Add to ORKGWe study the thermal conditions in the polar areas of the irregularly shaped Martian moon Phobos. As was previously discussed, we consider direct illumi- nation by the Sun, eclipses by Mars, Mars shine, and single scattering of solar light by other surface areas of Phobos
On Sept. 10, 2007, the Cassini spacecraft encountered Saturn's third largest moon, Iapetus, during t...
A 3D thermal model that includes a discrete subsurface exponential density profile, surface shadowin...
We present a numerical illumination model to calculate direct as well as diffuse or Hapke scattered...
A manned mission to Phobos may be an important precursor and catalyst for the human exploration of M...
This study used high fidelity computer simulation to investigate the lighting conditions, specifical...
The first thermal images of Phobos' shadow on the surface of Mars, in addition to simultaneous visib...
We present a map of the thermal inertia of Phobos, the larger of Mars' two moons, based on observati...
International audienceAbstractWe use the Martian surface temperature response to Phobos transits obs...
Abstract We use the Martian surface temperature response to Phobos transits observed next to the InS...
Following Svitek (Martian Water Frost: Control of Global Distribution by Small-Scale Processes, Ph.D...
The two natural satellites of Mars, Phobos and Deimos are both important targets for scientific inve...
The surfaces of the Martian moons, Phobos and Deimos may offer a stable environment for long-term op...
Mars is accompanied by two small natural satellites. Deimos, the smaller of the two, is orbiting at ...
The surface thermal properties of Phobos and Deimos have been determined from observations made with...
Permanently shadowed regions (PSRs) are present at the Lunar poles. The surface temperature inside a...
On Sept. 10, 2007, the Cassini spacecraft encountered Saturn's third largest moon, Iapetus, during t...
A 3D thermal model that includes a discrete subsurface exponential density profile, surface shadowin...
We present a numerical illumination model to calculate direct as well as diffuse or Hapke scattered...
A manned mission to Phobos may be an important precursor and catalyst for the human exploration of M...
This study used high fidelity computer simulation to investigate the lighting conditions, specifical...
The first thermal images of Phobos' shadow on the surface of Mars, in addition to simultaneous visib...
We present a map of the thermal inertia of Phobos, the larger of Mars' two moons, based on observati...
International audienceAbstractWe use the Martian surface temperature response to Phobos transits obs...
Abstract We use the Martian surface temperature response to Phobos transits observed next to the InS...
Following Svitek (Martian Water Frost: Control of Global Distribution by Small-Scale Processes, Ph.D...
The two natural satellites of Mars, Phobos and Deimos are both important targets for scientific inve...
The surfaces of the Martian moons, Phobos and Deimos may offer a stable environment for long-term op...
Mars is accompanied by two small natural satellites. Deimos, the smaller of the two, is orbiting at ...
The surface thermal properties of Phobos and Deimos have been determined from observations made with...
Permanently shadowed regions (PSRs) are present at the Lunar poles. The surface temperature inside a...
On Sept. 10, 2007, the Cassini spacecraft encountered Saturn's third largest moon, Iapetus, during t...
A 3D thermal model that includes a discrete subsurface exponential density profile, surface shadowin...
We present a numerical illumination model to calculate direct as well as diffuse or Hapke scattered...