Opportunities for X-ray remote sensing at Mercury
Contribuinte(s) |
Institute of Mathematics & Physics (ADT) Mathematics and Physics |
---|---|
Data(s) |
04/12/2008
04/12/2008
2001
|
Resumo |
Grande, Manuel; Dunkin, S. K.; Kellett, B., 'Opportunities for X-ray remote sensing at Mercury', Planetary And Space Science (2001) 49(14-15) pp.1553-1559 RAE2008 Mercury is the little known innermost terrestrial planet. A number of significant questions remain unanswered. We describe areas in which a compact imaging X-ray spectrometer could make a valuable contribution. It can provide high quality spectroscopic analysis of Mercury, using the fluorescence technique. A solar monitor is required to provide the calibration of the illumination necessary to produce a global map of absolute Hermean elemental abundances. In the case of Mercury studies of the surface and the magnetosphere form a single linked problem. The intense level of the radiation observed by Mariner 10 suggests that the auroral zone, where the energetic radiation interacts with the surface, is a potential intense source of X-rays. We estimate the fluxes. The solar wind may also contribute to X-ray generation, if it can reach the surface during highly excited periods. We describe briefly the instrument characteristics that could produce these observations. Peer reviewed |
Formato |
7 |
Identificador |
Kellett , B , Dunkin , S K & Grande , M 2001 , ' Opportunities for X-ray remote sensing at Mercury ' Planetary and Space Science , vol 49 , no. 14-15 , pp. 1553-1559 . DOI: 10.1016/S0032-0633(01)00092-7 0032-0633 PURE: 90087 PURE UUID: 35c10c4f-9ff9-49f2-ba23-61e9d3660ecb dspace: 2160/1359 |
Idioma(s) |
eng |
Relação |
Planetary and Space Science |
Tipo |
/dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article Article (Journal) |
Direitos |