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The effects of reflected protons on the plasma environment of the moon for parallel interplanetary magnetic fields

Author
HALEKAS, J. S1 ; POPPE, A. R1 ; MCFADDEN, J. P1 ; GLASSMEIER, K.-H2
[1] Space Sciences Laboratory, University of California, Berkeley, California, United States
[2] Institut für Geophysik und Extraterrestrische Physik, Technische Universität Braunschweig, Brunswick, Germany
Source

Geophysical research letters. 2013, Vol 40, Num 17, pp 4544-4548, 5 p ; ref : 1/4 p

CODEN
GPRLAJ
ISSN
0094-8276
Scientific domain
Astronomy earth cosmic environment; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Champ magnétique interplanétaire Champ magnétique Cinétique Comète Ecoulement Etude comparative Fréquence cyclotron ionique Géométrie Lune Onde magnétoacoustique Onde précurseur Oscillation Particule épreuve Plasma Proton Sillage Turbulence Vent solaire Ile Wake Océan Pacifique
Keyword (en)
Interplanetary magnetic field magnetic field kinetics comets flow Comparative study Ion cyclotron frequency geometry Moon Magnetoacoustic wave foreshocks oscillations Test particle Plasma protons Wake turbulence solar wind Wake Pacific Ocean
Keyword (es)
Campo magnético interplanetario Campo magnético Cinética Estudio comparativo Frecuencia ciclotrón iónico Geometría Luna Onda magnetoacústica Onda precursora Oscilación Partícula prueba Plasma Protón Estela (marina) Viento solar Isla Wake Océano Pacífico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
27823195

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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