) of Tb-Fe. Further, the difference in temperature between Tc and Tcry is about 200 C or more except the case of t3d content x=l8, o that it is well understood that magneto-optic writing of data onto the thin film is well possible by applying heat (, e.g. , by a laser beam). The temperature difference of 200 C or more provides a sufficient stability to the alloy state which is kept substantially in the amorphous state even when heating is repeated. Fig. 2 shows the dependence of the Curie temperature Tc, the crystallization temperature Tcry and the saturation magnetization Ms in Fe100-xNdx upon the R(Nd) content x. Fig. 2 indicates that the change rate in both Tc or Ms is small over a wide range and therefore it is possible to fabricate very stable proaucts in quality with more easiness as compared with heavy rare earth - iron perpendicular magnetic anisotropy thin films. At a Nd content of 21 at % or more, the temperature difference (Tcry-Tc) is at least 50 C. Fig. 3 shows magnetization curves at 77K (-196oC) and 300K (27 C) in about 0.8 to 1.0 m thick Fel00 xNdx (X = 35, 40) films. The solid and broken lines correspond to curves obtained at a perpendicular direction (1 ) and parallel direction (//) of the film plane by applying an external magnetic field perpendicularperpendicular and parallel to the film plane, respectively. These curves indicate that the samples are perpendicularly magnetizable at both the temperatures but the residual magnetism is very small at 27 C but increases at a lower temperature -196 C. Further, the Kerr rotation angle Ok of these films are 0.3 degree, which is roughly equal to or more than that of the heavy rare earth - iron amorphous perpendicular magnetic film. In the than film accorciing to the present invention, since the saturation magnetization Ms is fairly high, it is necessary for the perpendicular magnetic recording medium that the perpendicular magnetic anisotropy constant Ku is greater than 1 x 106 erg/cc, and Ku of at least 2.5 x 106 erg/cc is preferred. As substrate materials for the amorphous thin film, glass, A1, r polyimido resin, polyester resin, etc. are generally usable. However, in the embodiment according to the present invention, since the substrate should be maintained at a temperature between 180"C and a temperature lower than the crystallization temperature in order to obtain a perpendicular magnetic anisotropy film, it is necessary to use a substrate material which can withstand the above temperature. The substrate temperature from 200 to 300"C is a preferable range in which Ku= 3 x 106 erg/cc or more can be obtained. Fig 4 4 shows the dependence of the perpendicular magnetic anisotropy constant Ku upon the substrate temperature in Fe65Nd35. This curve clearly indicates that the anisotropy constant Ku is near its maximum between 260 and 290"C. Further, the black circles represent that the samples are perpendicularly anisotropic, and the white circles represent that the samples are not perpendicularly anisotropic (but in-plane anisotropic), the numerals near the circles designate the thickness (A) of the sample films. Furthermore, this curve indicates that if the substrate temperature Ts exceeds the crystallization temperature Tcry (about 320 C) the perpendicular magnetic anisotropic characteristics are not present (Ku is almost zero). In the thin film according to the present invention, amorphous phase or microfine-crystalline phase of about a few tenthsof a nm to about 10 nm in the average is desirable; that is, it is desirable that there exist no crystal grain boundaries which will cause noise as already explained. Fig. 5 shows the intensity of X-ray diffraction patterns at different temperatures as a function of an angle 2e. These patterns indicate that the intensity curves have some sharp peaks at Ts=335 C but almost no sharp peaks at Ts= 212 C, which represents that the film is fairly amorphous. Additionally. a high resolution electron microscopic observation confirms that there exist microfine - crystalline grains when the substrate temperature Ts is at 212"C or 287 C, but to some extent grown crystalline grains when at 335 C. which demonstrates the crystal grain size hereinabove mentioned is desired. The perpendicular