Comparative study of high-latitude, mid-latitude and low-latitude ionosphere on basis of local empirical models
The analysis of the regular features of the high-, mid- and low-latitude ionosphere characteristics has been carried out using local empirical models. The local empirical models were derived from the manual scaled ionogram data recorded by DPS-4 Digisondes located at Norilsk (69N,88E), Irkutsk (52N,...
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Veröffentlicht in: | Advances in space research 2014-08, Vol.54 (3), p.509-516 |
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description | The analysis of the regular features of the high-, mid- and low-latitude ionosphere characteristics has been carried out using local empirical models. The local empirical models were derived from the manual scaled ionogram data recorded by DPS-4 Digisondes located at Norilsk (69N,88E), Irkutsk (52N,104E) and Hainan (19N,109E) for a 6-year period from December, 2002 to December, 2008. The technique used to build the local empirical model is described. Primary focuses are diurnal, seasonal and solar cycle variations of the peak electron density and the peak height under low solar activity and their changes with increasing solar activity. The main objective of the paper is to reveal both common and specific features of high-, mid- and low-latitude ionosphere. Based on earlier comparisons with the International Reference Ionosphere model, we analyze how the common and specific features are reproduced by this model. |
doi_str_mv | 10.1016/j.asr.2014.02.019 |
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The local empirical models were derived from the manual scaled ionogram data recorded by DPS-4 Digisondes located at Norilsk (69N,88E), Irkutsk (52N,104E) and Hainan (19N,109E) for a 6-year period from December, 2002 to December, 2008. The technique used to build the local empirical model is described. Primary focuses are diurnal, seasonal and solar cycle variations of the peak electron density and the peak height under low solar activity and their changes with increasing solar activity. The main objective of the paper is to reveal both common and specific features of high-, mid- and low-latitude ionosphere. Based on earlier comparisons with the International Reference Ionosphere model, we analyze how the common and specific features are reproduced by this model.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/j.asr.2014.02.019</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Construction ; Digisonde ; Diurnal–seasonal–solar activity behavior ; Electron density ; Empirical analysis ; High-latitude, mid-latitude and low-latitude ionosphere ; Ionograms ; Ionosphere ; IRI model ; Local model ; Manuals ; Mathematical models ; Solar activity</subject><ispartof>Advances in space research, 2014-08, Vol.54 (3), p.509-516</ispartof><rights>2013 COSPAR</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c363t-34524fff770608016ce9b6391a1bf19c89498d404eac34a850772009a204608f3</citedby><cites>FETCH-LOGICAL-c363t-34524fff770608016ce9b6391a1bf19c89498d404eac34a850772009a204608f3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.asr.2014.02.019$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3548,27923,27924,45994</link.rule.ids></links><search><creatorcontrib>Ratovsky, K.G.</creatorcontrib><creatorcontrib>Shi, J.K.</creatorcontrib><creatorcontrib>Oinats, A.V.</creatorcontrib><creatorcontrib>Romanova, E.B.</creatorcontrib><title>Comparative study of high-latitude, mid-latitude and low-latitude ionosphere on basis of local empirical models</title><title>Advances in space research</title><description>The analysis of the regular features of the high-, mid- and low-latitude ionosphere characteristics has been carried out using local empirical models. 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Based on earlier comparisons with the International Reference Ionosphere model, we analyze how the common and specific features are reproduced by this model.