Spaceflight programs such as the planned Viking landing on Mars require the determination of planetary surface slopes and surface dielectric constants by earth-based methods. Heavy reliance is often placed on radar backscattering data for estimation of these surface properties. An assessment is presented of the basic theory by which the raw radar data are interpreted, and it is shown that serious difficulties and internal inconsistencies are present in the available theoretical formulas. The discussion brings into question the reliability of the presently available results for these surface properties as obtained by earth-based radar methods
The paper deals with the investigation of the Mars subsurface by means of data collected by the Mars...
A semiquantitative appreciation for the physical properties of the Mars surface materials and their ...
The nature of the Martian surface was characterized by means of its reflectance properties. The Mari...
Earth based radar has often observed planets decades before space missions and provided valuable inf...
The topographies of several debris flow units near the Mount St. Helens Volcano were measured at lat...
The radar astronomy activities supported by the Deep Space Network are reported. The high power S- a...
AbstractThe potential for a nadir-looking radar sounder to retrieve significant surface roughness/pe...
Our present knowledge of the topography of Mars is completely inadequate for addressing a wide range...
The planetary radar (e.g. MARSIS) data inversion is based on the selection of groups of stationary f...
Prepared at Langley Research Center.Cover title.Includes bibliographical references (p. 32-33).Mode ...
International audienceThe Selk crater region is the future landing site of NASA's Dragonfly mission ...
Studies sponsored by NASA at the University of Kansas in cooperation with several other universities...
In bistatic radar observations, refected echoes from the surface of a target planet can be analyzed ...
Our efforts have been focused on understanding the physical properties of planetary surfaces using r...
Abstract The interaction of radar signals with a planetary surface is critical for the utility of ra...
The paper deals with the investigation of the Mars subsurface by means of data collected by the Mars...
A semiquantitative appreciation for the physical properties of the Mars surface materials and their ...
The nature of the Martian surface was characterized by means of its reflectance properties. The Mari...
Earth based radar has often observed planets decades before space missions and provided valuable inf...
The topographies of several debris flow units near the Mount St. Helens Volcano were measured at lat...
The radar astronomy activities supported by the Deep Space Network are reported. The high power S- a...
AbstractThe potential for a nadir-looking radar sounder to retrieve significant surface roughness/pe...
Our present knowledge of the topography of Mars is completely inadequate for addressing a wide range...
The planetary radar (e.g. MARSIS) data inversion is based on the selection of groups of stationary f...
Prepared at Langley Research Center.Cover title.Includes bibliographical references (p. 32-33).Mode ...
International audienceThe Selk crater region is the future landing site of NASA's Dragonfly mission ...
Studies sponsored by NASA at the University of Kansas in cooperation with several other universities...
In bistatic radar observations, refected echoes from the surface of a target planet can be analyzed ...
Our efforts have been focused on understanding the physical properties of planetary surfaces using r...
Abstract The interaction of radar signals with a planetary surface is critical for the utility of ra...
The paper deals with the investigation of the Mars subsurface by means of data collected by the Mars...
A semiquantitative appreciation for the physical properties of the Mars surface materials and their ...
The nature of the Martian surface was characterized by means of its reflectance properties. The Mari...