The Extreme Ultraviolet Explorer mission - Instrumentation and science goals

Details The Extreme Ultraviolet Explorer mission - Instrumentation and science goals The Extreme Ultraviolet Explorer mission - Instrumentation and science goals

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jbis...41..357b&link_type=abstract

British Interplanetary Society, Journal (ISSN 0007-084X), vol. 41, Aug. 1988, p. 357-361.

Astronomy and Astrophysics

Astronomy

6

Extreme Ultraviolet Explorer Satellite, Nasa Space Programs, Satellite-Borne Instruments, Spaceborne Astronomy, Ultraviolet Astronomy, Astronomical Spectroscopy, Bandpass Filters, Data Simulation, Radiation Sources

Scientific paper

NASA's Extreme Ultraviolet Explorer (EUVE) will carry out an all-sky survey from 80 to 800 Å in four bandpasses. It is expected that many types of sources will be detected, including white dwarfs and late type stars. A deep survey will also be carried out along the ecliptic which will have a limiting sensitivity a factor of 10 better than the all-sky survey in the bandpass from 80 to 300 Å. The payload includes a spectrometer to observe the brighter sources found in the surveys with a spectral resolution of 1 to 2 Å.

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