The Optical Solar Sensor (OSD) has been designed to determine the direction towards the center of the Sun's visible disc. The direction to the Sun is computed in the instrument coordinate system relative to the pixels' position on the linear CCDs illuminated with the light passed through the incoming coding mask. The OSD coding mask has three groups of slits with three slits in each group. This mask configuration provides for reliability increase as well as for the required accuracy. ...

Princeton Instruments was incorporated in 1981 and has been building low light systems for its entire history. ... Princeton Instruments uses the latest in computer aided design to engineer the highest performance camera systems possible. ... We work with every major manufacturer of CCD arrays and image intensifiers in the world. ... From early in the company history, Princeton Instruments has offered complete detection systems for many different types of applications. ... Princeton Instruments, Inc. ...

FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 2: FGS Instrument Design > 2.1 The Optical Train . ... Light from the HST Optical Telescope Assembly (OTA) is intercepted by a plane pickoff mirror in front of the HST focal plane and directed into the FGS. The beam is collimated and compressed (by a factor of ~60) by an aspheric collimating mirror, and guided to the optical elements of the Star Selector A (SSA) servo assembly. ...

... Archives . ... When it comes to survey, the first thing comes in my mind is the census packet although I only saw it once (an easy way to disguise my age but this is true) but the questionaire layouts are so carefully and extensively done so as to give me a strong impression. Such survey is designed prior to collecting data so that after collection, data can be analyzed according to statistical methodology suitable to the design of the survey. ... Chandra Blog . ... SAMSI AstroStat Prog. ...

... Taken from the NASA/JPL information summary "Our Solar System at a Glance". The National Aeronautics and Space Administration's (NASA's) automated spacecraft for solar system exploration come in many shapes and sizes. ... Electrical power is required to operate the spacecraft instruments and systems. ... Between 1959 and 1971, NASA spacecraft were dispatched to study the Moon and the solar environment; they also scanned the inner planets other than Earth -- Mercury , Venus and Mars . ...

Next: The OPUS Pipeline Toolkits . ... Table of Contents - Index - PS reprint - PDF reprint . ... OPUS is both a generic event-driven pipeline environment and a set of applications designed to process the spacecraft telemetry at the Space Telescope Science Institute in Baltimore, Maryland. This paper describes those OPUS applications which process the telemetry, validate the integrity of the information, and produce standard FITS (Flexible Image Transport System) data files for further analysis. ...

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...

Slithead identification (which slithead is installed?) will be sensed and reported by the on-board spectrograph computer. ... Observer's software to handle spectrographic observations will be written by JHU and installed on the Fermilab supplied observatory workstation. ... UW will be responsible for the slithead latch-down control. ... Database computer at APO: The observer's software will query the observatory database for information on the currently installed fiber cartridge. ...

... The choice of the spectrograph design (Fig.2) is determined by the quantity R, the overall dimensions of the PF cage and the restrictions on the rigidity of the structure of the device. ... As the camera's objective a fast 4-lens aplanat is used having a focal distance F cam =140 mm and a relative aperture of 1:1.8, the resolution at the centre is no less than 80 gr/mm, that over the field at a distance of 3 mm from the edge along the frame ( ) diagonal is 35 gr/mm. ...