Mercury: Observations of the 3.4-Millimeter Radio Emission

Details Mercury: Observations of the 3.4-Millimeter Radio Emission Mercury: Observations of the 3.4-Millimeter Radio Emission

Sep 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967sci...157.1550e&link_type=abstract

Science, Volume 157, Issue 3796, pp. 1550-1552

Physics

3

Scientific paper

Observations of the 3.4-millimeter radio emission from Mercury during 1965 and 1966 yielded the following relationship between average brightness temperature TB of the disk and the planetocentric phase angle i: TB = 277 (± 12) + 97 (± 17) cos[i + 29 deg (± 10 deg)] degrees K The errors are statistical standard; the phase shift corresponds to a phase lag -that is, the maximum and minimum of insolation lag the maximum and minimum of planetary radiation.

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