Characterization of solar X-ray response data from the REXIS instrument
Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020
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| Format: | Thesis |
| Language: | eng |
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Massachusetts Institute of Technology
2020
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| Online Access: | https://hdl.handle.net/1721.1/127145 |
| _version_ | 1811079880818819072 |
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| author | Cummings, Andrew T. |
| author2 | Richard P. Binzel and Rebecca A. Masterson. |
| author_facet | Richard P. Binzel and Rebecca A. Masterson. Cummings, Andrew T. |
| author_sort | Cummings, Andrew T. |
| collection | MIT |
| description | Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020 |
| first_indexed | 2024-09-23T11:22:03Z |
| format | Thesis |
| id | mit-1721.1/127145 |
| institution | Massachusetts Institute of Technology |
| language | eng |
| last_indexed | 2024-09-23T11:22:03Z |
| publishDate | 2020 |
| publisher | Massachusetts Institute of Technology |
| record_format | dspace |
| spelling | mit-1721.1/1271452024-05-15T03:34:41Z Characterization of solar X-ray response data from the REXIS instrument Cummings, Andrew T. Richard P. Binzel and Rebecca A. Masterson. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Earth, Atmospheric, and Planetary Sciences. Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020 Cataloged from the official PDF of thesis. Includes bibliographical references (pages 67-68). The REgolith X-ray Imaging Spectrometer (REXIS) is a student-built instrument that was flown on NASA's Origins, Spectral Interpretation, Resource Identification, Safety, Regolith Explorer (OSIRIS-REx) mission. During the primary science observation phase, the REXIS Solar X-ray Monitor (SXM) experienced a lower than anticipated solar x-ray count rate. Solar x-ray count decreased most prominently in the low energy region of instrument detection, and made calibrating the REXIS main spectrometer difficult. This thesis documents a root cause investigation into the cause of the low x-ray count anomaly in the SXM. Vulnerable electronic components are identified, and recommendations for hardware improvements are made to better facilitate future low-cost, high-risk instrumentation. by Andrew T. Cummings. S.B. S.B. Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences 2020-09-03T17:49:20Z 2020-09-03T17:49:20Z 2020 2020 Thesis https://hdl.handle.net/1721.1/127145 1191838987 eng MIT theses may be protected by copyright. Please reuse MIT thesis content according to the MIT Libraries Permissions Policy, which is available through the URL provided. http://dspace.mit.edu/handle/1721.1/7582 116 pages application/pdf Massachusetts Institute of Technology |
| spellingShingle | Earth, Atmospheric, and Planetary Sciences. Cummings, Andrew T. Characterization of solar X-ray response data from the REXIS instrument |
| title | Characterization of solar X-ray response data from the REXIS instrument |
| title_full | Characterization of solar X-ray response data from the REXIS instrument |
| title_fullStr | Characterization of solar X-ray response data from the REXIS instrument |
| title_full_unstemmed | Characterization of solar X-ray response data from the REXIS instrument |
| title_short | Characterization of solar X-ray response data from the REXIS instrument |
| title_sort | characterization of solar x ray response data from the rexis instrument |
| topic | Earth, Atmospheric, and Planetary Sciences. |
| url | https://hdl.handle.net/1721.1/127145 |
| work_keys_str_mv | AT cummingsandrewt characterizationofsolarxrayresponsedatafromtherexisinstrument |