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...peeds. These high speed protons are sometimes referred to as [[cosmic ray|cosmic rays]].

| [[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

| [[Boston University]] || [[CRaTER]] Cosmic Ray Telescope for the Effects of Radiation || PI:[[Harlan Spence]] CoI:[[Justi

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

*[[Radiation Sickness]] - e.g. cosmic rays, solar radiation, nuclear piles, RTGs *[[Ionizing Photons]] - X-ray, Gamma-ray, Ultra-violet

Title: Resources of the Moon: Solar Wind/Cosmic Ray Derived</ref>.

...move into space habitats, NASA researchers explain: "Many individual gamma-ray lines from a wide variety of different elements in the solar atmosphere hav ...ith the electrons and protons of the solar wind plasma and with unhindered cosmic rays with the power to break atomic nuclei. If even that does not relieve