A hard disk platter (or disk) is a component of a hard disk drive: it is the circular disk on which the magnetic data are stored. The rigid nature of the platters in a hard drive is what gives them their name (as opposed to the flexible materials which are used to make floppy disks). Hard drives typically have several platters which are mounted on the same spindle.

Description

The magnetic surface of each platter is divided into small sub-micrometre-sized magnetic regions, each of which is used to represent a single binary unit of information. A typical magnetic region on a hard disk platter (in 2006) is about 200-250 nanometers wide (in the radial direction of the platter) and extends about 25-30 nanometers in the down-track direction (the circumferential direction on the platter), corresponding to about 100 billion bits (gigabits) per square inch of disk area. The material of the main magnetic medium layer is typically a cobalt-based alloy. In today's hard drives each of these magnetic regions is composed of a few hundred magnetic grains, which are the base material that gets magnetized. However, future hard drives may use different systems to create the magnetic regions. As a whole, each magnetic region will have a magnetization.Comparison of the transition width caused by Neel Spikes in continuous media and granular media, at a boundary between two magnetic regions of opposite magnetization

One reason magnetic grains are used as opposed to a continuous magnetic medium is that they reduce the space needed for a magnetic region. In continuous magnetic materials, formations called Neel spikes tend to appear. These are spikes of opposite magnetization, and form for the same reason that bar magnets will tend to align themselves in opposite directions. These cause problems because the spikes cancel each other's magnetic field out, so that at region boundaries, the transition from one magnetization to the other will happen over the length of the Neel spikes. This is called the transition width. Grains help solve this problem because each grain is in theory a single magnetic domain (though not always in practice). This means that the magnetic domains can't grow or shrink to form spikes, and therefore the transition width will be on the order of the diameter of the grains.Therefore, much of the development in hard drives has been in reduction of grain size.

Manufacture

Platters are typically made using an aluminium or glass substrate. In disk manufacturing, a thin coating is deposited on both sides of the substrate, mostly by a vacuum deposition process called magnetron sputtering. The coating has a complex layered structure consisting of various metallic (mostly non-magnetic) alloys as underlayers optimized control of crystallographic orientation and grain size of the actual magnetic media layer on top of them, i.e. the film storing the bits of information. On top of it a protective carbon-based overcoat is deposited in the same sputtering process. In post-processing a nanometer thin polymeric lubricant layer is deposited on top of the sputtered structure by dipping the disk into a solvent solution, after which the disk is buffed by various processes to eliminate small defects and verified by a special sensor on a flying head for absence of any remaining asperities or other defects (where the size of the bit given above roughly sets the scale for what constitutes a significant defect size). In the hard disk drive the hard drive heads fly and move radially over the surface of the spinning platters to read or write the data. Extreme smoothness, durability, and perfection of finish are required properties of a hard disk platter.

In the 2005-2006 a major shift in technology of hard disk drives and of magnetic disks/media began. Originally, in-plane magnetized materials have been used to store the bits but perpendicular magnetization is now taking over. (see perpendicular recording).