Latitude variations in interplanetary Lyman-α data from the Galileo EUVS modeled with solar He 1083 nm images

Geophysical Research Letters

Volumn 23, Issue 15, 1996, Pages 1893-1896

  Pryor, W R ^a   Barth, C A ^a   Hord, C W ^a   Stewart, A I F ^a   Simmons, K E ^a   Gebben, J J ^a   McClintock, W E ^a   Lineaweaver, S ^a   Ajello, J M ^b   Tobiska, W K ^b   Naviaux, K L ^b   Edberg, S J ^b   White, O R ^c   Sandel, B R ^d  

^a UNIVERSITY OF COLORADO   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MATHEMATICAL MODELS; SOLAR RADIATION; ULTRAVIOLET SPECTROMETERS;

GALILEO EXTREME ULTRAVIOLET SPECTROMETER; LATITUDE MIGRATION; LYMAN PHOTONS; SOLAR ROTATION;

PHOTONS; LUMINANCE;

ECLIPTIC PLANE; EXTREME ULTRAVIOLET SPECTROMETERS; GALILEO; SOLAR MAXIMA; SOLAR ROTATION;

EID: 0040200657     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/96GL01978     Document Type: Article

References (14)

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