Current pixel-based methods of image analysis are too computationally expensive to feasibly discover meaningful changes in Mars surface features in NASA's large, continuously expanding database of satellite imagery. We worked on the beginning stages of a more efficient method of change detection that ...
Geomorphologic analysis of some martian surface images from the Mars 4 and 5 automatic stations. Icarus 26 (2), 219-229.Florenski CP, Basilevski AT, Kuzmin RO, Chernaya IM (1975) Geomorphologic analysis of some Martian surface images from the Mars 4 and 5 automatic stations. Icarus 26:219...
ElectrophoresisFEBS Lett. 1973 Jan 15;29(2):97-100.doi:10.1080/01431169208904129SELIVANOV, A. S.NARAEVA, M. K.GORNY, V. I.KOLESNIKOV, V. I.SHI LIN, B. V.TRONIN, A. A.Taylor & Francis GroupInternational Journal of Remote Sensing...
Our analysis of the rover’s position from locomotion data and camera imagery over that time shows that the rover traversed 450.9 m southwards over a flat surface with mild wheel slippage. Soil parameters determined by terramechanics, which observes wheel–terrain interactions, indicate that the ...
This paper extends the analysis performed in Viúdez-Moreiras et al. (2017) to provide the first comprehensive diurnal, seasonal, and interannual wind speed characterization of Martian surface wind speeds in terms of Weibull best-fit parameters, based on the complete MSL REMS dataset. This wind ...
The terrains and surface features in view of the lander include craters in various stages of degradation and dusty eolian bedforms. Based upon the origin and modification of Homestead hollow and adjacent impact craters, slow mass wasting and eolian processes punctuated by impacts are the dominant pr...
Mars is characterized its barren, rocky surface, which is covered with a thick layer of iron oxide, or rust, giving it its distinctive red color. The planet's landscape features a variety of terrain, including vast plains, towering volcanoes, and deep canyons. One of the most notable ...
The instrument package SEIS (Seismic Experiment for Internal Structure) with the three very broadband and three short-period seismic sensors is installed on the surface on Mars as part of NASA's InSight Discovery mission. When compared to terrestrial installations, SEIS is deployed in a very harsh...
Our interpretation is that, in the tenuous CO2 Martian near-surface environment, the daytime BL is to first order controlled by the infrared radiative heating, fairly independent of elevation, which implies a simple correlation between the BL potential temperature and the inverse pressure (‘pressure...
Erosion by flowing water is one of the major forces shaping the surface of Earth. Studies in the last decade have shown, in particular, that the drainage region of rivers, where water is collected, exhibits scale invariant features characterized by exponents that are the same for rivers around...