Voyager EUV solar spectra during 1981–1993

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book 01 Jan 1994 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 152, pages 315-315 (issn: 0038-0938, eissn: 1573-093X,

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Authors: Giuliana de Toma; R. J. Vervack; B. R. Sandel; R. Stalio;

doi: 10.1007/bf01473223 , 10.1007/978-94-011-0950-5_49

Voyager EUV solar spectra during 1981–1993

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Abstract

EUV solar observations have been obtained with the Voyager 1 and Voyager 2 Ultraviolet Spectrometers since 1981. The two instruments, which are now at a distance of more than 40 AU, cover the wavelength range between 500 and 1700 A at a resolution of about 30 A. Stellar observations have demonstrated their photometric stability, and both instruments are operating correctly and capable of solar observations for the next several years. This long term data set represents the longest monitoring of the sun in this spectral region performed by the same instrument.

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