Revisiting the identification of methane on Mars using TES data
Revisiting the identification of methane on Mars using TES data
复制标题
使用 TES 数据重新审视火星上甲烷的识别
DOI:
10.1051/0004-6361/201526235
复制
发表时间:
2015
期刊:
影响因子:
--
通讯作者:
A. Blanco
中科院分区:
文献类型:
--
作者:
S. Fonti;F. Mancarella;G. Liuzzi;T. Roush;M. C. Frouard;J. Murphy;A. Blanco
The presence and variability of methane in the Martian atmosphere has been investigated by several authors and spurred a lively discussion. In this context, we address our previous inference of spatial and temporal CH4 variability identified from Mars Global Surveyor Thermal Emission Spectrometer measurements which was used to suggest the possible existence of a martian methane cycle. The importance of the topic requires a clear assessment of such variability to correctly comprehend the possible production and destruction mechanisms of Martian methane. It is therefore important to carefully revisit previous results from a different perspective to confirm them before they are used for further investigations. We here describe in detail a new procedure used to validate these earlier Thermal Emission Spectrometer measurements and thoroughly analyze the results obtained with the revised procedure. In spite of our efforts of defining an efficient data analysis procedure, we have not been able to either confirm or refute the existence of the spatial and temporal variability of methane. Nevertheless, our work has produced new interesting tools, which, with the necessary adaptation, can be of some aid in processing and interpreting planetary spectra and, in general, for all the other cases requiring a preliminary selection of data included in very extensive datasets, which are difficult to be efficiently treated with traditional techniques.