Absolute solar 30.4 nm flux from sounding rocket observations during the solar cycle 23 minimum

Citation
Dl. Judge et al., Absolute solar 30.4 nm flux from sounding rocket observations during the solar cycle 23 minimum, J GEO R-S P, 104(A12), 1999, pp. 28321-28324
Citations number
25
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
104
Issue
A12
Year of publication
1999
Pages
28321 - 28324
Database
ISI
SICI code
0148-0227(199912)104:A12<28321:AS3NFF>2.0.ZU;2-F
Abstract
A transmission grating extreme ultraviolet (EUV) spectrometer, nominally id entical to the Charge, Element, and Isotope Analysis System/Solar EUV Monit or (CELIAS/SEM) instrument on the Solar and Heliospheric Observatory (SOHO) , has obtained accurate measurements of the integrated absolute solar extre me ultraviolet irradiance in an 8 nm band pass centered at 30.4 nm. The spe ctrometer also measured the EUV/soft X-ray flux, but those data will be rep orted in a later paper. The instrument was launched an two sounding rocket flights from White Sands Missile Range, New Mexico, on June 26, 1996, and a gain on August 11, 1997, to provide a SOHO underflight calibration database in the EUV. The full disk solar 30.4 +/- 40 nm fluxes measured by it on th e above 2 days were 1.21 x 10(10) and 1.42 x 10(10) photons cm(-2) s(-1) at 1 AU, respectively. These measurements have an absolute la uncertainty of 8.1%.