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A statistical study of the relative locations of electron and proton auroral boundaries inferred from meridian scanning photometer observations

Author
ZOU, Y1 ; NISHIMURA, Y1 ; LYONS, L. R1 ; DONOVAN, E. F2
[1] Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, California, United States
[2] Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada
Source

Journal of geophysical research. 2012, Vol 117, Num A6 ; A06206.1-A06206.14 ; ref : 3/4 p

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)
Activité géomagnétique Aurore proton Convection Durée Electron Energie Etude comparative Etude statistique Latitude Ovale auroral Petit Nuage Magellan Proton Précipitation proton Pénétration Raie Hβ Canada Amérique du Nord
Keyword (en)
Geomagnetic activity Proton aurora convection duration electrons energy Comparative study Statistical study latitude Auroral oval Small Magellanic Cloud protons Proton precipitation penetration Hβ line Canada North America
Keyword (es)
Actividad geomagnética Aurora protón Convección Electrón Energía Estudio comparativo Estudio estadístico Ovalo auroral Pequeña Nube Magallanes Protón Precipitación protón Raya Hβ Canada America del norte
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26151265

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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