On the feasibility of characterizing jovian auroral electrons via <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mrow><mml:msubsup><mml:mrow><mml:mtext>H</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math> infrared line-emission analysis-Reference-Cited by-同舟云学术

On the feasibility of characterizing jovian auroral electrons via H3+ infrared line-emission analysis

Published:2012-09 Issue:1 Volume:221 Page:236-247
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Tao Chihiro,Badman Sarah V.,Uno Takeru,Fujimoto Masaki

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

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3. The Cassini Visual and Infrared Mapping Spectrometer (VIMS) investigation;Brown;Space Sci. Rev.,2004

4. Excitation of the FUV Io tail on Jupiter: Characterization of the electron precipitation;Gérard;J. Geophys. Res.,2002

5. Spectral observations of transient features in the FUV jovian polar aurora;Gérard;J. Geophys. Res.,2003

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