Introduction - Université Pierre et Marie Curie Accéder directement au contenu
Chapitre D'ouvrage Année : 2013

Introduction

Résumé

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.

Dates et versions

hal-00870078 , version 1 (04-10-2013)

Identifiants

Citer

Eric Quémerais, Martin Snow, Roger-Maurice Bonnet. Introduction. Quémerais, Eric; Snow, Martin; Bonnet, Roger-Maurice. Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere, Springer, pp.1-3, 2013, ISSI Scientific Report Series, Vol. 13, 978-1-4614-6383-2. ⟨10.1007/978-1-4614-6384-9_1⟩. ⟨hal-00870078⟩
219 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More