magnetic anisotropy constant Ku increases with increasing thickness of the film. However, if the thickness D exceeds 3pmt it is not preferable from the standpoint of productivity, because it becomes difficult to form a uniform film. Fig. 6 shows the dependence of the anisotropy constant Ku upon film thickness D, which indicates that the perpendicular magnetic anisotropy constant Ku larger than 2 Ms2 can be obtained at a thickness D of 0.3 pm or more, and Ku > 2.5 x 106 erg/cc can be obtained when the thickness D exceeds about 0.7 ym. In Fig. 6, the black circles represent that the film is of perpendicular anisotropy while the white circles represent that the film is not of perpendicular anisotropy. Further, the numerals near circles designate substrate temperature Ts( C). The thin film according to the present invention can be formed in accordance with a metal gas deposition (or. so-called vapor deposition) technique; that is, by any of vacuum deposition method, PVD such as sputtering, ion plating, etc., CVD or the like. In the case of the sputtering method, preferably, the samples are fabricated within an argon Ar atmosphere under pressure of about 2.67.l0l mbar (26.7Pa) (2 x 10 Torr) . Fig. 7 shows the dependence of the anisotropy constant Ku upon Ar pressure. Similarly, the black circles represent that the samples are perpendicular anisotropy while the white circles represent that the samples are not perpendicular anisotropy; the numerals near the circles represent film thickness (A). Fig. 7 indicates that the change in Ar pressure P has a relatively less influence upon the Ku than other factors such as the substrate temperature or the film thickness D. In sputter-depositing the material onto the substrate, it is preferred to apply a magnetic field of a few to several tens Oe to the substrate in the direction perpendicular thereto. This magnetic field can readily be obtained by passing a direct current to a solenoid of a sheath wire for heating wound in a coil and disposed under the film substrate. In order to understand the origin of the perpendicular magnetic anisotropy, the temperature dependence of Ku was examined on Fe60NdA0 and Fe65Nd35. Fig. 9 (2) is an example of the torque curves measured in various fields at 4r 2 77 and 300K. There, e is the angle between the field direction and a direction in the film plane, (Thus e = 0 is the direction in the film plane.) The torque curves at 300K indicate that the easy axis for magnetization is along the direction normal to the film plane (e = 90 ). Also, very little rotational hysteresis loss is found at 20kOe at 300K. Fig. 9 (1) shows a sequence of torque curves obtained at more various temperatures in H = 15kOe(4.78 x 106 Aim) to show in more detail the change in torque curves with temperature. It is seen that both the torque amplitude and the rotational hysteresis loss W increase with decreasing temperature down to about 84K, and then decrease. It should also be noted here that the slope at e = 0 changes its sign from positive to negative with decreasing temperature from about 80 to 4.2k. However, since the thin film according to the present invention is provided with relatively large saturation magnetization Ms, when used as a magneto-optic disk for thermo-magnetic writing of data, it is possible to reduce the magnitude of magnetic field to be applied from the outside, because the leak magnetic flux coming from the surroundings can effectively be utilized. Flg. 10 shows the perpendicular magnetic anisotropy constant ru and the hysteresis loss W at low temperatures. The Ku increases with decreasing temperature and reaches its maximum 3 x 107 ers/cc near liquid nitrogen temperature of 80guv (-1930C) . Also, the hysteresis loss W reaches its maximum at 100K (-173"C) or less. Fig. 11 51ws temperature characteristics of the thin film including Co, in particular. This graphical representation indicates that the addition of Co increases the Curie temperature Tc and the temperature T1 at which the perpendicular magnetic anisotropy constant Ku attains a maximum value (i.e., it is believed to be a transition temperature at which the magnetic anisotropy transforms from unidirectional characteristic perpendicular to film plane to