TY - JOUR
T1 - Skipper - An innovative U.S. And Russian University space science mission
AU - Levin, Deborah A.
AU - Caveny, Leonard H.
AU - Mann, David M.
AU - Burt, David A.
N1 - Funding Information:
The Ballistic Missile Defense Organization contracted with USU/SDL to conduct the Bow Shock 3 experiment, i.e., Skipper. The design of Skipper is a collaborative university effort with USU/SDL serving as the program manager. The Moscow Aviation Institute and NPO Lavotchkin are the principal subcontractors. USU/SDL is designing the filtered photometers and the atomic oxygen [OI ? 130.4 nm] and hydrogen [HI ?121.5 nm] VUV instruments. The University of Pittsburgh is developing the rapid scanning spectrometers. TsIINIMASH will provide VUV photoionization cells. The Skipper Science Group is headed by the Army Research Office and includes U.S. and Russian participation. The Institute for Defense Analyses has a central role within the Skipper Science Group.
Publisher Copyright:
© 1994 SPIE. All rights reserved.
PY - 1994/7/22
Y1 - 1994/7/22
N2 - Skipper is the third space experiment in the Bow Shock series to obtain aerothermochemistry and emission data from shock-heated layers. Onboard instrumentation will include two scanning spectrometers and 20 photometers. The spectrometers will scan over the range of 0.2 to 0.4 μm. The photometers will be designed to view the VUV and UV wavelengths with emphasis on atomic oxygen, Lyman-alpha, NO, OH, and N2+ wavelengths. The mission starts with launch into a 822 km circular orbit at 97° inclination. Utah State University designed Skipper with their instrumentation module integrated on top of the Russian spacecraft bus. After spacecraft checkout in the 822 km orbit, the satellite uses hydrazine engines to change to an elliptical orbit with a perigee of about 180 km and begins the scientific measurements. The experimenters will then lower the perigee farther (in approximately 10 km steps) 10 increase the signal to noise ratios, as drag and thermal limits permit. These experiments will be completed in a two week period, followed by positioning the satellite for reentiy over a Pacific test range. Additional data will be collected during the reentry (until the satellite burns up) using both onboard instrumentation and ground observation systems. Thermal modeling predicts that data can be collected down to about 80 km (at a speed of 7 km/sec).
AB - Skipper is the third space experiment in the Bow Shock series to obtain aerothermochemistry and emission data from shock-heated layers. Onboard instrumentation will include two scanning spectrometers and 20 photometers. The spectrometers will scan over the range of 0.2 to 0.4 μm. The photometers will be designed to view the VUV and UV wavelengths with emphasis on atomic oxygen, Lyman-alpha, NO, OH, and N2+ wavelengths. The mission starts with launch into a 822 km circular orbit at 97° inclination. Utah State University designed Skipper with their instrumentation module integrated on top of the Russian spacecraft bus. After spacecraft checkout in the 822 km orbit, the satellite uses hydrazine engines to change to an elliptical orbit with a perigee of about 180 km and begins the scientific measurements. The experimenters will then lower the perigee farther (in approximately 10 km steps) 10 increase the signal to noise ratios, as drag and thermal limits permit. These experiments will be completed in a two week period, followed by positioning the satellite for reentiy over a Pacific test range. Additional data will be collected during the reentry (until the satellite burns up) using both onboard instrumentation and ground observation systems. Thermal modeling predicts that data can be collected down to about 80 km (at a speed of 7 km/sec).
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U2 - 10.1117/12.179956
DO - 10.1117/12.179956
M3 - Conference article
AN - SCOPUS:85076642199
SN - 0277-786X
VL - 2217
SP - 292
EP - 306
JO - Proceedings of SPIE - The International Society for Optical Engineering
JF - Proceedings of SPIE - The International Society for Optical Engineering
T2 - Aerial Surveillance Sensing Including Obscured and Underground Object Detection 1994
Y2 - 4 April 1994 through 8 April 1994
ER -