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原始太陽系星雲における酸素同位体組成進化の理論とその成立過程
倉本 圭 (北大理)
2008-11-12 森羅万象セミナー
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
参考資料
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
参考資料
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
参考資料
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
参考資料
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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
参考資料1 参考資料2
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