Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5597
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dc.contributor.authorGoyal, S. K.en_US
dc.contributor.authorBAPAT, BHAS et al.en_US
dc.coverage.spatialEdinburgh, United Kingdomen_US
dc.date.accessioned2021-02-05T06:14:06Z-
dc.date.available2021-02-05T06:14:06Z-
dc.date.issued2016-07en_US
dc.identifier.citationProceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray; 99054N.en_US
dc.identifier.isbn-en_US
dc.identifier.issn-en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5597-
dc.identifier.urihttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/9905/99054N/Multi-directional-measurements-of-high-energy-particles-from-the-Sun/10.1117/12.2232259.fullen_US
dc.description.abstractAditya Solar wind Particle EXperiment (ASPEX) is one of the scientific experiments onboard the Aditya-L1 mission, the first Indian solar mission planned to be launched in the year of 2019. The primary objective of the ASPEX experiment is to carry out in-situ, multi-directional measurements of solar wind ions in the energy range of 100 eV/n to 5 MeV/n. ASPEX instrument has been configured into two subsystems: Solar Wind Ion Spectrometer (SWIS) and Supra Thermal & Energetic Particle Spectrometer (STEPS). SWIS will measure the angular and energy distribution of solar wind ions in the energy range of 100 eV to 20 keV and STEPS will measure the energy spectrum of high energetic particles from six directions covering the energy range of 20 keV/n to 5 MeV/n. This paper presents the overall configuration of the STEPS subsystem with preliminary results obtained from the bread board model.en_US
dc.language.isoenen_US
dc.publisherSociety of Photo-Optical Instrumentation Engineersen_US
dc.subjectAditya Solar wind Particle EXperimenten_US
dc.subject2016en_US
dc.titleMulti-directional measurements of high energy particles from the Sun-Earth L1 point with STEPSen_US
dc.typeConference Papersen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.doihttps://doi.org/10.1117/12.2232259en_US
dc.identifier.sourcetitleProceedings Volume 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray; 99054Nen_US
dc.publication.originofpublisherForeignen_US
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