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The response of the atmosphere to solar variations
The present work examines and discusses the response of the atmospheric layers to solar variations, whereas the solar outputs are responsible for the changes in the Earth’s environment. Galactic cosmic ray rates (GCRs), solar cycle lengths (SCLs), sunspots (Rz), coronal index (CI) of solar activitie...
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Published in: | Indian journal of physics 2020-06, Vol.94 (6), p.737-752 |
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container_title | Indian journal of physics |
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creator | El-Borie, M. A. Thabet, A. A. El-Mallah, E. S. Abd El-Zaher, M. Bishara, A. A. |
description | The present work examines and discusses the response of the atmospheric layers to solar variations, whereas the solar outputs are responsible for the changes in the Earth’s environment. Galactic cosmic ray rates (GCRs), solar cycle lengths (SCLs), sunspots (Rz), coronal index (CI) of solar activities, the aa geomagnetic activity index, total solar irradiance (TSI), CO
2
concentrations, global surface temperatures (GSTs), the near-Earth of the northern and southern hemispheres temperatures have been examined. Our results displayed that every SCL has different behaviors to the sensitivity of GST, according to different modulations of GCRs by solar wind/helio-magnetic field parameters. Lower cosmic rays and higher solar irradiance and geomagnetic activity occur when solar activity increases. Furthermore, the average sensitivities of global temperature to geomagnetics aa and total solar irradiance and in turn low-level cloud cover are significant and real. Our results could indicate that geomagnetic disturbances, which driven by the solar wind, may influence global temperature. Both correlations of GST–Rz displayed the same behavior to the end of SC 22nd, and a great discrepancy is observed during the SC 23rd. The observed correlations of Rz with NH and SH temperatures displayed different behaviors. Four different mechanisms are involved in the direct/indirect effect of TSI variations on the Earth’s atmosphere and temperatures. |
doi_str_mv | 10.1007/s12648-019-01502-x |
format | article |
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2
concentrations, global surface temperatures (GSTs), the near-Earth of the northern and southern hemispheres temperatures have been examined. Our results displayed that every SCL has different behaviors to the sensitivity of GST, according to different modulations of GCRs by solar wind/helio-magnetic field parameters. Lower cosmic rays and higher solar irradiance and geomagnetic activity occur when solar activity increases. Furthermore, the average sensitivities of global temperature to geomagnetics aa and total solar irradiance and in turn low-level cloud cover are significant and real. Our results could indicate that geomagnetic disturbances, which driven by the solar wind, may influence global temperature. Both correlations of GST–Rz displayed the same behavior to the end of SC 22nd, and a great discrepancy is observed during the SC 23rd. The observed correlations of Rz with NH and SH temperatures displayed different behaviors. Four different mechanisms are involved in the direct/indirect effect of TSI variations on the Earth’s atmosphere and temperatures.</description><identifier>ISSN: 0973-1458</identifier><identifier>EISSN: 0974-9845</identifier><identifier>DOI: 10.1007/s12648-019-01502-x</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Astrophysics and Astroparticles ; Cloud cover ; Cosmic rays ; Galactic cosmic rays ; Geomagnetism ; Hemispheres ; Irradiance ; Original Paper ; Physics ; Physics and Astronomy ; Sensitivity ; Solar activity ; Solar corona ; Solar cycle ; Solar magnetic field ; Solar wind ; Sunspot cycle ; Sunspots</subject><ispartof>Indian journal of physics, 2020-06, Vol.94 (6), p.737-752</ispartof><rights>Indian Association for the Cultivation of Science 2019</rights><rights>Indian Association for the Cultivation of Science 2019.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c319t-ee54b928b944f705bcb5447ac7b488582f484da67b216b065b4d252a4a3012923</citedby><cites>FETCH-LOGICAL-c319t-ee54b928b944f705bcb5447ac7b488582f484da67b216b065b4d252a4a3012923</cites><orcidid>0000-0003-3850-4936</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27922,27923</link.rule.ids></links><search><creatorcontrib>El-Borie, M. A.</creatorcontrib><creatorcontrib>Thabet, A. A.</creatorcontrib><creatorcontrib>El-Mallah, E. S.</creatorcontrib><creatorcontrib>Abd El-Zaher, M.</creatorcontrib><creatorcontrib>Bishara, A. A.</creatorcontrib><title>The response of the atmosphere to solar variations</title><title>Indian journal of physics</title><addtitle>Indian J Phys</addtitle><description>The present work examines and discusses the response of the atmospheric layers to solar variations, whereas the solar outputs are responsible for the changes in the Earth’s environment. Galactic cosmic ray rates (GCRs), solar cycle lengths (SCLs), sunspots (Rz), coronal index (CI) of solar activities, the aa geomagnetic activity index, total solar irradiance (TSI), CO
