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- W4236838145 abstract "Measurements of the diffuse background radiation in the 85–115 μ band are presented, as observed from altitudes close to 190 km with a rocket-borne, liquid helium cooled telescope. Evidence is given for detection of the galactic background due to thermal grain emission at galactic latitudes of 5–35°, and at a galactic longitude of ~ 163°. At small latitudes, the background intensity is measured to be ~ 9 × 10 –11 W cm –2 sr –1 ; the average number density of grains derived is consistent with the optically determined measure. The 100 μ data is compared with 20 μ data taken on the same flight, in order to draw some conclusions about the grain emissivity and temperature." @default.
- W4236838145 created "2022-05-12" @default.
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- W4236838145 date "1973-01-01" @default.
- W4236838145 modified "2023-10-16" @default.
- W4236838145 title "Rocket Measurements of the Galactic Background at 100 μ" @default.
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- W4236838145 doi "https://doi.org/10.1017/s0074180900054735" @default.
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