技術的な課題
Fit into a small housing
Remain close to ambient temperature
Precise power
Overcoming wave-front aberrations in search of deep space discoveries
Overcoming wave-front aberrations in search of deep space discoveries
Microgate, established in 1989 and located in Bolzano Italy, designs linear motor-drive control systems for Extremely Large Telescopes (ELTs), which are the biggest telescope installations on the planet. Used for deep space exploration, ELT’s require highly sophisticated automated optics to capture the weakest light arriving from trillions of miles away to produce high resolution images. Atmospheric disturbances known as a wave-front aberration, degrade light sources and distort imagery, and require a delicate process to re-align and remove these aberrations.
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solution-statement
Thermally adept high density power modules are mission critical to adaptive optics
Microgate has developed an innovative adaptive optics technology that overcomes the complex wave-front aberration challenge. The system consists of a primary mirror that reflects captured light to a secondary adaptive mirror, which physically deforms the light to re-establish what is known as a “plane” wave-front. Deforming the mirror to manipulate the incoming wave-front is achieved using sophisticated contactless linear motors. These motors, correct for atmospheric disturbances and enhance images.
Vicor advantages
Vicor の特長
Power dense
Lightweight
Thermally adept
Power dense modules enable a thermally-adept solution with precise voltage regulation
The adaptive mirror of the European Extremely Large Telescope (E- ELT)is 2.4 meters in diameter and is made of specialized glass, 1.9 millimeters thick. Linear motors are powered by a precise current driver and a series of co-located permanent magnets. These are attached to the back of the mirror and provide the force to deform the glass. This process is performed across the entire surface of the adaptive optics using 5,316 motors, each with an inter-axis distance, or pitch, of about 30 millimeters.
Precise manipulation and thermal management of the adaptive optics system is critical and requires all exposed surfaces to be kept close to ambient temperature to avoid local turbulence.
The Vicor DCM3623 series of DC-DC converter powers the linear motors in the adaptive mirror. The power system board is mounted on the underside of the gas-cooled cold plate, and each module powers up to 36 motors, eliminating complex wiring.
電力供給ネットワーク（PDN）
The Microgate power delivery network uses the Vicor DCM3623 to deform the secondary lens. The voice-coil motors are driven by a precise current driver and a series of co-located permanent magnets that provide the force to deform the glass. This process is performed across the adaptive optics lens using 5,316 motors powered by multiple Vicor DCM3623 DC-DC converters.
The Microgate power delivery network uses the Vicor DCM3623 to deform the secondary lens. The voice-coil motors are driven by a precise current driver and a series of co-located permanent magnets that provide the force to deform the glass. This process is performed across the adaptive optics lens using 5,316 motors powered by multiple Vicor DCM3623 DC-DC converters.
絶縁 レギュレータ
入力電圧: 9 – 420V
出力電圧: 3.3, 5, 12, 13.8, 15, 24, 28, 36, 48V
出力電力: 最大1300W
効率: 最大96%
24.8 x 22.8 x 7.21mm 他