2
concentrations, global surface temperatures (GSTs), the near-Earth of the northern and southern hemispheres temperatures have been examined. Our results displayed that every SCL has different behaviors to the sensitivity of GST, according to different modulations of GCRs by solar wind/helio-magnetic field parameters. Lower cosmic rays and higher solar irradiance and geomagnetic activity occur when solar activity increases. Furthermore, the average sensitivities of global temperature to geomagnetics aa and total solar irradiance and in turn low-level cloud cover are significant and real. Our results could indicate that geomagnetic disturbances, which driven by the solar wind, may influence global temperature. Both correlations of GST–Rz displayed the same behavior to the end of SC 22nd, and a great discrepancy is observed during the SC 23rd. The observed correlations of Rz with NH and SH temperatures displayed different behaviors. Four different mechanisms are involved in the direct/indirect effect of TSI variations on the Earth’s atmosphere and temperatures.</description><subject>Astrophysics and Astroparticles</subject><subject>Cloud cover</subject><subject>Cosmic rays</subject><subject>Galactic cosmic rays</subject><subject>Geomagnetism</subject><subject>Hemispheres</subject><subject>Irradiance</subject><subject>Original Paper</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Sensitivity</subject><subject>Solar activity</subject><subject>Solar corona</subject><subject>Solar cycle</subject><subject>Solar magnetic field</subject><subject>Solar wind</subject><subject>Sunspot cycle</subject><subject>Sunspots</subject><issn>0973-1458</issn><issn>0974-9845</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWKt_wNOC5-gkO9kkRyl-QcFLPYdkm7Vb2mZNUqn_3tgVvHkYZgaedwYeQq4Z3DIAeZcYb1BRYLqUAE4PJ2QCWiLVCsXpca4pQ6HOyUVKa4BGMykmhC9Wvoo-DWGXfBW6Kpfd5m1Iw8pHX-VQpbCxsfq0sbe5L9glOevsJvmr3z4lb48Pi9kznb8-vczu57Stmc7Ue4FOc-U0YidBuNYJRGlb6VApoXiHCpe2kY6zxkEjHC654BZtDYxrXk_JzXh3iOFj71M267CPu_LScARgoKTCQvGRamNIKfrODLHf2vhlGJgfN2Z0Y4obc3RjDiVUj6FU4N27j3-n_0l9A_7oZes</recordid><startdate>20200601</startdate><enddate>20200601</enddate><creator>El-Borie, M. 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S.</creatorcontrib><creatorcontrib>Abd El-Zaher, M.</creatorcontrib><creatorcontrib>Bishara, A. A.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Indian journal of physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>El-Borie, M. A.</au><au>Thabet, A. A.</au><au>El-Mallah, E. S.</au><au>Abd El-Zaher, M.</au><au>Bishara, A. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The response of the atmosphere to solar variations</atitle><jtitle>Indian journal of physics</jtitle><stitle>Indian J Phys</stitle><date>2020-06-01</date><risdate>2020</risdate><volume>94</volume><issue>6</issue><spage>737</spage><epage>752</epage><pages>737-752</pages><issn>0973-1458</issn><eissn>0974-9845</eissn><abstract>The present work examines and discusses the response of the atmospheric layers to solar variations, whereas the solar outputs are responsible for the changes in the Earth’s environment. Galactic cosmic ray rates (GCRs), solar cycle lengths (SCLs), sunspots (Rz), coronal index (CI) of solar activities, the aa geomagnetic activity index, total solar irradiance (TSI), CO
2
concentrations, global surface temperatures (GSTs), the near-Earth of the northern and southern hemispheres temperatures have been examined. Our results displayed that every SCL has different behaviors to the sensitivity of GST, according to different modulations of GCRs by solar wind/helio-magnetic field parameters. Lower cosmic rays and higher solar irradiance and geomagnetic activity occur when solar activity increases. Furthermore, the average sensitivities of global temperature to geomagnetics aa and total solar irradiance and in turn low-level cloud cover are significant and real. Our results could indicate that geomagnetic disturbances, which driven by the solar wind, may influence global temperature. Both correlations of GST–Rz displayed the same behavior to the end of SC 22nd, and a great discrepancy is observed during the SC 23rd. The observed correlations of Rz with NH and SH temperatures displayed different behaviors. Four different mechanisms are involved in the direct/indirect effect of TSI variations on the Earth’s atmosphere and temperatures.</abstract><cop>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12648-019-01502-x</doi><tpages>16</tpages><orcidid>https://orcid.org/0000-0003-3850-4936</orcidid></addata></record> |
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subjects | Astrophysics and Astroparticles Cloud cover Cosmic rays Galactic cosmic rays Geomagnetism Hemispheres Irradiance Original Paper Physics Physics and Astronomy Sensitivity Solar activity Solar corona Solar cycle Solar magnetic field Solar wind Sunspot cycle Sunspots |
title | The response of the atmosphere to solar variations |
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