...peeds. These high speed protons are sometimes referred to as [[cosmic ray|cosmic rays]].
1 KB (180 words) - 00:49, 28 September 2007
| [[University of Helsinki Observatory ]] || [[Smart-1]] || [[XSM]] X-ray Solar Monitor || [[Juhani Huovelin]] [http://http://smart.esa.int/science-
...tory]] || [[Smart-1]] || [[D-CIXS]] Demonstration of a Compact Imaging X-ray Spectrometer || [[Dr Manuel Grande]] [http://www.sstd.rl.ac.uk/SMART-1/ind
8 KB (824 words) - 10:10, 14 June 2012
| [[Boston University]] || [[CRaTER]] Cosmic Ray Telescope for the Effects of Radiation || PI:[[Harlan Spence]] CoI:[[Justi
3 KB (412 words) - 08:07, 26 January 2011
For her doctoral thesis under advisor B. Ray Hawke at the University of Hawaii, Cassandra Coombs scoured [[Lunar Orbiter
...ing is sufficient against [[Solar Proton Events]], but powerful [[Galactic Cosmic Rays]] need roughly six meters for effective shielding. Their analysis took
6 KB (824 words) - 05:49, 2 September 2020
*[[Radiation Sickness]] - e.g. cosmic rays, solar radiation, nuclear piles, RTGs
*[[Ionizing Photons]] - X-ray, Gamma-ray, Ultra-violet
5 KB (702 words) - 19:03, 20 October 2013
Title: Resources of the Moon: Solar Wind/Cosmic Ray Derived</ref>.
12 KB (1,911 words) - 06:49, 4 April 2016