cone characteristic), without increasing the crystallization temperature Tcry. EYMPL ES The various characteristics of various embodiments of the perpendicular magnetic or magneto-optic recording medium according to the present invention will be described hereinbelow with reference to the drawings again. The test samples were all fabricated on glass substrates within an Ar atmosphere in accordance with a rf sputtering method. Before introducing the Ar gas, the pressure within the sputter vessel is evacuated down to 5 x 10'-7 Torr (3.7 x 10 9 Pa) or less. The sputtering speed was approzimatcly 2pmXh. No bias voltage was applied to the sample substrate during the sputtering process. The substrates were heated by adjusting the magnitude of current passed through a heater coil disposed under the substrate. The heater coil comprised cylindrical copper bobbin the outer circumference of which was wound by a sheath wire. Since a direct current was applied through the heater coil, a magnetic field of a few to several tens Oe was applied to the substrate. The magnetic anisotropy of the test samples was measured by a high sensitivity type torque magnetometer having in fields of 20 kOe (1.6 x 106 A/m), and the saturation magnetization by a vibrating sample magnetometer (VSM). The microstructure of the thin film was analyzed by X-ray diffractomentry on the basis of Cu-Ki radiation and high resolution transmission electron microscopy. The intrinsic perpendicular magnetic anisotropy constant Ku was derived from the relation between (fl/H)2 vs L, where L is the torque amplitude obtained at the external field H applied at 450 with respect to the film plane. (Here, Ku is defined as Su=Kl +271Ms2, where K is the observed anisotropy from the torque, and Ms is the saturation magnetization) Example 1 Five Fe100-xNdx thin films (where x= 18, 30. 35, 38 and 40) were formed on glass substrates under the following conditions: the Ar pressure was 1 to 2 x 10-1 Torr (13.3 to 26.6 Pa); the substrate temperature Ts was 220 to 290 C; and the film thickness D was 0.5 to 1.2 urn. The dependence of the magnetization M is upon temperature T s1in in Fig. 1 with different values of Nd content x. The dependence of the Curie temperature Tc, the crystallization temperature Tcry and the saturation magnetization MS upon the Nd content x is shown in Fig. 2, respectively. The detailed discussion of these figures have already been made hereinabove, therefore being omitted here. Fig. 2 is based on Example 1, as discussed previously. Fig. 2 also shows that Ms at 77K and 30CK depends upon the composition Fe-Id. nt a Nd content of 21 at % or more the temperature difference (Tcry-Tc) amounts to at least about 50 C, while at 30 at t or more the difference amounts to 200"C or more. The magnetization M was measured within a magnetic field of 10 kOe (8 x 105 A/m) after the samples have been magnetized to the saturation point in the direction of easy axis of magnetization. To measure the magnetization M, a vibrating sample type magnetometer was used. The Curie temperatures Tc were obtained from points of intersection between the extrapolation curve M2/T (where M is the magnetization and T is the temperature) and the horizontal temperature axis. To obtain the magnetization curve, the temperature was increased gradually as shown by the solid lines in Fig. 1. The dashed lines show the magnetization curves obtained when the temperature was lowered from a high temperature more than 1000K (727"C). Example 2 Three Fe100-xNdx thin films (where x = 30, 35 and 40) were formed by sputtering under the following conditions: Ar pressure was 1 to 2 x 10 1 Torr (13.3 to 26.6 Pa); and Ts was 240 to 2 G C. The magnetic characteristics of the sputtered film were measured at 77K (-196eC) and 300K (27 C) in a directions perpendicular (1) and parallel (//) to the film plane, and are shown in Fig. 3, which shows parpendicular anisotropy as discussed previously. Tile Kerr rotation angle ek was measured on this film to be 0.3 degree which is substantially equivalent to that of the heavy rare earth - iron perpendicular magnetic film. Example 3 Various Fe60Na35 thin films were forme unuer the following conditions: Ar pressure was 1 to 2 x 10-1 Torr (13.3 to 