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Soft x-ray imager using multilayer mirror optics for martian exospheric studies

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dc.contributor.author Panini, S. S
dc.contributor.author Narendranath, S
dc.contributor.author Sreekumar, P
dc.contributor.author Athiray, P. S
dc.date.accessioned 2020-11-10T02:37:38Z
dc.date.available 2020-11-10T02:37:38Z
dc.date.issued 2010-07
dc.identifier.citation 3rd International Workshop on Instrumentation for Planetary Mission, held 24-27 October, 2016 in Pasadena, California. LPI Contribution No. 1980, id.4054 en_US
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6745
dc.description Restricted Access http://adsabs.harvard.edu/abs/2016LPICo1980.4054P en_US
dc.description.abstract Planetary 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.iso en en_US
dc.title Soft x-ray imager using multilayer mirror optics for martian exospheric studies en_US
dc.type Other en_US


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