Time dependent model of the interplanetary Lyman α glow: Applications to the SWAN data

Astronomy and Astrophysics

Volumn 488, Issue 1, 2008, Pages 351-359

  Quemerais E ^a,e   Izmodenov, V ^b,c,d   Koutroumpa, D ^a   Malama, Y ^c,d  

^a LABORATOIRE DES SCIENCES DU CLIMAT ET DE L ENVIRONNEMENT   (France)

^b MOSCOW STATE UNIVERSITY   (Russian Federation)

^c Russian Academy of Sciences   (Russian Federation)

^d RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^e UNIVERSITÉ PARIS SUD   (France)

Author keywords

Interplanetary medium; Ultraviolet: solar system

Indexed keywords

ASTROPHYSICS; CRYSTALLOGRAPHY; HYDROGEN; IONIZATION; LINEWIDTH; NONMETALS; PRESSURE; RADIATION EFFECTS; RADIATIVE TRANSFER; SOLAR ENERGY; SOLAR SYSTEM; SOLAR WIND; UPPER ATMOSPHERE;

BACKGROUND EMISSIONS; DATA SETS; HELIOSPHERE; HYDROGEN DISTRIBUTION; INTERFACE EFFECTS; INTERPLANETARY MEDIUM; IONIZATION RATES; LINE-WIDTHS; LINESHIFTS; MODEL RESULTS; PHOTO-IONIZATION; RADIATION PRESSURES; RADIATIVE TRANSFER MODEL; SOLAR CYCLE VARIATIONS; SOLAR CYCLES; SOLAR PARAMETERS; TEMPORAL VARIATIONS; TIME-DEPENDENT; TIME-DEPENDENT MODELS; ULTRAVIOLET: SOLAR SYSTEM;

SOLAR POWER GENERATION;

EID: 49749151000     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078204     Document Type: Article

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