26.6 Pa);thickness D was 6000 to 12650 (0.6 to 1.26 and Ts was 70 to 330'C. Ku was measured by a torquf meter. The dependence of the uniaxial perpendicular magnetic anisotropy constant Ku upon the substrate temperature Ts is shown in Fig. 4. This figure indicates that the black circles indicative of perpendicular anisotropy lie above Ku = 1.5 x 106 erg/cc and between Ts = 200 and 3000C and that the maximum Ku lies between Ts = 260 and 290-C. The white circles indicate that it is not of perpendicular anisotropy. If the substrate temperature Ts is above the crystallization temperature Tcry (= about 320C) , it provides no perpencicular magnetic film. Further, the Y.-ray diffraction patterns at Ts = 212, 287 and 335 C are srown in Fig. 5. At Ts of 335 C and 2870C, sharp peaks appear which are believed to correspond those of Hd2Fe27 or As discussed previously, the electron microcopy revealed that the presence of an amorphous matrix and the average grain size of microfine-crystallite ranging from about ç few h to about 100 (2 few tenths of a nrn to about 10 nm) is sui Example 4 Various Fe65Nd35 thin films were formed under the following conditions: Ar pressure was 1 to 2 x 10-1 Torr (13.3 to 26.6 Pa); Ts was 210 to 290 C; and D was v2ri ec:. Ku waE measured by the torque meter. The dependence of the anisotropy constant Ku upon film thickness D is shown in Fig. 6, wherein black circles represent perpendicular anisotropy and white circles represent in-plane anisotropy. This figure indicates that a thickness D of 0.3m or more is necessary to obtain Ku larger than 2Ms2, and D of 0.7 m or more is necessary for Ku of at least 2.5 x 106 erg/cc. Example S Various Fe65Nd35 thin films were formed under the following conditions: Ts was 210 to 290 C; D was 6140 to l2650A (0.6 to 1.2 m), and Ar pressure was varied. The dependence of the anisotropy constant Ku upon Ar pressure is shown in Fig. 7. This figure indicates that the Ar pressure exerts z less influence upon Ku than other factors such as Ts or D. Example 6 Various Fe100xNdx thin films (where x = 18 to 50) were formed under the following conditions: Ar pressure was 1 to 3 x 10-1 Torr (13.3 to 39.9 Pa); TE was 250 to 280 C; and D was 6000 to 13000A (0.6 to i.3pm). The dependence of the anisotropy constant Ku upon Nd content x is shown in Fig. 8. The Ku reaches its maximum value of 1 to 2 x 107 crS/cc near Mdzo. As the Nd amount decreases therefrom, Ku rapidly decreases thus Ku drops down below 2.5 x 1C6 erg/cc at a Nd amount of less than 31 at t. This curve indicates that when the R content lies between 33 and 55 atomic percent, the Ku is within a preferable range of 3 x 106 erg/cc or more. Further, in Fig. 8, each plotted value is an average of several test samples fabricated at different times. At 21 at % Nd, the film shows perpendicular magnetic anisotr opy. Example 7 Various Fe60Nd35M5 thin films (where M is at least one of Ni, Zr, Nb, V, Ta, Cr, Mo, W, Mn, Bi, Al, Si, Pb, Sb, Ge and Sn) are form under the following condition: Ar pressure is 1 to 2 x 10-1 Torr (13.3 x 26.6 Pa); Ts is 220 to 290 C; and D is 6300 to 11000 (0.6 to 1.1 m). It is possible to obtain perpendicular magnetic anisotropy for each test sample. Example 8 An Fe40Co25Nd35 thin film was formed under the following conditions: Ar pressure was 2 x 10-1 Torr (26.6 Pa); Ts was 240 C; and D was 7400 (0.74 m). The anisotropy constant Ku was 2.5 x 106 erg/cc or more. Example 9 An Fe60Nd25Pr15 thin film was formed under the following conditions: An pressure was 1.5 to 2 x 10-1 Torr (19.5 to 26.6 Pa); Ts was 2600C; and D was 7900A (0.79 m). The anisotropy constant Ku was 2.5 x 106 erg/cc or more. Example 10 Three tlln films of Fe60Nd32Dy8, Fe58Nd32Ce10 and Fe57Nd30Co10V3 were formed under the following conoitions: Ar pressure was 1 to 2 x 10-1 l;orr (13.3 to 26.6 Pa); Ts was 240 to 2900C; and D was 7300 to 11000 A (0.73 to 1.1 The The anisotropy constants Ku thereof were each 2.5 x 106 erg/cc or more. Example 11 Two Fe65Nd35 and Fe60Nd40 thin films were formed under the following conditions: Ar pressure was 2 x 10-1 Torr (26.6 Pa); Ts was 2900C and 250 C, respectively; and D was 12650 (1.26pm) and 4860t (0.48 m), respectively. The torque curves in Fe60No40 measured at 4.2 to 300R