A.: Mapping the methane on Mars, As- tron. Astrophys., 512, A51, doi:10.1051/0004-6361/200913178, 2010.Fonti, S., Marzo, G.A., 2010. Mapping the methane on mars. Astron. Astrophys. 512. A51.Fonti, S., Marzo, G. A. 2010. Mapping the methane on Mars. Astronomy and ...
Using the extensive data set of the thermal emission spectrometer onboard Mars Global Surveyor and a statistical clustering technique, here we tracked the gas evolution over three martian years using the ν4 Q-branch methane band at 1306cm-1.Results. We identify three localized sources, ...
1994). Relative good agreements between calculated temperatures and downhole measured temperatures were found. On converting temperatures and depths to thermal gradients and comparing, errors ranged from 5 to 25% for both methane/pure water and methane/seawater assumptions, although the seawater assumption...
Cao S, Liu Y, Wang Y (2008) A forecasting and forewarning model for methane hazard in working face of coal mine based on LS-SVM. J China Univ Min Technol 18:172–176. https://doi.org/10.1016/S1006-1266(08)60037-1 Article Google Scholar Chen D, Stow D (2002) The Effect of Tra...
MAPPING METHANE AND WATER DURING NORTHERN MID-WINTER AND MID-SUMMER ON MARSNovak, R. E.Mumma, M. J.Villanueva, G. L.Faggi, SaraLPI Contribution
The main goal of this work is to show the methane behaviour across the planet seasonally. To this aim, we analyze the strongest methane band in the short wavelength channel of the Planetary Fourier Spectrometer (PFS) on board ESA Mars Express (MeX) spacecraft. The optical line depth is ...
The main goal of this work is to show the methane behaviour across the planet seasonally. To this aim, we analyze the strongest methane band in the short wavelength channel of the Planetary Fourier Spectrometer (PFS) on board ESA Mars Express (MeX) spacecraft. The optical line depth is ...
Global apparent short wave infrared (SWIR) (1.64-1.66 渭m) albedo mapping results from data acquired by Methane Sensor for Mars (MSM) onboard Indian Mars Orbiter Mission from October 2014 to February 2015, are presented. Global analysis of low and high albed...
Marsmethane sensor for MarsGlobal apparent short wave infrared (SWIR) (1.64鈥 1.66 m) albedo mapping results from data acquired by Methane Sensor for Mars (MSM) onboard Indian Mars Orbiter Mission from October 2014 to February 2015, are presented. Global analysis of low and high albedo ...
We have searched for CH 4 over the martian disk, but were unable to detect it. Our upper limits are consistent with earlier reports on the methane abundance on Mars. Finally, we have obtained new measurements of CO 2 isotopic ratios in Mars. As compared to the terrestrial values, these ...