Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6745
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dc.contributor.authorPanini, S. S-
dc.contributor.authorNarendranath, S-
dc.contributor.authorSreekumar, P-
dc.contributor.authorAthiray, P. S-
dc.date.accessioned2020-11-10T02:37:38Z-
dc.date.available2020-11-10T02:37:38Z-
dc.date.issued2010-07-
dc.identifier.citation3rd International Workshop on Instrumentation for Planetary Mission, held 24-27 October, 2016 in Pasadena, California. LPI Contribution No. 1980, id.4054en_US
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6745-
dc.descriptionRestricted Access http://adsabs.harvard.edu/abs/2016LPICo1980.4054Pen_US
dc.description.abstractPlanetary X ray measurements in the past have yielded valuable science in several areas such as the surface chemistry, polar auroras, magnetospheres and solar wind interaction with the exosphere. X-ray spectrometers have been flown in several missions primarily to map the surface elemental abundances. We are developing a soft X-ray imager where multilayer mirrors are used to selectively image the energies of interest onto the focal plane detector. This would be thus capable of doing imaging spectroscopy of the Martian exosphere.en_US
dc.language.isoenen_US
dc.titleSoft x-ray imager using multilayer mirror optics for martian exospheric studiesen_US
dc.typeOtheren_US
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