Sporadic structures and small-scale irregularity in the nighttime polar ionosphere in the period of high solar activity according to the data of radio occultation measurements on satellite-to-satellite paths
Results of the analysis of 327 sessions of radio occultation on satellite-to-satellite paths are presented. The data are taken in the nighttime polar ionosphere in the regions with latitudes of 67°–88°, and in the period of high solar activity from October 26, 2003 to November 9, 2003. Typical ionos...
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| Veröffentlicht in: | Cosmic research 2009-08, Vol.47 (4), p.259-267 |
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| creator | Yakovlev, O. I. Matyugov, S. S. Anufriev, V. A. Cherkunova, G. P. |
| description | Results of the analysis of 327 sessions of radio occultation on satellite-to-satellite paths are presented. The data are taken in the nighttime polar ionosphere in the regions with latitudes of 67°–88°, and in the period of high solar activity from October 26, 2003 to November 9, 2003. Typical ionospheric changes in the amplitude and phase of decimeter radio waves on paths
GPS
satellites-
CHAMP
satellite are presented. It is demonstrated that these data make it possible to determine characteristics of the sporadic
E
s
structures in the lower ionosphere at heights of 75–120 km. Histograms of distribution of the lower and upper boundaries, thickness, and intensity of the
E
s
structures are presented. Dispersion and spectra of amplitude fluctuations of decimeter radio waves caused by small-scale irregularity of the ionospheric plasma are analyzed. The relation of the polar
E
s
structures and intensity of small-scale plasma irregularity to various manifestations of solar activity is discussed. The efficiency of monitoring the ionospheric disturbances caused by shock waves of the solar wind by the radio occultation method on satellite-to-satellite paths is demonstrated. |
| doi_str_mv | 10.1134/S0010952509040017 |
| format | Article |
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GPS
satellites-
CHAMP
satellite are presented. It is demonstrated that these data make it possible to determine characteristics of the sporadic
E
s
structures in the lower ionosphere at heights of 75–120 km. Histograms of distribution of the lower and upper boundaries, thickness, and intensity of the
E
s
structures are presented. Dispersion and spectra of amplitude fluctuations of decimeter radio waves caused by small-scale irregularity of the ionospheric plasma are analyzed. The relation of the polar
E
s
structures and intensity of small-scale plasma irregularity to various manifestations of solar activity is discussed. The efficiency of monitoring the ionospheric disturbances caused by shock waves of the solar wind by the radio occultation method on satellite-to-satellite paths is demonstrated.</description><identifier>ISSN: 0010-9525</identifier><identifier>EISSN: 1608-3075</identifier><identifier>DOI: 10.1134/S0010952509040017</identifier><language>eng</language><publisher>Dordrecht: SP MAIK Nauka/Interperiodica</publisher><subject>Amplitudes ; Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Global Positioning System ; Ionosphere ; Irregularities ; Physics ; Physics and Astronomy ; Radio occultation ; Radio waves ; Satellite navigation systems ; Solar activity ; Solar flares ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Sun</subject><ispartof>Cosmic research, 2009-08, Vol.47 (4), p.259-267</ispartof><rights>Pleiades Publishing, Ltd. 2009</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c380t-4ae3a560b630cc8ae47f964aead6e652ffd3d02e9475f95f4abe1d52668065253</citedby><cites>FETCH-LOGICAL-c380t-4ae3a560b630cc8ae47f964aead6e652ffd3d02e9475f95f4abe1d52668065253</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0010952509040017$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0010952509040017$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Yakovlev, O. I.</creatorcontrib><creatorcontrib>Matyugov, S. S.</creatorcontrib><creatorcontrib>Anufriev, V. A.</creatorcontrib><creatorcontrib>Cherkunova, G. P.</creatorcontrib><title>Sporadic structures and small-scale irregularity in the nighttime polar ionosphere in the period of high solar activity according to the data of radio occultation measurements on satellite-to-satellite paths</title><title>Cosmic research</title><addtitle>Cosmic Res</addtitle><description>Results of the analysis of 327 sessions of radio occultation on satellite-to-satellite paths are presented. The data are taken in the nighttime polar ionosphere in the regions with latitudes of 67°–88°, and in the period of high solar activity from October 26, 2003 to November 9, 2003. Typical ionospheric changes in the amplitude and phase of decimeter radio waves on paths
GPS
satellites-
CHAMP
satellite are presented. It is demonstrated that these data make it possible to determine characteristics of the sporadic
E
s
structures in the lower ionosphere at heights of 75–120 km. Histograms of distribution of the lower and upper boundaries, thickness, and intensity of the
E
s
