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Solar X-ray Jets, Type-II Spicules, Granule-size Emerging Bipoles, and the Genesis of the Heliosphere
From Hinode observations of solar X-ray jets, Type-II spicules, and granule-size emerging bipolar magnetic fields in quiet regions and coronal holes, we advocate a scenario for powering coronal heating and the solar wind. In this scenario, Type-II spicules and Alfven waves are generated by the granu...
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Published in: | Astrophysical journal. Letters 2011-04, Vol.731 (1), p.L18-jQuery1323917968051='48' |
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creator | Moore, Ronald L Sterling, Alphonse C Cirtain, Jonathan W Falconer, David A |
description | From Hinode observations of solar X-ray jets, Type-II spicules, and granule-size emerging bipolar magnetic fields in quiet regions and coronal holes, we advocate a scenario for powering coronal heating and the solar wind. In this scenario, Type-II spicules and Alfven waves are generated by the granule-size emerging bipoles (EBs) in the manner of the generation of X-ray jets by larger magnetic bipoles. From observations and this scenario, we estimate that Type-II spicules and their co-generated Alfven waves carry into the corona an area-average flux of mechanical energy of ~7 X 105 erg cm--2 s--1. This is enough to power the corona and solar wind in quiet regions and coronal holes, and therefore indicates that the granule-size EBs are the main engines that generate and sustain the entire heliosphere. |
doi_str_mv | 10.1088/2041-8205/731/1/L18 |
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Letters</title><description>From Hinode observations of solar X-ray jets, Type-II spicules, and granule-size emerging bipolar magnetic fields in quiet regions and coronal holes, we advocate a scenario for powering coronal heating and the solar wind. In this scenario, Type-II spicules and Alfven waves are generated by the granule-size emerging bipoles (EBs) in the manner of the generation of X-ray jets by larger magnetic bipoles. From observations and this scenario, we estimate that Type-II spicules and their co-generated Alfven waves carry into the corona an area-average flux of mechanical energy of ~7 X 105 erg cm--2 s--1. 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Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Moore, Ronald L</au><au>Sterling, Alphonse C</au><au>Cirtain, Jonathan W</au><au>Falconer, David A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Solar X-ray Jets, Type-II Spicules, Granule-size Emerging Bipoles, and the Genesis of the Heliosphere</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2011-04-10</date><risdate>2011</risdate><volume>731</volume><issue>1</issue><spage>L18</spage><epage>jQuery1323917968051='48'</epage><pages>L18-jQuery1323917968051='48'</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>From Hinode observations of solar X-ray jets, Type-II spicules, and granule-size emerging bipolar magnetic fields in quiet regions and coronal holes, we advocate a scenario for powering coronal heating and the solar wind. In this scenario, Type-II spicules and Alfven waves are generated by the granule-size emerging bipoles (EBs) in the manner of the generation of X-ray jets by larger magnetic bipoles. From observations and this scenario, we estimate that Type-II spicules and their co-generated Alfven waves carry into the corona an area-average flux of mechanical energy of ~7 X 105 erg cm--2 s--1. This is enough to power the corona and solar wind in quiet regions and coronal holes, and therefore indicates that the granule-size EBs are the main engines that generate and sustain the entire heliosphere.</abstract><cop>United States</cop><pub>IOP Publishing</pub><doi>10.1088/2041-8205/731/1/L18</doi></addata></record> |
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subjects | ALFVEN WAVES ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATMOSPHERES CHROMOSPHERE ELECTROMAGNETIC RADIATION HELIOSPHERE HYDROMAGNETIC WAVES IONIZING RADIATIONS JETS MAGNETIC FIELDS RADIATIONS SOLAR ACTIVITY SOLAR ATMOSPHERE SOLAR CORONA SOLAR PROMINENCES SOLAR WIND STELLAR ACTIVITY STELLAR ATMOSPHERES STELLAR CORONAE STELLAR WINDS X RADIATION |
title | Solar X-ray Jets, Type-II Spicules, Granule-size Emerging Bipoles, and the Genesis of the Heliosphere |
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