TEMPERATURE PROFILE SIMULATION BASED ON THE APOLLO ERA IN-SUIT MEASUREMENTS

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Introduction: The microwave radiometers (MRM) on the Chinese ChangeE-1 (CE1) and ChangeE-2 (CE2) passively measured microwave emission from the lunar surface at four frequencies: 3, 7.8, 19.35, and 37 GHz for the first time.
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Crater is the most typical geologic unit of the moon.As the outer part of a crater, the ejecta often occurs even beyond ten crater diameters, which makes it one of the most important features in lunar
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The Extreme Ultraviolet Camera (EUVC) of Change-3 (CE-3) on the moon provides a global and instantaneous view of the earths plasmasphere.The EUV images of the telescope not only outline the shape of t