Physics
Scientist
Institute for Terrestrial and Planetary Atmospheres, Stony Brook University, Stony Brook, NY 11777, USA
Monte Carlo computations of the escape of atomic nitrogen from Mars
Numerical Simulations of the Transition from Plate Tectonics to Stagnant Lid Convection: Application to Global Resurfacing on Venus
Production of hot nitrogen atoms in the martian thermosphere
Rebuttal to “Comment on the papers “Production of hot nitrogen atoms in the martian thermosphere” by F. Bakalian (2006), and “Monte Carlo computations of the escape of atomic nitrogen from Mars” by F. Bakalian and R.E. Hartle (2006)"
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