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Lunar radiation dose due to cosmic rays and their secondary particles

K. Hayatsu ; Y. Karouji ; Lembit Sihver (Institutionen för teknisk fysik, Nukleär teknik) ; N. Hasebe
61st International Astronautical Congress 2010, IAC 2010.Prague, 27 September-1 October 2010 Vol. 5 (2010), p. 4084-4088.
[Konferensbidrag, refereegranskat]

To be able to safely perform human activities on the lunar surface, it is very important to assess the radiation environment, including the dose from galactic cosmic Rays (GCRs) and large Solar Energetic Particles (SEPs). Especially, large SPEs are highly hazardous to lunar habitants. In this paper, several SPEs have been evaluated in order to estimate the effective dose equivalent on the lunar surface. Several events give more than 1 Sv without any shield.

Denna post skapades 2011-09-13.
CPL Pubid: 146139


Institutioner (Chalmers)

Institutionen för teknisk fysik, Nukleär teknik (2006-2015)


Teknisk fysik

Chalmers infrastruktur