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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Thirty Years of Interplanetary Background Data: A Global Viewion factors derived here are significantly different from the values published by Hall (Ultraviolet resonance radiation and the structure of the heliosphere. Dissertation, University of Arizona, 1992).

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Lyman-α Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWANquire significant processing to remove interplanetary and geocoronal backgrounds which increased the uncertainty of the result. However, both instruments measured similar Lyman-α irradiances, confirming their calibration agreement.

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FATAL

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Distribution of Interstellar Hydrogen Atoms in the Heliosphere and Backscattered Solar Lyman-αhe atoms penetrate through the region of the solar wind (SW) interaction with the local interstellar medium (LISM). In the interaction region the atoms can exchange charge with both solar wind and interstellar protons disturbed in the SW/LISM interaction region. Charge exchange results in a disturba

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Solar Parameters for Modeling the Interplanetary Backgroundn Bern, Switzerland was to establish a photometric cross-calibration of various UV and extreme ultraviolet (EUV) heliospheric observations. Realization of this goal required a credible and up-to-date model of the spatial distribution of neutral interstellar hydrogen in the heliosphere, and to that e

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