The solar ionization rate of the interplanetary hydrogen as a function of a heliomagnetic latitude: A new model for the interplanetary Lyman alpha studies

Astrophysics and Space Science

Volumn 274, Issue 1-2, 2000, Pages 143-148

  Summanen, Tuula ^a  

^a FINNISH METEOROLOGICAL INSTITUTE   (Finland)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0034393304     PISSN: 0004640X     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1026552107568     Document Type: Article

References (5)

1. Bertaux, J.-L., Quémerais, E. and Lallement, R.: 1996, Observations of a sky Lyman α groove related to enhanced solar wind mass flux in the neutral sheet, Geophys. Res. Lett. 23, 3675-3678.
2. Bavassano, B., Woo, R. and Bruno, R.: 1997, Heliospheric plasma sheet and coronal streamers, Geophys. Res. Lett. 24, 1655-1658.
3. Brandt, J.C. and Chamberlain, J.W.: 1959, Interplanetary gas. I. Hydrogen radiation in the night sky, Astrophys. J. 130, 670-682.
4. McComas, D.J., Funsten, H.O., Gosling, J.T. and Pryor, W.R.: 1999, Ulysses measurements of variations in the solar wind - interstellar hydrogen charge exchange rate, Geophys. Res. Lett. 26, 2697-2701.
5. Summanen, T.: 1992, Latitudinal distribution of solar wind as deduced from Lyman alpha measurements, Lic thesis, Helsinki University, Finland.