Opportunities for X-ray remote sensing at Mercury


Autoria(s): Kellett, B.; Dunkin, S. K.; Grande, Manuel
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

http://hdl.handle.net/2160/1359

http://dx.doi.org/10.1016/S0032-0633(01)00092-7

Idioma(s)

eng

Relação

Planetary and Space Science

Tipo

/dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article

Article (Journal)

Direitos