EURD: First Year Results |
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Authors: | Carmen Morales José F Gómez Joaquín Trapero Stuart Bowyer Jerry Edelstein Eric Korpela |
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Institution: | (1) INTA, Laboratorio de Astrofísica Espacial y Física Fundamental, Apartado de Correos 50727, 28080 Madrid, Spain;(2) Space Sciences Laboratory, University of California, Berkeley, CA 94720-5030, USA |
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Abstract: | EURD (Espectrógrafo Ultravioleta extremo de Radiación Difusa), one of the instruments onboard the Spanish satellite MINISAT-01,
is a spectrograph specially designed to detect diffuse radiation, covering the wavelength range of 350-1100 Å, with a spectral
resolution of 6-8 Å. Its main scientific objectives are the detection of the emission line spectrum from the hot phase of
the interstellar medium and the spectrum of the upper atmospheric airglow. In order to reduce geocoronal noise, EURD always
observes in the anti-sun direction and only when the satellite is in orbital eclipse. After more than one year of observation
we have obtained the best spectrum of the upper atmospheric nightglow in this wavelength range, the spectrum of 15 OB stars
and the spectrum of the full Moon throughout the year.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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