Over-reflection of hydromagnetic planetary-gravity waves at the solar helmet streamers and magnetic sectors
Overreflection of propagating hydromagnetic planetary-gravity waves incident on the current sheets of the helmet streamers and magnetic sectors of the solar corona is investigated. It is shown that overreflection arises only if the wavenumbers, or the energy fluxes per unit mass, perpendicular to th...
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Veröffentlicht in: | Solar physics 1985-04, Vol.96 (2), p.397-411 |
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description | Overreflection of propagating hydromagnetic planetary-gravity waves incident on the current sheets of the helmet streamers and magnetic sectors of the solar corona is investigated. It is shown that overreflection arises only if the wavenumbers, or the energy fluxes per unit mass, perpendicular to the current sheet of the incident and the transmitted waves in both cases are in opposite directions. The overreflected waves then draw magnetic energy from the Sun's field and communicate it to the interplanetary magnetic field. |
doi_str_mv | 10.1007/BF00149693 |
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M</creatorcontrib><title>Over-reflection of hydromagnetic planetary-gravity waves at the solar helmet streamers and magnetic sectors</title><title>Solar physics</title><description>Overreflection of propagating hydromagnetic planetary-gravity waves incident on the current sheets of the helmet streamers and magnetic sectors of the solar corona is investigated. It is shown that overreflection arises only if the wavenumbers, or the energy fluxes per unit mass, perpendicular to the current sheet of the incident and the transmitted waves in both cases are in opposite directions. The overreflected waves then draw magnetic energy from the Sun's field and communicate it to the interplanetary magnetic field.</description><subject>Astronomy</subject><subject>Corona. Coronal loops, streamers, and holes</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Solar physics</subject><subject>Solar system</subject><issn>0038-0938</issn><issn>1573-093X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1985</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LAzEQhoMoWKsXf0EO4kFYnXx1k6MWq4LQi4K3ZZrNtqv7UZO00n9vSks9epoX5pkX5iHkksEtA8jvHiYATJqREUdkwFQuMjDi45gMAITeZn1KzkL4TFTC1YB8TdfOZ95VjbOx7jvaV3SxKX3f4rxzsbZ02WAK6DfZ3OO6jhv6g2sXKEYaF46GvkFPF65pXaQheoet82nblfRQEVJ378M5OamwCe5iP4fkffL4Nn7OXqdPL-P718wKDjHTTklZajOSUgphwCpUasZLrgEsy0dgFHBTGkSpZioH5IqzUmMFlVBClGJIrne9S99_r1yIRVsH65rtI_0qFFzqHIQy_4JMC660kgm82YHW9yEkW8XS121yUjAotiaLP_EJvtq3YrDYVB47W4fDhZaGCcbEL5wsgmM</recordid><startdate>198504</startdate><enddate>198504</enddate><creator>EL MEKKI, O. 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M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Over-reflection of hydromagnetic planetary-gravity waves at the solar helmet streamers and magnetic sectors</atitle><jtitle>Solar physics</jtitle><date>1985-04</date><risdate>1985</risdate><volume>96</volume><issue>2</issue><spage>397</spage><epage>411</epage><pages>397-411</pages><issn>0038-0938</issn><eissn>1573-093X</eissn><coden>SLPHAX</coden><abstract>Overreflection of propagating hydromagnetic planetary-gravity waves incident on the current sheets of the helmet streamers and magnetic sectors of the solar corona is investigated. It is shown that overreflection arises only if the wavenumbers, or the energy fluxes per unit mass, perpendicular to the current sheet of the incident and the transmitted waves in both cases are in opposite directions. The overreflected waves then draw magnetic energy from the Sun's field and communicate it to the interplanetary magnetic field.</abstract><cop>Boston, MA</cop><cop>Dordrecht</cop><pub>Reidel</pub><doi>10.1007/BF00149693</doi><tpages>15</tpages></addata></record> |
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source | Springer Nature - Complete Springer Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
subjects | Astronomy Corona. Coronal loops, streamers, and holes Earth, ocean, space Exact sciences and technology Solar physics Solar system |
title | Over-reflection of hydromagnetic planetary-gravity waves at the solar helmet streamers and magnetic sectors |
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