Drift-parallax determination of the altitude of traveling ionospheric disturbances observed with the Los Alamos radio-beacon interferometer
From 1993 to 1997, the Los Alamos very long baseline interferometer was routinely employed to detect traveling ionospheric disturbances (TID) and inner plasmaspheric irregularities by measuring the change in the electrical phase of several satellite beacon signals that backlit the inner plasmasphere...
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Veröffentlicht in: | Radio Science 1998-11, Vol.33 (6), p.1807-1825 |
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description | From 1993 to 1997, the Los Alamos very long baseline interferometer was routinely employed to detect traveling ionospheric disturbances (TID) and inner plasmaspheric irregularities by measuring the change in the electrical phase of several satellite beacon signals that backlit the inner plasmasphere and ionosphere from geosynchronous orbit. The fortuitous placement of two satellite beacons nearly in the Los Alamos geographic meridian, in late 1995, permits us to infer the nominal altitude of each TID event by employing a novel parallax ranging technique. In the context of this paper, the nominal altitude of a TID refers to the altitude at which the slant‐path averaged, amplitude‐weighted phase perturbation existed along the lines of sight from the interferometer to the satellite. In this paper, we outline the method and present validation results. |
doi_str_mv | 10.1029/98RS02033 |
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The fortuitous placement of two satellite beacons nearly in the Los Alamos geographic meridian, in late 1995, permits us to infer the nominal altitude of each TID event by employing a novel parallax ranging technique. In the context of this paper, the nominal altitude of a TID refers to the altitude at which the slant‐path averaged, amplitude‐weighted phase perturbation existed along the lines of sight from the interferometer to the satellite. 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The fortuitous placement of two satellite beacons nearly in the Los Alamos geographic meridian, in late 1995, permits us to infer the nominal altitude of each TID event by employing a novel parallax ranging technique. In the context of this paper, the nominal altitude of a TID refers to the altitude at which the slant‐path averaged, amplitude‐weighted phase perturbation existed along the lines of sight from the interferometer to the satellite. In this paper, we outline the method and present validation results.</description><subject>ALTITUDE</subject><subject>INFORMATION RETRIEVAL</subject><subject>INTERFEROMETRY</subject><subject>MICROWAVE EQUIPMENT</subject><subject>PHYSICS</subject><subject>RADAR</subject><subject>TRAVELLING IONOSPHERIC DISTURBANCE</subject><issn>0048-6604</issn><issn>1944-799X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1998</creationdate><recordtype>article</recordtype><recordid>eNqF0c1u1DAQB_AIgcRSOPAG4YLgkGLH38eqZdtKW5BaENwsxxmzhiTe2t5-PENfut4G9UY5jSz9_jPWTFW9xWgfo1Z9UvL8ArWIkGfVAitKG6HUz-fVAiEqG84RfVm9Suk3QpgyThfV3VH0LjcbE80wmJu6hwxx9JPJPkx1cHVeQ22G7PO2h4d3NFcw-OlXXUBImzVEb-vep7yNnZkspDp0CeIV9PW1z-uHBquQ6oPBjKVE0_vQdGBs6e-nMs1BDONu7OvqhTNDgjd_6171ffn52-FJs_p6fHp4sGosbRlvWsSAsh4zi60wXJgO804hJazphCTcdT1WvXMOFMGtxAwxqRy4zlorWEvIXvVu7htS9jpZn8Guy3cmsFkTVCI78342mxgut5CyHn2yUHY0Qdgm3QqqGEbivxBLjGRLd_DD05BRIamgEhX6caY2hpQiOL2JfjTxVmOkd2fWj2cudn-2136A239DfX50QVvCS6CZA-VkcPMYMPGP5oIIpn98OdZyuZRkpbg-I_fr8bmK</recordid><startdate>199811</startdate><enddate>199811</enddate><creator>Kirkland, Matt W.</creator><creator>Jacobson, Abram R.</creator><general>Blackwell Publishing Ltd</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>7SP</scope><scope>8FD</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>199811</creationdate><title>Drift-parallax determination of the altitude of traveling ionospheric disturbances observed with the Los Alamos radio-beacon interferometer</title><author>Kirkland, Matt W. ; Jacobson, Abram R.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4256-205e45d15c1c7a67ab16b9097cab7836fbd19dfffe93128150589fefbccc75233</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1998</creationdate><topic>ALTITUDE</topic><topic>INFORMATION RETRIEVAL</topic><topic>INTERFEROMETRY</topic><topic>MICROWAVE EQUIPMENT</topic><topic>PHYSICS</topic><topic>RADAR</topic><topic>TRAVELLING IONOSPHERIC DISTURBANCE</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kirkland, Matt W.</creatorcontrib><creatorcontrib>Jacobson, Abram R.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Electronics & Communications Abstracts</collection><collection>Technology Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Radio Science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kirkland, Matt W.</au><au>Jacobson, Abram R.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Drift-parallax determination of the altitude of traveling ionospheric disturbances observed with the Los Alamos radio-beacon interferometer</atitle><jtitle>Radio Science</jtitle><addtitle>Radio Sci</addtitle><date>1998-11</date><risdate>1998</risdate><volume>33</volume><issue>6</issue><spage>1807</spage><epage>1825</epage><pages>1807-1825</pages><issn>0048-6604</issn><eissn>1944-799X</eissn><abstract>From 1993 to 1997, the Los Alamos very long baseline interferometer was routinely employed to detect traveling ionospheric disturbances (TID) and inner plasmaspheric irregularities by measuring the change in the electrical phase of several satellite beacon signals that backlit the inner plasmasphere and ionosphere from geosynchronous orbit. The fortuitous placement of two satellite beacons nearly in the Los Alamos geographic meridian, in late 1995, permits us to infer the nominal altitude of each TID event by employing a novel parallax ranging technique. In the context of this paper, the nominal altitude of a TID refers to the altitude at which the slant‐path averaged, amplitude‐weighted phase perturbation existed along the lines of sight from the interferometer to the satellite. In this paper, we outline the method and present validation results.</abstract><cop>United States</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/98RS02033</doi><tpages>19</tpages></addata></record> |
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subjects | ALTITUDE INFORMATION RETRIEVAL INTERFEROMETRY MICROWAVE EQUIPMENT PHYSICS RADAR TRAVELLING IONOSPHERIC DISTURBANCE |
title | Drift-parallax determination of the altitude of traveling ionospheric disturbances observed with the Los Alamos radio-beacon interferometer |
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