Titlebook: Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere; Eric Quémerais,Martin Snow,Roger-Maurice Bonnet Book 2013

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,Auff?lligkeiten in H?ufigkeitsverteilungen,majority of the previous work on characterizing the lunar reflectance has been in the visible part of the spectrum using ground-based lunar images. The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) can be used to extend the lunar spec

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Begriff der Wahrscheinlichkeit,ison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) both made observations of comet 17P/Holmes at Lyman-α wavelengths. The intent of these observations was to compare the calibration of SWAN and SOLSTICE, rather than to study the properties of comets. The two datasets re

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https://doi.org/10.1007/978-1-4614-6384-9Lyman-alpha Comet Holmes; Lyman-alpha Models; Modeling Interplanetary Background; Moon Irradiance; UV Sp

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Theoretical Foundations of the Welfare Stated by the two ultraviolet (UV) spectrometers on Voyager 1 and Voyager 2 with models and other more recent datasets shows that it is indeed necessary to derive new calibration factors for these two instruments.

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,Auff?lligkeiten in H?ufigkeitsverteilungen,llar observations. Since only a handful of stars in the IUE archive have been converted to the white dwarf scale and many of them are relatively faint, the SOLSTICE catalog of bright stars can be an extremely useful resource for inflight calibration of ultraviolet spectrographs.

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New Horizons Cruise Observations of Lyman-, Emissions from the Interplanetary Mediuml simulations, although the brightness of interplanetary Lyman-. emissions falls off more slowly than expected with radial distance from the Sun. The ratio of Lyman-./Lyman-. brightnesses in the interplanetary medium agrees well with previous measurements by the Voyager ultraviolet spectrometers.