An upper bound on the solar radar cross section at 50 MHz
W. A. Coles(University of California San Diego), R. F. Woodman(Instituto Geofísico del Perú), M. P. Sulzer(Arecibo Observatory), Jorge L. Chau(Leibniz Institute of Atmospheric Physics at the Rostock University), J. K. Harmon(University of Puerto Rico at Arecibo)
Cited by 6
Related Papers
The International Pulsar Timing Array project: using pulsars as a gravitational wave detector
|Classical and Quantum Gravity|2010|695
Radar Mapping of Mercury: Full-Disk Images and Polar Anomalies
|Science|1992|203
Propagation observations of the solar wind near the sun
|The Astrophysical Journal|1989|181
Radar mapping of Mercury's polar anomalies
|Nature|1994|152
Thermal Stability of Volatiles in the North Polar Region of Mercury
|Science|2012|148