Comparison of measured galactic background radiation at L-band with model

Radiation from the celestial sky in the spectral window at 1.413 GHz is strong and an accurate accounting of this background radiation is needed for calibration and retrieval algorithms. Modern radio astronomy measurements in this window have been converted into a brightness temperature map of the c...

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Main Authors: Le Vine, D.M., Abraham, S., Kerr, Y.H., Wilson, W.J., Skou, N., Sobjaerg, S.
Format: Conference Proceeding
Language:English
Subjects:
Antenna measurements
Applied geophysics
Atmospheric measurements
Earth sciences
Earth, ocean, space
Exact sciences and technology
Extraterrestrial measurements
Internal geophysics
L-band
Ocean temperature
Radiometers
Remote sensing
Sea measurements
Sea surface
Soil measurements
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cited_by cdi_FETCH-LOGICAL-c1002-bec89b5915ec64c1d0961f358d99ffcfe17ce0e4eb2024200913314ffc9e393a3
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container_end_page 1932 vol.3
container_issue
container_start_page 1930
container_title
container_volume 3
creator Le Vine, D.M.
Abraham, S.
Kerr, Y.H.
Wilson, W.J.
Skou, N.
Sobjaerg, S.
description Radiation from the celestial sky in the spectral window at 1.413 GHz is strong and an accurate accounting of this background radiation is needed for calibration and retrieval algorithms. Modern radio astronomy measurements in this window have been converted into a brightness temperature map of the celestial sky at L-band suitable for such applications. This work presents a comparison of the background predicted by this map with the measurements of several modern L-band remote sensing radiometers.
doi_str_mv 10.1109/IGARSS.2004.1370720
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subjects Antenna measurements
Applied geophysics
Atmospheric measurements
Earth sciences
Earth, ocean, space
Exact sciences and technology
Extraterrestrial measurements
Internal geophysics
L-band
Ocean temperature
Radiometers
Remote sensing
Sea measurements
Sea surface
Soil measurements
title Comparison of measured galactic background radiation at L-band with model
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