It will monitor energetic X rays from solar flares and survey the sky with X ray charge coupled device (CCD) sensors along an axis perpendicular to the Sun line.

Charge coupled device (CCD) detectors are planned for these telescopes, which will improve their performance.

Two phased charge coupled devices were to be used as micrometers for both telescopes.

Various experiments were conducted between 1996 and 1997 using KITSAT II payloads that include a charge coupled device (CCD) Earth imaging system (CEIS), a low energy electron detector (LEED) and an infra red sensor experiment (IREX).

It should satisfy servicing for small remote sensors, CCD cameras, scientific experimental instruments, experimental communications and new technology test payloads.

The development of high density two dimensional semi conductor charged couple device (CCD) optical detectors, coupled with low power consumption microprocessors, presented a new opportunity for remote sensing by using inexpensive satellites.

Operational software costs were minimized by modifying software previously developed for JSC apos s Charge Coupled Device Debris Telescope.

The satellite is 1.8 m in height and has a diameter of 1.1. m. It has a total mass of 500 kg and as payload will carry a high resolution CCD camera a low resolution camera (Ocean colour monitor) a high energy particle detector and an ionospheric measurement sensor.

Under ESA contract 10623 93 D, SIRA have provided advice and guidance to the prime contractor, the Astronomical Institute at the University of Berne, Switzerland, on algorithms for detecting and analysing debris using CCD arrays.

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It is based on a system of coupled differential equations for the populations of 80,000 bins in mass, semi major axis and eccentricity.

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It consists of a 1.5 m aperture telescope, a peltier cooled CCD camera with a chip size of 1242 x 1152 pixels, an image processing computer and other scientific and communication equipment.

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Figure I below shows in more detail the fraction as a function of absolute magnitude (H) of recoverable NEOs, while figure II shows those that were precovered in astronomical archives (photographic or charged coupled device) or for which pre existing astrometric observations were identified.

Based on information and data provided by States Parties the following broadly available fuzes and sensors shall be considered as relevant acoustic sensors, break wires, fiber optic wires, infrared sensors, magnetic sensors, pressure sensors, roller arms, scratch wire sensors, seismic vibration sensors, tilt rods, trip wires.

(a) Based on information and data provided by States the following broadly available fuzes and sensors should be considered as relevant acoustic sensors break wires fiber optic wires infra red sensors magnetic sensors pressure sensors roller arms scratch wire sensors seismic vibration sensors tilt rods trip wires.

It's like a wireless accelerometer, pedometer.

For most of the infrared and the ultraviolet, X rays and gamma rays, instruments need to be placed just above the atmosphere.

But inside a standard transformer are two coils of wire.

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