Results 191 to 200 of about 4,430 (260)
ABSTRACT Safe and reliable mobility over different kinds of ground is important for planetary rovers on space missions. Since terrain changes might affect the mobility of the rover, energy consumption, and safety, detecting the type of ground in real‐time is vital.
Md Masrul Khan +7 more
wiley +1 more source
Lunar and seasonal patterns of a longnose emperor spawning aggregation in Palau. [PDF]
Muller Karanassos C +9 more
europepmc +1 more source
Abstract This article reports on the initial calibration and performance of the High‐resolution Volatiles and Minerals Moon Mapper (HVM3 ${\mathrm{H}\mathrm{V}\mathrm{M}}^{3}$), slated for launch on the National Aeronautics and Space Administration's Lunar Trailblazer mission.
David R. Thompson +38 more
wiley +1 more source
The oldest anchor for lunar crater chronology constrained by the new age of 4.25 Ga of the South Pole-Aitken basin. [PDF]
Xu YG, Chen J.
europepmc +1 more source
Abstract The Lunar Trailblazer mission aimed to assess the presence of water on the lunar surface using imaging spectroscopy in visible shortwave infrared (VSWIR) coupled with high‐resolution multispectral imaging in thermal midwave‐infrared (MWIR), captured simultaneously over the same target from orbit around the Moon with two different instruments ...
Kevin D. Gauld +5 more
wiley +1 more source
Martian samples, hazards, and biosecurity: Between science and bioethics. [PDF]
Siqueira-Batista R, Gómez F.
europepmc +1 more source
Abstract Coastal inundation occurs when the total height of mean sea level (MSL), tide, and surge, including subsequent propagation into estuaries, exceeds a given threshold. We developed a nonparametric Joint Probability of Maxima Method and applied to four major Australian estuaries, deriving frequency‐based exceedance thresholds and quantifying the ...
K. Palmer +5 more
wiley +1 more source
Effect of Field Line Torsion on the Polarization of ULF Waves
Abstract In this paper we suggest a simple modification of the dipole magnetic field which introduces field‐aligned currents and torsion to the field lines. The resulting field lines are not contained in the meridional planes and have resemblance to the geomagnetic field lines in the dawn and dusk flanks of the magnetosphere. We analyze polarization of
K. Kabin, A. W. Degeling, R. Rankin
wiley +1 more source

