Does impact erosion set the limit to the mass and size of a planet? – Mars as an example - Pham, L.B.S. et al - Talk presented at ISSI meeting : Evolution of Exoplanet Atmospheres and their characterization, ISSI, Bern, Switzerland on 2008-03-18 - CTALK-2022-0090
 
People who viewed this page also viewed:
(159)  Imaging the solar corona in the EUV - Delaboudiniere, J.-P. et al - published in Advances in Space Research, 20, pp. 2231--2237 (1997) - SIDCimport-100
(158)  Enceladus's internal ocean and ice shell constrained from Cassini gravity. - Čadek, O. et al - published in Geophysical Research Letters, 43 issue 11, pp. 5653-5660 (2016) - SCART-2020-0102
(158)  Modeling CMEs with EUHFORIA using different coronal models: evaluation of results with old and new metrics - Samara, E. et al - Poster presented at 17th European Space Weather, Glasgow, Scotland on 2021-10-25 - POSTER-2022-0010
(158)  EIT: Extreme-Ultraviolet Imaging Telescope for the SOHO Mission - Delaboudiniere, J.-P. et al - published in Solar Physics, 162, pp. 291--312 (1995) - SIDCimport-18
(157)  Radiation hardness of AlxGa1-xN photodetectors exposed to Extreme UltraViolet (EUV) light beam - Malinowski, P. et al - published in Proceedings of SPIE, 7361, pp. 73610T-73610T-8 (2009) - SIDCimport-403