Completed
PRISM Mission so to Phobos and Deimos
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Classroom Contents
Radiation Processing of Dust, Asteroids and Moons - What Does It Do and What Can It Tell Us?
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- 1 Intro
- 2 Organizers
- 3 Webinar Format
- 4 Today's Speaker
- 5 Stars interact with planetary materials
- 6 Definitions: ·lonizing Radiation: lons, electrons, and photons containing energy above the target ionization threshold
- 7 Radiation Chemistry & Space Weathering 101
- 8 Saturnian Magnetosphere Evironm
- 9 Electron environment at Mimas
- 10 The PacMan Anomalies
- 11 MeV Electron Energy Losses in H2O
- 12 Sintering of regolith grains
- 13 Radiation induced diffusion
- 14 Molecular Dynamics Simulation of Elect Excitation in Water Ice
- 15 Estimates of spherical grain sintering rat
- 16 ROUGH Approximations of Resurfacing
- 17 Sintering timescales (Myr) Comparisons with resurfacing rates can constrain surface properties
- 18 Determining the Origins of Phobos and Demos
- 19 Solar wind sputtering of small bod.
- 20 Sputtering and secondary ion detection
- 21 Monte Carlo Simulations
- 22 Sputtering Experiment
- 23 SIMS: Experimental Yields Secondary ion yields for lunar soil exposed to keV energy ions
- 24 Relative Secondary lon Yield
- 25 Simulated lon Trajectories and Densit
- 26 Small body classification
- 27 PRISM Mission so to Phobos and Deimos
- 28 Formation of pre-biotic molecules in spa
- 29 Chiral-specific reactions caused by sp polarized electrons
- 30 Spin-polarized LEE Damage of Chiral Molec
- 31 Argonne National Laboratory
- 32 Amino Acid Damage: Chirality and Magnetization
- 33 XPS Characterization of Deposited Film
- 34 Cross-section statistical testing
