Hard disks record data ferromagnetic directional magnetic field, to represent a 0 or a 1 bit. Re-read the data by detecting the magnetization of materials. A typical design consists of a shaft of hard disk that contains one or more flat circular disks called dishes in which data are recorded. The dishes are made of nonmagnetic material, aluminum alloy or glass in general and are coated with a thin layer of magnetic material, usually 10-20 nm thick with an outer layer of carbon for protection. Older disks used iron (III) oxide of a magnetic material, but current disks use a cobalt alloy.
The plates are spun at very high speeds. Information is written in a flat when you turn the devices already can read and write heads that operate very close (a few tens of nanometers in new readers) in the magnetic surface. Reading and writing in the head is used to detect and modify the magnetization of the material immediately below. There is a head for each magnetic platter surface on the stem, mounted on a common arm. An actuator arm (or access arm) moves the head in an arc (roughly radially) across the plates as they spin, allowing each head to access almost the entire surface of the plate as it rotates . The arm moves with an operating coil, or in some older models, a stepper motor.
The magnetic surface of each platter is conceptually divided into several smaller sub-micrometer-sized magnetic regions, each of which is used to encode binary information unit only. Initially, the regions have been oriented horizontally, but from around 2005, the focus has shifted to perpendicular. Due to the nature of the polycrystalline magnetic material each of these magnetic regions is composed of a few hundred magnetic grains. Magnetic grains are typically 10 nm in size and shape to each a single magnetic field. Each region is magnetic in the total magnetic dipole which generates a highly localized magnetic field nearby. A write head to magnetize a region by generating a strong local magnetic field. Early hard drives used an electromagnet to magnetize both the region and then reading its magnetic field by electromagnetic induction. Later versions of inductive heads included metal in Gap (MIG) heads and thin film heads. As higher density data, with the help of gramophone MR (magnetoresistance) entered service, the electrical resistance of the head changes according to the strength of the magnetism of the plate. The development made use of spintronics in the head, the magnetoresistance effect is much larger than previous types, and was nicknamed “giant magnetoresistance (GMR). Inside the mind of today, read and write elements are separate, but nearby in the head actuator arm. The component of the overall reading magneto-resistive while the write element is typically thin-film inductive.
HD heads need to contact the surface of the plate in the air that is very near the base, the air moves in or near the plateau at high speed. [Edit] The recording and playback head are mounted on a block known as the regulator, and the area next to the board, is designed to keep just out of touch. This type of air bearing.
In modern drives, the small size of the magnetized regions creates the danger that their magnetic state can be lost due to thermal effects. To counter this, the trays are covered with two parallel magnetic layers separated by a layer of 3 atoms thick non magnetic element ruthenium, and the two layers are magnetized in the opposite direction, thus enhancing mutual Another technology used to overcome thermal effects which allow greater recording density perpendicular recording, first shipped in 2005 from 2007, technology has been used in many hard drives.
Grain boundaries are very important in the design of hard disk. The reason is that the grains are very small and close together, so that the coupling between adjacent grains is very high. When a grain is magnetized, adjacent grains tend to be parallel to it or demagnetized. Then both stability and SNR data will be sabotaged. A clear grain boundary can weaken the coupling of the grains and subsequently increase the SNR. In longitudinal recording, the single domain grains have uniaxial anisotropy with easy axes lie in the plane of the film. The result of this agreement is that adjacent magnets repel each other. Therefore, the magnetostatic energy is so great that it is difficult to increase the storage density. Perpendicular recording media, by contrast, has the grain easy axis oriented perpendicular to the plane of the disk. The attraction of the magnets adjacent to each other and magnetostatic energy are much lower. Thus, much higher surface density can be achieved in perpendicular recording. Another unique feature of perpendicular recording is a soft magnetic sublayer join disk.This under-recording layer is used to make the writing of magnetic flux that is more effective writing. This will be discussed in the writing process. Therefore, a rapid means of film anisotropy, such as L10-FEPTO and rare earth magnets can be used.