The possible effect of stratospheric quasi-biennial oscillation on the critical frequency of the ionospheric F2-layer
In this study, the coupling between the stratospheric quasi-biennial oscillation (QBO) and the critical frequency of the ionospheric F2-layer (foF2) was analysed statistically. The multiple regression model was used as a statistical tool. The model was developed by adding the sunspot number (SSN), w...
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| Veröffentlicht in: | Pramāṇa 2018-10, Vol.91 (4), p.1-8, Article 54 |
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| description | In this study, the coupling between the stratospheric quasi-biennial oscillation (QBO) and the critical frequency of the ionospheric F2-layer (foF2) was analysed statistically. The multiple regression model was used as a statistical tool. The model was developed by adding the sunspot number (SSN), which affects the foF2 (measured for Madras, Kodaikanal, Bogota, Manila and Tahiti) in the ionosphere at a significant level. Four different ‘Dummy’ sets of data were used in the model in order to observe the effect of the direction (east–west) and the magnitude (for both directions, between 0 and 15 m / s and between 0 and 16 m / s and the largest value) of QBO. It was observed that the variations of foF2 in the range of 60–78% in the model could be explained by SSN and
SSN
2
. The change of 2–13% that occurred in foF2 could be explained by the whole set of QBO. It was also observed that the effect of the direction and magnitude of QBO on foF2 differed between the stations. |
| doi_str_mv | 10.1007/s12043-018-1627-9 |
| format | Article |
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SSN
2
. The change of 2–13% that occurred in foF2 could be explained by the whole set of QBO. It was also observed that the effect of the direction and magnitude of QBO on foF2 differed between the stations.</description><identifier>ISSN: 0304-4289</identifier><identifier>EISSN: 0973-7111</identifier><identifier>DOI: 10.1007/s12043-018-1627-9</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; F 2 region ; Ionosphere ; Multiple regression models ; Observations and Techniques ; Physics ; Physics and Astronomy ; Quasi-biennial oscillation ; Regression analysis ; Statistical analysis ; Stratosphere ; Sunspots</subject><ispartof>Pramāṇa, 2018-10, Vol.91 (4), p.1-8, Article 54</ispartof><rights>Indian Academy of Sciences 2018</rights><rights>Copyright Springer Science & Business Media 2018</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-b5f007062d2e1ca9f84eb4fc8b14519427fbc1a973ef7f21abecc816191ddbfa3</citedby><cites>FETCH-LOGICAL-c316t-b5f007062d2e1ca9f84eb4fc8b14519427fbc1a973ef7f21abecc816191ddbfa3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s12043-018-1627-9$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s12043-018-1627-9$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Sağir, S</creatorcontrib><creatorcontrib>Atici, R</creatorcontrib><creatorcontrib>Özcan, O</creatorcontrib><title>The possible effect of stratospheric quasi-biennial oscillation on the critical frequency of the ionospheric F2-layer</title><title>Pramāṇa</title><addtitle>Pramana - J Phys</addtitle><description>In this study, the coupling between the stratospheric quasi-biennial oscillation (QBO) and the critical frequency of the ionospheric F2-layer (foF2) was analysed statistically. The multiple regression model was used as a statistical tool. The model was developed by adding the sunspot number (SSN), which affects the foF2 (measured for Madras, Kodaikanal, Bogota, Manila and Tahiti) in the ionosphere at a significant level. Four different ‘Dummy’ sets of data were used in the model in order to observe the effect of the direction (east–west) and the magnitude (for both directions, between 0 and 15 m / s and between 0 and 16 m / s and the largest value) of QBO. It was observed that the variations of foF2 in the range of 60–78% in the model could be explained by SSN and
SSN
2
