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• W2892233785 abstract "An Earth radiation observatory on the nearside of the Moon could provide long-term measurements complementary to the satellite-based Earth radiation observation data. This study is intended as a preliminary step towards the design of a Moon-based Earth Radiation Observatory (MERO) and its instrumentation. Based on the analysis of data from the JPL Horizons Ephemeris System for an 18.6-years precession cycle, we show that due to the irregularities of the lunar orbit, for a MERO to maintain an all-time whole Earth disk coverage, it needs to be located within the region of 80.5º W–80.5º E and 81.5º S–81.5º N on the nearside of the Moon and requires a minimum angular instantaneous field of view of 2.07º. Additionally, it should have a 360º horizontally and 15.5º vertically orientation adjustability. On one hand there is a risk for a MERO instrument to receive direct sunlight which might excess the radiation allowance of the sensor; on the other hand, a MERO would have a better polar coverage than does a low orbit spacecraft borne Earth observatory. Within the deployable region, a multi-station MERO network may increase the instantaneous spatial coverage by up to around 10% with abundant overlaps to facilitate inter calibration and validation." @default.
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• W2892233785 date "2018-09-11" @default.
• W2892233785 modified "2023-09-26" @default.
• W2892233785 title "Conceptual design of a Moon-based Earth radiation observatory" @default.
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• W2892233785 doi "https://doi.org/10.1080/01431161.2018.1512770" @default.
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