</description><subject>Construction</subject><subject>Digisonde</subject><subject>Diurnal–seasonal–solar activity behavior</subject><subject>Electron density</subject><subject>Empirical analysis</subject><subject>High-latitude, mid-latitude and low-latitude ionosphere</subject><subject>Ionograms</subject><subject>Ionosphere</subject><subject>IRI model</subject><subject>Local model</subject><subject>Manuals</subject><subject>Mathematical models</subject><subject>Solar activity</subject><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqNUctu2zAQJIoGqOvkA3LjsYdK2SWpB9FTYeQFBOilPRM0tYppSKJKyg7y96Hhor0FPe3uYGawg2HsGqFEwPpmX9oUSwGoShAloP7AVtg2ukCt2o9sBaKRBWLTfGKfU9oDoGgaWLGwCeNso138kXhaDt0rDz3f-eddMWQwA_SVj777e3E7dXwIL_8AH6aQ5h1F4mHiW5t8OnkMwdmB0zj76E_bGDoa0iW76O2Q6OrPXLNfd7c_Nw_F04_7x833p8LJWi6FVJVQfd_nH2toc0BHeltLjRa3PWrXaqXbToEi66SybQVNIwC0FaCyoJdr9uXsO8fw-0BpMaNPjobBThQOyWCthMgmlf4PqqxAaFlhpuKZ6mJIKVJv5uhHG18Ngjn1YPYm92BOPRgQJveQNd_Ompyejp6iSc7T5KjzkdxiuuDfUb8B_O2QLA</recordid><startdate>20140801</startdate><enddate>20140801</enddate><creator>Ratovsky, K.G.</creator><creator>Shi, J.K.</creator><creator>Oinats, A.V.</creator><creator>Romanova, E.B.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20140801</creationdate><title>Comparative study of high-latitude, mid-latitude and low-latitude ionosphere on basis of local empirical models</title><author>Ratovsky, K.G. ; Shi, J.K. ; Oinats, A.V. ; Romanova, E.B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c363t-34524fff770608016ce9b6391a1bf19c89498d404eac34a850772009a204608f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Construction</topic><topic>Digisonde</topic><topic>Diurnal–seasonal–solar activity behavior</topic><topic>Electron density</topic><topic>Empirical analysis</topic><topic>High-latitude, mid-latitude and low-latitude ionosphere</topic><topic>Ionograms</topic><topic>Ionosphere</topic><topic>IRI model</topic><topic>Local model</topic><topic>Manuals</topic><topic>Mathematical models</topic><topic>Solar activity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ratovsky, K.G.</creatorcontrib><creatorcontrib>Shi, J.K.</creatorcontrib><creatorcontrib>Oinats, A.V.</creatorcontrib><creatorcontrib>Romanova, E.B.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ratovsky, K.G.</au><au>Shi, J.K.</au><au>Oinats, A.V.</au><au>Romanova, E.B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Comparative study of high-latitude, mid-latitude and low-latitude ionosphere on basis of local empirical models</atitle><jtitle>Advances in space research</jtitle><date>2014-08-01</date><risdate>2014</risdate><volume>54</volume><issue>3</issue><spage>509</spage><epage>516</epage><pages>509-516</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><abstract>The analysis of the regular features of the high-, mid- and low-latitude ionosphere characteristics has been carried out using local empirical models. The local empirical models were derived from the manual scaled ionogram data recorded by DPS-4 Digisondes located at Norilsk (69N,88E), Irkutsk (52N,104E) and Hainan (19N,109E) for a 6-year period from December, 2002 to December, 2008. The technique used to build the local empirical model is described. Primary focuses are diurnal, seasonal and solar cycle variations of the peak electron density and the peak height under low solar activity and their changes with increasing solar activity. The main objective of the paper is to reveal both common and specific features of high-, mid- and low-latitude ionosphere. Based on earlier comparisons with the International Reference Ionosphere model, we analyze how the common and specific features are reproduced by this model.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.asr.2014.02.019</doi><tpages>8</tpages></addata></record> |
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subjects | Construction Digisonde Diurnal–seasonal–solar activity behavior Electron density Empirical analysis High-latitude, mid-latitude and low-latitude ionosphere Ionograms Ionosphere IRI model Local model Manuals Mathematical models Solar activity |
title | Comparative study of high-latitude, mid-latitude and low-latitude ionosphere on basis of local empirical models |
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