The Solar EUV Experiment (SEE) on the NASA Thermosphere, Ionosphere, Mesosp
here, Energetics and Dynamics (TIMED) mission will measure the solar vacuum
ultraviolet (VUV) spectral irradiance from 1 to 195 nm. To cover this wide
spectral range two different types of instruments are used: a grating spec
trograph for spectra above 25 nm and a set of silicon photodiodes with thin
film filters for the soft x-ray (XUV) below 35 nm. Redundant channels of t
he spectrograph and XUV photodiodes provide in-flight calibration checks on
the time scale of a week, and annual rocket underflight measurements provi
de absolute calibration checks traceable to radiometric standards. Both typ
es of instruments have been developed and night proven as part of a NASA so
lar EUV irradiance rocket experiment. The SEE instrument is currently on th
e NASA TIMED spacecraft at the Johns Hopkins University (JHU) Applied Physi
cs Laboratory (APL). The TIMED launch is planned for October 2000 as a two
year mission. (C) 2000 Elsevier Science Ltd. All rights reserved.