MOSIR Project

Contents List

	FDEPS Lecture; 1) Venus - the runaway greenhouse, history of water, super rotation of the atmosphere, general circulation, equator-to-pole temperature gradient. (1/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference
	FDEPS Lecture; 1) Venus - the runaway greenhouse, history of water, super rotation of the atmosphere, general circulation, equator-to-pole temperature gradient. (2/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference
	FDEPS Lecture; 1) Venus - the runaway greenhouse, history of water, super rotation of the atmosphere, general circulation, equator-to-pole temperature gradient. (3/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference
	FDEPS Lecture; 1) Venus - the runaway greenhouse, history of water, super rotation of the atmosphere, general circulation, equator-to-pole temperature gradient. (4/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference
	FDEPS Lecture; 2) Mars - atmospheric pressure controlled by polar cap heat balance, CO2 cycle, water at the triple point, dust storms, weather and climate (1/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 2) Mars - atmospheric pressure controlled by polar cap heat balance, CO2 cycle, water at the triple point, dust storms, weather and climate (2/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 2) Mars - atmospheric pressure controlled by polar cap heat balance, CO2 cycle, water at the triple point, dust storms, weather and climate (3/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 2) Mars - atmospheric pressure controlled by polar cap heat balance, CO2 cycle, water at the triple point, dust storms, weather and climate (4/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 3) Io, Triton, Titan - supersonic atmospheres, atmospheres that collapse in the winter, hydrologic cycles without water, escaping atmospheres (1/3) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 3) Io, Triton, Titan - supersonic atmospheres, atmospheres that collapse in the winter, hydrologic cycles without water, escaping atmospheres (2/3) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 3) Io, Triton, Titan - supersonic atmospheres, atmospheres that collapse in the winter, hydrologic cycles without water, escaping atmospheres (3/3) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 4) Jupiter - winds, jets, vortices, eddy momentum flux, heat budget, lightning, deep winds, equatorial super rotation (1/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 4) Jupiter - winds, jets, vortices, eddy momentum flux, heat budget, lightning, deep winds, equatorial super rotation (2/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 4) Jupiter - winds, jets, vortices, eddy momentum flux, heat budget, lightning, deep winds, equatorial super rotation (3/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 4) Jupiter - winds, jets, vortices, eddy momentum flux, heat budget, lightning, deep winds, equatorial super rotation (4/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 5) Saturn and other giant planets - winds increase with distance from the sun, oscillating spots, shallow or deep, anelastic dynamics (1/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 5) Saturn and other giant planets - winds increase with distance from the sun, oscillating spots, shallow or deep, anelastic dynamics (2/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 5) Saturn and other giant planets - winds increase with distance from the sun, oscillating spots, shallow or deep, anelastic dynamics (3/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 5) Saturn and other giant planets - winds increase with distance from the sun, oscillating spots, shallow or deep, anelastic dynamics (4/4) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2
	FDEPS Lecture; 6) Saturn and other giant planets - winds increase with distance from the sun, oscillating spots, shallow or deep, anelastic dynamics (1/2) Andrew Ingersoll (California Institute of Technology) 2008-11-04 FDEPS Reference1 Reference2

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