1.0d8 Pa での温度をパラメタとして木星大気の温度と静的安定度を計算する.
温度構造 ※印は基準温度圧力
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obratmos_uranus_x100_560.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_570.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_580.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_590.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_600.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_610.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_620.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_630.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_640.0K-1.0d8Pa.nc_temp.png
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obratmos_uranus_x100_650.0K-1.0d8Pa.nc_temp.png
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静的安定度
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obratmos_uranus_x100_560.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_570.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_580.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_590.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_600.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_610.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_620.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_630.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_640.0K-1.0d8Pa.nc_stab.png
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obratmos_uranus_x100_650.0K-1.0d8Pa.nc_stab.png
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