are shown in Figs. 9 (1) and (2). Further, the hysteresis loss W at low temperatures in both films is shown in Fig. 10. Example 12 Four Fe60yCoyNd40 thin films (where y is 0, 5, 10 and 15) were formed under the following conditions: Ar pressure was 1 to 2 x 10 1 Torr (13.3 to 26.6 Pa); Ts was 220 to 270 C; and D was 5000 to 8200 (0.5 to 0.82 m). The change in the Curie temperature Tc, the crystallization temperature Tcry, the temperature T1 at which the perpendicular anisotropy constant Ku depicts a maximum, and the coercivity Hc is shown in Fig. 11, respectively, as a function of the Co content y. As the Co amount increasesr Tc, He and T1 increase without changing Tcry. Example 13 The Kerr rotation angle ek as a function of the wavelength A was measured on the thin films of Sd35Fes5 (Example 1) and (Fe1-yCoy)60Nd40 (Example 13) by applying a linearly polarized ray (light source of a Hg lamp, wavelength A = 230 to E30 ran, without half-mirror) with an incident light angle of 80 degrees onto the surface of the thin film, wherein the measurement was effected on the surface side of the films by using a "Magneto-Optical Instrument J-250" manufactured by Japan Spectroscopy Co., Ltd. The result is shown in Fig. 12, in which Co 5, Co 10 and Co 15 represent y = 0.083, 0.17 and 0.25 respectively. The Kerr rotation angle ek is positive at a low wavelength below A = 340 nm, approximately zero at 340 nm, and negative at a higher wavelength than 340 nm. The absolute Kerr rotation angle 16l;l rapidly increases above A = 340 nm and reaches a roughly constatn high level at A above 500 nm. The |#k| values show maximum values around A = 400 to 500 nm. Fig. 13 shows the change of the Kerr rotation angle |#k| as G function of the Co concentration y for (Fel¯yCoy)60N oo at A = 500 and 633 nm to illustrate its dependence upon the composition. |#k| increases as the Co concentration y increases, depicting a peak around y = 0.25. At y = 0.25 the Kerr rotation angle is 0.55 degree for N = 500 nm, and 0.45 degree for A, = 633 nm, which are significantly larger than those attained by the GÅa-Fe-Co system. Co is effective at 0.1 %, tco. Example 14 By using tbe same samples employed in Example 13, the saturation magnetization Ms and the perpendicular magnetic anisotropy constant Ku at 300K were measureo and the results are shown in Fig. 14. As the amount of Co substituted for Fe increases, the lilts and Ku decrease. Example 15 Sample thin films of Fe100xNdx prepared under the same conditions as Example 1 were measured for Ok and coercivity 13c (kOe), which are shown in Fig. 15. Additional oxidizing treatment of the thin film surface was carried out on the samples of x=35 and 50 at %, respectively, to oxidize the surface in the depth of about 100 to about 300 (1C-30 nm) just after the thin film had been prepared whereby the Kerr rotation angle significantly increased as shown by arrows in Fig. 15. For instance at a Nd concentration x = 50 at %, #k increased from 0.3 to about 0.6 degrees; i.e., by about twice. It is believed that the surface oxidation serves to increase the effective Kerr rotation angle due to an occurrence of multiple interference through the contribution of the Kerr effect and Faraday effect. The surface oxidization treatment was effected by maintaining the film on the substrate at a temperature of 100-150 C within the sputter vessel for a half to one hour after sputtering. The surface oxidization is more convenient in preparation than the coating treatment such as SiO - coating or the like applied onto (above) the film surface, since in the oxidization treatment the film surface in situ can be subjected to oxidization. The present invention provides a great advantage in this respect over the prior art. Further, such oxiized layer can serve as a protective layer of the base thin film. SiO coating (¯5icmess of 12C02 (120nm)) was also applied on the frestily prepare tr.in film of the same same (x = 35 at %) , and the result is shown in Fig. 15. The SiO coating can increase the Kerr rotation angle, too. This means the conventional or additional treatment or layer provision can further increase the Kerr rotation angle ek, which is also counted as an advantage of the present invention. SiO coating or any other coating may be applied on the oxidized layer hereinabove mentioned too. Example 16 The change of the perpendicular magnetic anisotropy constant Ku as a fanction of temperature was measured on the same samples as Example 16, and the result is shown in Fig. 16. Ku generally increases as the temperature decreases to depict a maximum value at a temperature T1, and decreases thereafter (i.e., the temperature becomes still lower). The peak temperature T1 for Ru shifts as a function of the composition (e.g., Nd concentration x at %), which is also shown in Fig. 16, at the upper right corner. Example 17 writing test by laser beam was carriedout by using a sample film of Nd38Fe62 preparedin the same manner as Example 1, and having a thickness of about 4000 (0.4 pm) under the following conditions. laser: semiconductor laser (power 20 bias magnetic field; about 100 Oe; and writiny: line writing method. The result was observed through polarizing microscopy based on the Kerr effect to show that bits with a width of about 2 to 1C pm have been recorded. It should be noted, however, the width per one bit memory may be further improved based on the thin films of the present invention by applying various improvement in the writing devices and systems, too. Furthermore, it should be understood that any additional measures such as coating or surface treatment other than those disclosed herein may be applied without departing from the gist of the present invention. Example 18 A 150A (15nm) thick Fe60NdO film was made on a cleaved rocksalt substrate at Ts of 220 CC, and a high resolution transmission electron micrograph thereof is shown on Fig. 17. There is clearly observed a lattice image of a 0.2 nm spacing. The average size of such a region (clusters) varies from place to place (2-10nm) , however, on the average of about 3-5 nm. This feature was also found in most of the films examined in the present invention. i1aniely, though the X-ray diffraction patterns show an amorphous state, it is concluded that some sort of a short range atomic ordering is present in the amorphous matrix in the Fe-Nd or (Fe, Co)-Nd alloy systems, which gives rises to a lattice image. Thus the region of the perpendicular magnetic anisotropy is strongly suggested to be associated with an anisotropic arrangement in such structure. Example 19 Thin films of a composition Fe45Co15Nd35M5 wherein M was one of Zr, Ef, V, l1b, Ta, Cr, Mo, S1 and Ti are made to film thickness of 5300 to 12000A (530 to 1200 nm)underthe conditions of Ts=21O-285 C and an Ar pressure of 1-2x10-1 Torr (0.13 - 0.26 mbar) a: magnetic properties are measured. Each sample shows the perpendicular magnetic anisotropy having a Ku value of 2.5x10-6 erg/cc or more, and a Kerr rotation angle #k of 0.4 degree or more. Example 20 (Anticorrosion test) Films obtained in Examples 1, 7, 13 and 19 having the compositions of Fe65Nd35, Fe60Nd35M5 (M=Zr, Hf, V, Nb, Ta, Cr, Mo, Al, Bi, Mn, Sb, Ge, Sn, Pb, Ni and Si), Fe45Co15Nd40 and Fe45Co15Nd35M5 (M= Zr, Hf, V, Nb, Ta, Cr, Mo, Al, Ti, Pb, Ni and Si) are immersed in a one N NaCl aqueous solution for 20 minutes, then subjected to aging for 2 hours at 850C ano 85% RH (relative humidity). The resultant films are observed by an optical microscope with respect to corrosion or pin hole. The FeCoIjdM films shows a most exceilent corrosion resistance against pin hole, wherein a better corrosion resistance is shown with FeCoNd, then FeNdM (M=Zr, Hf, Nb, Ta, Cr, Mo, Al, Ni and Si) in this order, while FeNd an FeNdM (M=Ei, Mn, Sb, Ge and Sn) shows a worst pin hole corrosion. Example 21 Sputtered films having compositions of Fe 100-x pr x (x=20-50) were produced under the conditions of: Ar pressure at 2x10-1 Torr (0.26 nbar),Ts eaheach at 290 C an 270 C, and D each at 8200 (0.82 m) and S4OO (0.94 m). Tiie resultant thin films werc measured tor Kerr rotation angle 6k as a function of tte wavelength t of the incident light in the same manner as Example 13. The result is shown in Fig. 18. A maximum 6k of 0.35 degree is obtained at > ) about 500 nm for Fe70Pr30. Change of the Kerr rotation angle ek (degree) measured at different wavelength X = 633 and 500 nm is shown in Fig. 19 as a function of Pr concentration x(at%).

