Results 151 to 160 of about 3,040 (184)
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Neutron environments on the Martian surface.

Physica medica : PM : an international journal devoted to the applications of physics to medicine and biology : official journal of the Italian Association of Biomedical Physics (AIFB), 2002
Radiation is a primary concern in the planning of a manned mission to Mars. Recent studies using NASA Langley Research Center's HZETRN space radiation transport code show that the low energy neutron fluence on the Martian surface is larger than previously expected.
M S, Clowdsley   +7 more
openaire   +1 more source

Acoustic environment of the Martian surface

Journal of Geophysical Research: Planets, 2001
Prompted by the Mars Microphone aboard the 1998 Mars Polar Lander, a theoretical study of the acoustical environment of the Martian surface has been made to ascertain how the propagation of sound is attenuated under such conditions and to predict what sounds may be detectable by a microphone. Viscous and thermal relaxation (termed classical absorption),
openaire   +1 more source

On the composition of martian surface materials

Icarus, 1967
Abstract Observations were made of Mars with the birefringent interferometer. These observations when combined with spectra of the Sun show that Mars has an extremely strong band at 3.1 μ. This band is presumably produced by hydrated minerals on the surface of Mars.
openaire   +1 more source

pH of the Martian surface

Planetary and Space Science, 1995
Allan A. Mills, Mark R. Sims
openaire   +1 more source

Tracing martian surface interactions with the triple O isotope compositions of meteoritic phosphates

Earth and Planetary Science Letters, 2020
Jeremy J Bellucci   +2 more
exaly  

What Martian Meteorites Reveal About the Interior and Surface of Mars

Journal of Geophysical Research E: Planets, 2020
Arya Udry   +2 more
exaly  

Dielectric Map of the Martian Surface

2005
We have undertaken laboratory electromagnetic characterization of the total set of minerals identified by TES [1] on the Martian surface in order to investigate experimentally the dielectric properties of the sediments covering it in the frequency range from 1 to 1000 MHz.
Heggy, Essam, Pommerol, Antoine
openaire   +1 more source

Martian surface dating model refinement based on Chang'E-5 updated lunar chronology function

Earth and Planetary Science Letters, 2022
Zongyu Yue, Kaichang Di, Sheng Gou
exaly  

Martian Equatorial Atmospheric Tides From Surface Observations

Journal of Geophysical Research E: Planets, 2023
Joonas Leino   +2 more
exaly  

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