We developed a non-magnetic (CoCr
x)Zr
y [
x = 30-40 at%,
y = 7-14 at%] seed layer for CoCrPt glass media and investigated the dependence of the media noise and the microstructure on the Zr content of the seed layer. Media with a (CoCr
30)Zr
10 seed layer showed lower media noise owing to reduced grain size in the magnetic layer than the media with a Ta/Zr seed layer (refs. 1 and 2), which in turn had lower media noise than the media with a Cr seed layer. The Zr content of the seed layer should be less than 10 at%, because the grain size in the magnetic layer increased drastically (∼80%) when the Zr content was increased from 10 to 14 at%. The (CoCr
30)Zr
10 seed layer had a nanocrystalline structure, while the (CoCr
30)Zr
14 layer was almost amorphous. A seed layer with a nanocrystalline structure seems to be effective for reducing the grain size in the magnetic layer.
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