Claims: CLAIMS 1. A perpendicular magnetic recording medium with perpendicular magnetic anisotropy comprising a thin film, consisting essentially of: a) 21 to 60 atomic percent rare earth elements R wherein 70-100 atomic percent of said R consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce, Sm, Gd, Tb, Dy, Ho, Er and Yb; and b) the balance being Fe. 2. A perpendicular magnetic recording medium with perpendicular magnetic anisotropy comprising a thin film consisting essentially of: a) 21 to 60 atomic percent rare earth elements R wherein 70-100 atomic percent of said R consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce, Sm, Gd, Tbi Dy, Ho, Er and Yb; and b) the balance being Fe and Co wherein Co amounts to less than 50 atomic percent of the sum of Fe and Co counted as the balance. 3. A perpendicular magnetic receding medium with perpendicular magnetic anisotropy comprising a thin film consisting essentially of: a) 21 to 60 atomic percent rare earth elements R wherein 70-100 atomic percent of said R consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce, Sm, Gd, Tb, Dy, Ho, Er and Yb; b) not exceeding 10 atomic percent of one or more of Ni, Zr, Nb, V, Tat Cr, Mo, W, Mn, Bi, Al, Pb, Sb, Ge, Sn, Si and Hf; and c) the balance being Fe. 4. A perpendicular magnetic recording medium with perpendicular magnetic anisotropy comprising a thin film consisting essentially of: a) 21 to 60 atomic percent rare earth elements R wherein 70-100 atomic percent of said R consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce,. Sm, Gd, Tb, Dy, Ho, Er and Yb; b) not exceeding 10 atomic percent of one or more of Ni, Zr, Nb, V, Tat Cr, Mo, W, Mn, Bi, Al, Pb, Sb, Ge, Sn, Si, Ti and Hf; and c) the balance being Fe and Co wherein Co amounts to less than 50 atomic percent of the sum of Fe and Co counted as the balance. 5. A perpendicular magnetic recording medium with perpendicular magnetic anisotropy comprising a thin film expressed essentially by a formula: Rx(Fe1 -yCoy)2Mk wherein, by atomic percentr x is 21-GO %, k is 0-10 %, and z is 30-79 % provided that y is zero to less than 0.5 by atomic ratio; wherein 70-100 atomic percent of the entire R consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce, Sm, Gd, Tb, Dy, Ho, Er and Yb; and wherein said M is at least one selected from the group consisting of Ni, Zr, Nb, V, Ta, Cr, Mo, W, Mn, Bi, Al, Pb, Sb, Ge, Sn, Si, Ti and Hf; said film comprises an oxidized layer in the surface thereof. 6. The recording medium as defined in any one of the preceding claims, wherein R is 31 to 60 atomic percent. 7. The recording medium as defined in any one of the claims 1 to 5, which has a perpendicular magnetic anisotropy constant Ku of at least 1 x 106 erg/cc. 8. The recording medium as defined in claim 6, which has a perpendicular magnetic anisotropy constant Ku of at least 2.5 x 106 erg/cc. 9. The recording medium as defined in any onse of the preceding claims, which has a Kerr rotation angle le of at least 0.3 degree. 10. The recording medium as defined in claim 2 or 4, wherein Co amounts to less than 30 atomic percent of the sum of Fe and Co to be counted as the balance. 11. The recording medium as defined in claim 5, wherein y for Co is less than 0.3 by atomic ratio. 12. The recording medium as defined in any one of claims 1-4, wherein Fe or the sum of Fe and Co to be counted as the balance is at least 40 atomic percent. 13. The recording medium as defined in claim 5, wherein z is at least 40 atomic percent. 14. The recording medium as defined in any one of claims 1 to 5, which has a temperture difference of at least about 500C between the crystallization temperature Tcry and the Curie temperature Tc. 15. The recording medium as defined in claim 14, wherein the temperature difference is at least about 2000C. 16. The recording medium as defined in any one of claims 1-5, wherein R is 33-50 atomic percent. 