Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27778
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Cairns, I. H. | en_US |
dc.contributor.author | Lobzin, V. V. | en_US |
dc.contributor.author | Donea, A. | en_US |
dc.contributor.author | Tingay, S. J. | en_US |
dc.contributor.author | McCauley, P. I. | en_US |
dc.contributor.author | Oberoi, D. | en_US |
dc.contributor.author | Duffin, R. T. | en_US |
dc.contributor.author | Reiner, M. J. | en_US |
dc.contributor.author | Hurley-Walker, N. | en_US |
dc.contributor.author | Kudryavtseva, N. A. | en_US |
dc.contributor.author | Melrose, D. B. | en_US |
dc.contributor.author | Harding, J. C. | en_US |
dc.contributor.author | BERNARDI, GIANNI | en_US |
dc.contributor.author | Bowman, J. D. | en_US |
dc.contributor.author | