Spacecraft Radiation Protection
Astronauts and Robots 2015: Charles Elachi, JPL
Abundance of the Elements Meteoric and Solar
DOSE SPECTRA FROM ENERGETIC PARTICLES AND NEUTRONS (DoSEN) S. Smith 1, N. A. Schwadron 1 C. Bancroft 1, P. Bloser 1, J. Legere 1, J. Ryan 1, H. E. Spence.
SH1 and SH2.1 (Sun & Corona, IP Transport) C. M. S. Cohen (Caltech)
Solar Energetic Particles and Shocks. What are Solar Energetic Particles? Electrons, protons, and heavier ions Energies – Generally KeV – MeV – Much less.
The Lunar Reconnaissance Orbiter (LRO) is the first mission in NASA's Vision for Space Exploration, a plan to return to the moon and then to travel to.
COSPAR, Paris, July 18-25, 2004 Space Weather and Management of Environmental Risks and Hazards Risto Pirjola, Kirsti Kauristie, Hanna Lappalainen Finnish.
+ Hard X-Ray Footpoint Motion and Progressive Hardening in Solar Flares Margot Robinson Mentor: Dr. Angela DesJardins MSU Solar Physics Summer REU, 2010.
The Sources of Solar Hazards in Interplanetary Space Leonard Strachan & Jun Lin (Harvard – Smithsonian Center for Astrophysics) Paper [72.05] “Contributions.
Towards corpuscular diagnostics of coronal mass ejections at the Sun and in the interplanetary medium: The 2 May 1998 event Large solar energetic particle.
Chin-Chun Wu 1, Simon Plunkett 1, Kan Liou 2, Angelos Vourlidas 1, Murray Dryer 3, S. T. Wu 4, Richard A. Mewald 5 1 Space Science Division, Naval Research.