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doc#111 | sets; the temperature of our homes |
doc#117 | a very high temperature at the solid |
doc#117 | of the known temperature of Mars. |
doc#117 | , or low temperatures , the thermal |
doc#117 | , where the temperature variation due to |
doc#117 | to sample the temperature variation at different |
doc#117 | black-body temperature is used to |
doc#117 | -body disk temperature is the temperature |
doc#117 | temperature is the temperature which must be |
doc#117 | black-body temperature correspond to the |
doc#117 | to the physical temperature of the emitting |
doc#117 | average disk brightness temperature by less than |
doc#117 | the average disk temperatures of the nearer |
doc#117 | measured radio brightness temperatures . </p><p> In the |
doc#117 | The constant- temperature contours are much |
doc#117 | the measured antenna temperature change during a |
doc#117 | the average brightness temperature of the moon |
doc#117 | that the brightness temperature of the sky |
doc#117 | The measured brightness temperature is a good |
doc#117 | to the brightness temperature at the center |