| Autor: |
Epstein EE, Soter SL, Oliver JP, Schorn RA, Wilson WJ |
| Jazyk: |
angličtina |
| Zdroj: |
Science (New York, N.Y.) [Science] 1967 Sep 29; Vol. 157 (3796), pp. 1550-2. |
| DOI: |
10.1126/science.157.3796.1550 |
| Abstrakt: |
Observations of the 3.4-millimeter radio emission from Mercury during 1965 and 1966 yielded the following relationship between average brightness temperature T(B) of the disk and the planetocentric phase angle i: T(B) = 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. |
| Databáze: |
MEDLINE |
| Externí odkaz: |
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