Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign
Solar phase scintillation and solar amplitude scintillation are fundamentally important in deep space mission operations for designing a communication system capable of transmitting signals when the signal path is close to the Sun. The ESA’s BepiColombo measurement data were analyzed in a previous p...
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| Veröffentlicht in: | CEAS space journal 2024, Vol.16 (1), p.87-95 |
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| creator | Chen, Shun-Ping Lanucara, Marco Villalvilla, Jose |
| description | Solar phase scintillation and solar amplitude scintillation are fundamentally important in deep space mission operations for designing a communication system capable of transmitting signals when the signal path is close to the Sun. The ESA’s BepiColombo measurement data were analyzed in a previous paper in terms of the power spectral density of the solar phase scintillation, also with a comparison with Woo’s solar phase scintillation theory, when X-band and Ka-band signals propagate close to the Sun with a small Sun-Earth-Probe (SEP) angle during the superior solar conjunction campaign in March 2021 in its cruise phase to Mercury. In this paper the solar amplitude scintillation is analyzed both by calculating the power spectral density and the scintillation index. The results of scintillation index, derived from these measurement data, fit the NASA JPL’s scintillation index model. |
| doi_str_mv | 10.1007/s12567-023-00491-2 |
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The results of scintillation index, derived from these measurement data, fit the NASA JPL’s scintillation index model.</description><subject>Aerospace Technology and Astronautics</subject><subject>Amplitudes</subject><subject>Bepi Colombo (ESA)</subject><subject>Communications systems</subject><subject>Deep space</subject><subject>Engineering</subject><subject>Original Paper</subject><subject>Power spectral density</subject><subject>Scintillation</subject><subject>Signal paths</subject><subject>Space missions</subject><subject>Superhigh frequencies</subject><issn>1868-2502</issn><issn>1868-2510</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><recordid>eNp9Uc1K5TAULuLAiPoCswq4rp4kbZMu9eIfc8HFKMwupM3pJZc2qUkruPM13MzD-SSTa0V3Lg7ng_P9wPmy7BeFUwogziJlZSVyYDwHKGqas73sgMpK5qyksP-Jgf3MjmPcAgCjRaLSg-zfrXvCONmNnqx3xHfkb95oZ8hufusPPIy9nWaDJLbWTbbvF3ajIxqSwIA6zgEHdBMxetKk9X2P7ZSuZg7Wbcjln_O3l9dILnC0K9_7ofEkziMG6wOJvtchadx2du27c5sitd24o-xHp_uIxx_7MHu4urxf3eTru-vb1fk6bzktplxINCVnIASVpsaSc5DClCBbhrrsirJpEGjVcVmYmjLNsamM4CgaYaBrOD_MThbfMfjHOT1Ebf0cXIpUrIa6qmTJZWKxhdUGH2PATo3BDjo8KwpqV4VaqlCpCvVehWJJxBdRHHefwPBl_Y3qP7szj4E</recordid><startdate>2024</startdate><enddate>2024</enddate><creator>Chen, Shun-Ping</creator><creator>Lanucara, Marco</creator><creator>Villalvilla, Jose</creator><general>Springer Vienna</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0001-9747-2482</orcidid></search><sort><creationdate>2024</creationdate><title>Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign</title><author>Chen, Shun-Ping ; Lanucara, Marco ; Villalvilla, Jose</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c314t-78ed53207718d9e533087d508c2ea5f45bbe016f384d912a3eb6d73e7b7d0fb33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Aerospace Technology and Astronautics</topic><topic>Amplitudes</topic><topic>Bepi Colombo (ESA)</topic><topic>Communications systems</topic><topic>Deep space</topic><topic>Engineering</topic><topic>Original Paper</topic><topic>Power spectral density</topic><topic>Scintillation</topic><topic>Signal paths</topic><topic>Space missions</topic><topic>Superhigh frequencies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Chen, Shun-Ping</creatorcontrib><creatorcontrib>Lanucara, Marco</creatorcontrib><creatorcontrib>Villalvilla, Jose</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>CEAS space journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chen, Shun-Ping</au><au>Lanucara, Marco</au><au>Villalvilla, Jose</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign</atitle><jtitle>CEAS space journal</jtitle><stitle>CEAS Space J</stitle><date>2024</date><risdate>2024</risdate><volume>16</volume><issue>1</issue><spage>87</spage><epage>95</epage><pages>87-95</pages><issn>1868-2502</issn><eissn>1868-2510</eissn><abstract>Solar phase scintillation and solar amplitude scintillation are fundamentally important in deep space mission operations for designing a communication system capable of transmitting signals when the signal path is close to the Sun. 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| subjects | Aerospace Technology and Astronautics Amplitudes Bepi Colombo (ESA) Communications systems Deep space Engineering Original Paper Power spectral density Scintillation Signal paths Space missions Superhigh frequencies |
| title | Investigation of X-band and Ka-band amplitude scintillation based on measurement data collected during ESA’s BepiColombo superior solar conjunction campaign |
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