17. The recording medium as defined in claim 16, wherein R is 35-45 atomic percent. 18. The recording medium as defined in claim 16 or 17, wherein the perpendicular magnetic anisotropy constant Ku is at least 3.0 x 106 erglcc. 19. The recording medium as defined in claim 9, wherein Co amounts to at least about 8 atomic percent of the sum of Fe and Co to be counted as the balance. 20. The recording medium as defined in claim 19, wherein Co amounts to about 12 - about 27 atomic percent of the sum of Fe and Co to be counted as the balance. 21. The recording medium as defined in any one of the preceding claims, wherein the thin film is at least about 0.3 jim thick. 22. The recording medium as defined in claim 21, wherein the thin film is not thicker than about 3 pm. 23. The recording medium as defined in claim 22, wherein the thin film is at least about 0.7 pm thick. 24. The recording medium as defined in any one of the preceding claims, wherein R is Nd and/or Pr. 25. The recording medium as defined in claim 24, wherein R is Nd. 26. The recording medium as defined in any one of the preceding claims, wherein the thin film comprises a microfine-crystalline phase distributed in the amorphous matrix, said microfine-crystalline phase having an average crystal grain size of not exceeding about 10 nm. 27. The recording medium as defined in claim 8, which is a magneto-optic recording medium. 28. A method of producing a perpendicular magnetic recording medium with perpendicular magnetic anisotropy on a substrate comprising the following steps of: a) maintaining a substrate at a temperature between 180 C and a temperature lower than crystallization temperatures of said material elements; and b) forming a thin film having a composition as specified below on the substrate by a metal gas deposition technique: said composition being expressed essentially by a formula; Rx (Fe1yCoy) zMk wherein, by atomic percent, x is 21-60 %, k is 0-10 %, and z is 30-79 % provided that y is zero to less than 0.5 by atomic ratio; wherein 70-100 atomic percent of the entire R consists of Nd and/or Pr, the balance of said R being one or more selected from the group consisting of Y, La, Ce, Sm, Gd, Tb, Dy, Ho, Er and Yb; and wherein said M is at least one selected from the group consisting of Ni, Zr, Nb, V, Ta, Cr, Mo, W, Mn, Bi, Al, Pb, Sb1 Ge, Sn, Si, -Ti and Hf. 29. The method as defined in claim 28, wherein the substrate is maintained at a temperature of 200-300 C. 30. The method as defined in claim 28 or 29, wherein the thin film is formed to a thickness of about 0.3 to about 3 pm. 31. A method of producing a perpendicular magnetic recording medium with perpendicular magnetic anisotropy on a substrate comprising the steps of: a) providing a thin film having a composition as specified below on a substrate by a metal gas deposition technique, and b) cxiaizing the surface of said film to form an oxidized layer; said thin film composition being expressed essentially by a formula: RX (Fe1-yCoy)zMk wherein, by atomic percent, x is 21-60 %, k is 0-10 %, and z is 30-79 % provided that y is zero to less than 0.5 by atomic ratio; wherein 70-100 atomic percent of the entire k consists of Nd and/or Pr, the balance of said R being one or more of Y, La, Ce, Sm, Gd, Tb, Dy, Ho, Er and Yb; and wherein said M is at least one selected from the group consisting of Ni, Zr, Nb, V, Ta, Cr, Mo, W, Mn, Bi, Al, Pb, Sb, Ge, Sn, Si, Ti and Hf. 32. The method as defined in claim 31, wherein the oxidization is effected so as to form the oxidized layer with a thickness up to several tens nm.

Inventors: SAGAWA, MASATO, SUZUKI, TAKAO
Applicants: SUMITOMO SPECIAL METALS CO., LTD.
Application year: 1985
Main classification: G11B5
IPC codes: G11B5