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The relation of temporal variations of soft X-ray emission from comet hyakutake to variations of ion fluxes in the solar wind

Author
NEUGEBAUER, M1 ; CRAVENS, T. E2 ; LISSE, C. M3 ; IPAVICH, F. M4 ; CHRISTIAN, D3 ; VON STEIGER, R5 ; BOCHSLER, P6 ; SHAH, P. D2 ; ARMSTRONG, T. P2
[1] Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
[2] Department of Physics and Astronomy, University of Kansas, Lawrence, United States
[3] ' Space Telescope Science Institute, Baltimore, Maryland, United States
[4] ' Department of Physics, University of Maryland, College Park, United States
[5] International Space Science Institute, Bern, Switzerland
[6] Physikalisches Institut, University of Bern, Switzerland
Source

Journal of geophysical research. 2000, Vol 105, Num A9, pp 20949-20955 ; ref : 29 ref

ISSN
0148-0227
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Analyse corrélation Comète Echange charge Emission RX Interaction gaz neutre plasma Oxygène ion Proton Rayon X mou Vent solaire
Keyword (en)
Correlation analysis Comets Charge exchange X ray emission Neutral gas plasma interaction Oxygen ions Protons Soft X radiation Solar wind
Keyword (es)
Análisis correlación Emisión RX Interacción gas neutro plasma
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B50 Interplanetary space / 001E03B50E Solar wind interactions with planets, satellites, and comets

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
1495700

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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