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Introduction

  • Eric Quémerais
  • Martin Snow
  • Roger-Maurice Bonnet
Chapter
Part of the ISSI Scientific Report Series book series (ISSI, volume 13)

Abstract

In this book we discuss the problems encountered for calibrating space-borne instruments in the spectral range 50–300 nm. We also discuss the level of accuracy that can be achieved, and review the different sources of emissions that can be used in that range, i.e. the interplanetary background, stars, and solar system bodies such as planets, moons, and comets. As most of the work presented here is based on comparisons with older datasets obtained by experiments that have been calibrated independently, we also analyse the consistency between existing datasets. Whenever possible, we suggest a correction factor if an older dataset is in disagreement with a more recent one. For example, a comparison of the interplanetary background data acquired 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.

Keywords

Solar Wind Hubble Space Telescope Outer Heliosphere Solar System Body Local Interstellar Medium 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer Science+Business Media New York 2013

Authors and Affiliations

  • Eric Quémerais
    • 1
  • Martin Snow
    • 2
  • Roger-Maurice Bonnet
    • 3
  1. 1.LATMOS-IPSLUniversité Versailles-Saint-QuentinGuyancourtFrance
  2. 2.Laboratory Atmospheric & Space PhysicsUniversity of ColoradoBoulderUSA
  3. 3.International Space Science InstituteBernSwitzerland

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