Early drives are 130 mm and have the size of full-height 130 mm hard-drives (like in the
IBM PC XT). 130 mm media looks similar to a CD-ROM enclosed in an old-style
caddy, while 90 mm media is about the size of a regular 3-inch
floppy disk, but twice the thickness. The cases provide dust resistance, and the drives themselves have slots constructed in such a way that they always appear to be closed. Original MO systems were
WORM (write once, read many), and later systems were read/write. The disc consists of a
ferromagnetic material sealed beneath a plastic coating. The only physical contact is during recording when a magnetic head is brought into contact with the side of the disc opposite to the laser, similar to
Floptical drives, but not the same. During reading, a
laser projects a beam on the disk and, according to the magnetic state of the surface, the reflected light varies due to the
magneto-optic Kerr effect. During recording, laser power is increased to heat the material to the
Curie point in a single spot. This enables an
electromagnet positioned on the opposite side of the disc to change the local magnetic polarization. The polarization is retained after the temperature drops. Each write cycle requires both a pass to erase a region and another pass to write information. Both passes use the
laser to heat the recording layer; the magnetic field is used to change the magnetic orientation of the recording layer. The electromagnet reverses polarity for writing, and the laser is pulsed to record spots of "1" over the erased region of "0". As a result of this two-pass process, it takes twice as long to write data as it does to read it. In 1990, a 300 mm disc with 7 GB capacity was made available. In 1996,
Direct Overwrite technology was introduced for 90 mm discs eliminating the initial erase pass when writing. This requires special media. By default, magneto-optical drives verify information after writing it to the disc, and are able to immediately report any problems to the operating system. This means writing can actually take three times longer than reading, but it makes the media extremely reliable, unlike the CD-R or DVD-R media upon which data is written without any concurrent data integrity checking. Using a magneto-optical disc is much more like using a
diskette drive than a CD-RW drive. During a read cycle, the laser is operated at a lower power setting, emitting polarized light. The reflected light has a change in Kerr rotation and Kerr ellipticity which is measured by an analyzer and corresponds to either a logical 0 or 1. The 130 mm drives have been available in capacities from 650 MB to 9.2 GB. However, this is split in half over both sides of the disk. The 2.6 GB disks, for example, have a formatted capacity of 1.2 GB per side. The 130 mm drives were always
SCSI. The 90 mm discs had their entire capacity on one side, with no capability to flip them over. The 90 mm drives were produced in SCSI, IDE, and USB formats. Capacities range from 128 MB to 2.3 GB. While they were never particularly popular with consumers (the main consumer market was the 90 mm drives), the 130 mm drives had some lasting service in corporate storage and retrieval. Optical libraries, such as the Hewlett Packard 40XT, were created to automate loading and storing of the disks. A self-contained unit holding 16 or more disks and connected by SCSI to a host computer, the library required specialized archival software to store indices of data, and select disks. Popular uses were for legal document storage and medical imaging, where high reliability, long life, and (at the time) high storage capacity were required. The optical libraries could also manually be used on a Windows 2000/XP machine by selecting and ejecting discs under the Computer Management icon's Removable Storage Service, but this is cumbersome in practice.
LIMDOW Light Intensity Modulated Direct OverWrite (LIMDOW) technology used a different write technology, which improved on the performance levels of earlier magneto-optical devices. LIMDOW disks and drives worked on the same basic principle as a standard magneto-optical drive: the write surface is heated up and took on a magnetic force applied from outside. But instead of using a magnetic head in the drive to make the changes, the magnets were built into the disk itself. The LIMDOW disk has two magnetic layers just behind the reflective writing surface. This write surface can take magnetism from one of those magnetic layers when it is heated up to one temperature; but if it is heated up further, it will take its polarity from the other magnetic layer. To write the data onto the disk, the magneto-optical drive's laser pulses between two powers. At high power, the surface heats up more and takes its magnetic charge from the north pole magnetic layer. At the lower power, it heats up less and takes its magnetic charge from the south pole layer. Thus, with LIMDOW the magneto-optical write process has a single stage, improving write times. Because the magnetic surface is adjacent to the writing surface, rather than somewhere outside the disk itself, the magnetic writing can be done at a higher resolution, including that of the resolution of the laser spot doing the heating up. In the spring of 1997 Plasmon launched its DW260 drive, which used LIMDOW technology for a higher level of performance than previous magneto-optical drives. LIMDOW drives that shipped in the second half of 1997 has search speeds of less than 15 ms and data transfer rates in excess of 4 Mbit/s, which are fast enough for storing audio and streaming
MPEG-2 video. ==Vendors==