Vertical-structure effects on planetary microwave brightness temperature measurements: Applications to the lunar regolith
- 30 November 1981
- Vol. 48 (2) , 201-229
- https://doi.org/10.1016/0019-1035(81)90105-6
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- A comparison of the thermal and radar characteristics of MarsIcarus, 1981
- Possible effect of subsurface inhomogeneities on the lunar microwave spectrumIcarus, 1977
- The surface of Venus as revealed by Soviet Venera 9 and 10GSA Bulletin, 1977
- Thermal microwave emission from a scattering layerJournal of Geophysical Research, 1975
- Lunar microwave brightness temperature observations reevaluated in the light of Apollo program findingsIcarus, 1975
- Lunar near‐surface structureReviews of Geophysics, 1974
- Mathematical models for the reflection coefficients of dielectric half-spacesRadio Science, 1973
- Apollo 15 measurement of lunar surface brightness temperatures thermal conductivity of the upper 1 1/2 meters of regolithEarth and Planetary Science Letters, 1973
- Remote Probing of the Moon by Infrared and Microwave Emissions and by RadarRadio Science, 1970
- Averaging effect of antenna radiation pattern in measurements of the radio emission of the moonRadiophysics and Quantum Electronics, 1966