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General
Notes on Hard Disk Head Design |
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| There are three basic types of read/write head in
common use today: composite, MIG and thin film. A fourth
design -- magneto resistive -- is already used in high
end tape drives and is starting to be shipped in the
latest high capacity hard disk drives. Composite Head
The ferrite or composite head is composed primarily of
a ferrite core with a wire coil and a glass-filled gap,
and the material used to bond the core to the slider.
Ferrite is a hard material which makes it difficult to
meet today's physical and electrical characteristics
required for higher areal densities. MIG-head
Thin-film head
Thin film heads are created using vacuum deposition,
photolithographic and other similar techniques used in
semiconductor wafer processing, to achieve highly
controllable dimensions and characteristics. Through this
process, the coil winding is deposited on a ceramic base,
creating extremely small heads with equally small and
precise gaps between the pole pieces of the magnetic
recording material. Magneto Resistive head One of the most significant new generations in head technology is the magneto resistive head. This uses similar technology to thin film heads, but features a dual element design comprising a magneto resistive read element which is formed first, to which an inductive write element is added. By incorporating dedicated elements in this way, each part of the head is optimised for performance. Conventional heads use a dual function head, in which the same element controls both read and write: performance, therefore, has to be compromised between the two functions. A key advantage of the magneto resistive head is that it automatically senses flux, whereas an inductive element -- such as used in a thin film head -- has to be energised by the flux. This allows the magneto-resistive head to sense smaller magnetic domains which in turn facilitates smaller bit cells and narrower track widths with both contributing to increased capacities. Designs such as the magneto resistive head certainly seem to point the way forward, particularly for high performance drives. Flying height As we have discussed in this topic, the head
"flies" at sub-micron spacing above the disk
surface on an air bearing created by the geometry of the
head and the rotation of the disk. The flying height has
a major effect on storage densities. With lower flying
heights (i.e. the head closer to the disk), less fringing
occurs, enabling more bits to be stored per inch and the
tracks to be closer together, both resulting in increased
disk capacity. Lower flying heights also permit higher
frequencies which enable higher data rates to be
achieved. Much of the research into head design at Fujitsu is
therefore connected with reducing the flying height.
Since the early '80s it has been brought down from 2.5 to
just 0.15 micrometres today - that's 30 times smaller
than a smoke particle. An obvious goal then would appear
to be total contact heads.
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