. The change of 2–13% that occurred in foF2 could be explained by the whole set of QBO. It was also observed that the effect of the direction and magnitude of QBO on foF2 differed between the stations.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>F 2 region</subject><subject>Ionosphere</subject><subject>Multiple regression models</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quasi-biennial oscillation</subject><subject>Regression analysis</subject><subject>Statistical analysis</subject><subject>Stratosphere</subject><subject>Sunspots</subject><issn>0304-4289</issn><issn>0973-7111</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kEtLxDAUhYMoOI7-AHcF19HctNPHUgZfMOBmXIckc-NkqG0nSRfz772loishkMA959ycj7FbEPcgRPUQQYoi5wJqDqWseHPGFqKpcl4BwDm9c1HwQtbNJbuK8SAENEW-WrBxu8ds6GP0psUMnUObst5lMQWd-jjsMXibHUcdPTceu87rNuuj9W2rk--7jE6iCBt88pZmLuBxxM6eppRpQqLfnGfJW33CcM0unG4j3vzcS_bx_LRdv_LN-8vb-nHDbQ5l4mblqJso5U4iWN24ukBTOFsbKFZUQFbOWNBUE13lJGiD1tZQQgO7nXE6X7K7OXcIPf0qJnXox9DRSiVFI8qKEAlSwayygUAEdGoI_kuHkwKhJrpqpquIrproqoY8cvZE0nafGP6S_zd9A1SLf1U</recordid><startdate>20181001</startdate><enddate>20181001</enddate><creator>Sağir, S</creator><creator>Atici, R</creator><creator>Özcan, O</creator><general>Springer India</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20181001</creationdate><title>The possible effect of stratospheric quasi-biennial oscillation on the critical frequency of the ionospheric F2-layer</title><author>Sağir, S ; Atici, R ; Özcan, O</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-b5f007062d2e1ca9f84eb4fc8b14519427fbc1a973ef7f21abecc816191ddbfa3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>F 2 region</topic><topic>Ionosphere</topic><topic>Multiple regression models</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quasi-biennial oscillation</topic><topic>Regression analysis</topic><topic>Statistical analysis</topic><topic>Stratosphere</topic><topic>Sunspots</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sağir, S</creatorcontrib><creatorcontrib>Atici, R</creatorcontrib><creatorcontrib>Özcan, O</creatorcontrib><collection>CrossRef</collection><jtitle>Pramāṇa</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sağir, S</au><au>Atici, R</au><au>Özcan, O</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The possible effect of stratospheric quasi-biennial oscillation on the critical frequency of the ionospheric F2-layer</atitle><jtitle>Pramāṇa</jtitle><stitle>Pramana - J Phys</stitle><date>2018-10-01</date><risdate>2018</risdate><volume>91</volume><issue>4</issue><spage>1</spage><epage>8</epage><pages>1-8</pages><artnum>54</artnum><issn>0304-4289</issn><eissn>0973-7111</eissn><abstract>In this study, the coupling between the stratospheric quasi-biennial oscillation (QBO) and the critical frequency of the ionospheric F2-layer (foF2) was analysed statistically. The multiple regression model was used as a statistical tool. The model was developed by adding the sunspot number (SSN), which affects the foF2 (measured for Madras, Kodaikanal, Bogota, Manila and Tahiti) in the ionosphere at a significant level. Four different ‘Dummy’ sets of data were used in the model in order to observe the effect of the direction (east–west) and the magnitude (for both directions, between 0 and 15 m / s and between 0 and 16 m / s and the largest value) of QBO. It was observed that the variations of foF2 in the range of 60–78% in the model could be explained by SSN and
SSN
2
. The change of 2–13% that occurred in foF2 could be explained by the whole set of QBO. It was also observed that the effect of the direction and magnitude of QBO on foF2 differed between the stations.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12043-018-1627-9</doi><tpages>8</tpages></addata></record> |
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| source | SpringerNature Journals; Indian Academy of Sciences |
| subjects | Astronomy Astrophysics and Astroparticles F 2 region Ionosphere Multiple regression models Observations and Techniques Physics Physics and Astronomy Quasi-biennial oscillation Regression analysis Statistical analysis Stratosphere Sunspots |
| title | The possible effect of stratospheric quasi-biennial oscillation on the critical frequency of the ionospheric F2-layer |
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