structures are presented. Dispersion and spectra of amplitude fluctuations of decimeter radio waves caused by small-scale irregularity of the ionospheric plasma are analyzed. The relation of the polar
E
s
structures and intensity of small-scale plasma irregularity to various manifestations of solar activity is discussed. The efficiency of monitoring the ionospheric disturbances caused by shock waves of the solar wind by the radio occultation method on satellite-to-satellite paths is demonstrated.</description><subject>Amplitudes</subject><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Global Positioning System</subject><subject>Ionosphere</subject><subject>Irregularities</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Radio occultation</subject><subject>Radio waves</subject><subject>Satellite navigation systems</subject><subject>Solar activity</subject><subject>Solar flares</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Sun</subject><issn>0010-9525</issn><issn>1608-3075</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><recordid>eNp9kstu1jAQhS1UJP4WHoCdxQY2ATu-JF6iiptUiUVhHU2dyR9XSRw8DlKfklfC6c9FAsHKHp_vHB1Lw9hTKV5KqfSrayGkcKY2wgld7s0DdpBWtJUSjTljh12udv0ROye6FUK4RtkD-3a9xgR98Jxy2nzeEhKHpec0wzRV5GFCHlLC4zZBCvmOh4XnEfkSjmPOYUa-xqLwEJdI64gJfxIrphB7Hgc-FpbTPQY-h697DHgfUx-WI8_xHu8hww7vbSKP3m9Thlxi-YxApdeMSyZeZoKM0xQyVjlWvwa-Qh7pMXs4wET45Md5wT6_ffPp8n119fHdh8vXV5VXrciVBlRgrLixSnjfAupmcLa8Qm_RmnoYetWLGp1uzODMoOEGZW9qa1tRZKMu2PNT7prilw0pd3MgX5rAgnGjzonGmcYqXcgX_yWlbaSujTZtQZ_9gd7GLS3lH13bONtqoVyB5AnyKRIlHLo1hRnSXSdFt-9C99cuFE998lBhlyOm38H_Nn0Hy5a7DA</recordid><startdate>20090801</startdate><enddate>20090801</enddate><creator>Yakovlev, O. 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P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c380t-4ae3a560b630cc8ae47f964aead6e652ffd3d02e9475f95f4abe1d52668065253</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><topic>Amplitudes</topic><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Global Positioning System</topic><topic>Ionosphere</topic><topic>Irregularities</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Radio occultation</topic><topic>Radio waves</topic><topic>Satellite navigation systems</topic><topic>Solar activity</topic><topic>Solar flares</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Sun</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yakovlev, O. I.</creatorcontrib><creatorcontrib>Matyugov, S. S.</creatorcontrib><creatorcontrib>Anufriev, V. A.</creatorcontrib><creatorcontrib>Cherkunova, G. P.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Cosmic research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Yakovlev, O. I.</au><au>Matyugov, S. S.</au><au>Anufriev, V. A.</au><au>Cherkunova, G. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Sporadic structures and small-scale irregularity in the nighttime polar ionosphere in the period of high solar activity according to the data of radio occultation measurements on satellite-to-satellite paths</atitle><jtitle>Cosmic research</jtitle><stitle>Cosmic Res</stitle><date>2009-08-01</date><risdate>2009</risdate><volume>47</volume><issue>4</issue><spage>259</spage><epage>267</epage><pages>259-267</pages><issn>0010-9525</issn><eissn>1608-3075</eissn><abstract>Results of the analysis of 327 sessions of radio occultation on satellite-to-satellite paths are presented. The data are taken in the nighttime polar ionosphere in the regions with latitudes of 67°–88°, and in the period of high solar activity from October 26, 2003 to November 9, 2003. Typical ionospheric changes in the amplitude and phase of decimeter radio waves on paths
GPS
satellites-
CHAMP
satellite are presented. It is demonstrated that these data make it possible to determine characteristics of the sporadic
E
s
structures in the lower ionosphere at heights of 75–120 km. Histograms of distribution of the lower and upper boundaries, thickness, and intensity of the
E
s
structures are presented. Dispersion and spectra of amplitude fluctuations of decimeter radio waves caused by small-scale irregularity of the ionospheric plasma are analyzed. The relation of the polar
E
s
structures and intensity of small-scale plasma irregularity to various manifestations of solar activity is discussed. The efficiency of monitoring the ionospheric disturbances caused by shock waves of the solar wind by the radio occultation method on satellite-to-satellite paths is demonstrated.</abstract><cop>Dordrecht</cop><pub>SP MAIK Nauka/Interperiodica</pub><doi>10.1134/S0010952509040017</doi><tpages>9</tpages></addata></record> |
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| subjects | Amplitudes Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Global Positioning System Ionosphere Irregularities Physics Physics and Astronomy Radio occultation Radio waves Satellite navigation systems Solar activity Solar flares Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Sun |
| title | Sporadic structures and small-scale irregularity in the nighttime polar ionosphere in the period of high solar activity according to the data of radio occultation measurements on satellite-to-satellite paths |
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