Radiation and particle exposure of the martian paleoatmosphere: Implications for the loss of water

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 518, 2002, Pages 553-554

  Selsis, F ^a   Lammer, H ^b   Ribas, I ^c,d   Guinan, E F ^d   Lichtenegger, H I M ^b   Lara, L M ^e   Tehrany, M G ^b,f   Hanslmeier, A ^f  

^a CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^b Austrian Academy of Sciences   (Austria)

^c VILLANOVA UNIVERSITY   (United States)

^d UNIVERSITY OF BARCELONA   (Spain)

^e INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^f UNIVERSITY OF GRAZ   (Austria)

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC COMPOSITION; SATELLITES; SOLAR RADIATION; SUN; WATER; X RAYS;

STARS;

MARTIAN SURFACE ANALYSIS;

EID: 0036766114     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (2)

1. Guinan, E. F. and I. Ribas. Our changing Sun: the role of solar nuclear evolution and magnetic activity on Earth's atmosphere and climate, in: The evolving Sun and its Influence on Planetary Environments, Eds. B. Montesinos, A. Giménz and E. F: Guinan, ASP, in press, 2002.
2. Lammer et al. Loss of water from Mars: Implications for the oxidation of the soil, submitted to J. Geophys. Res., 2002.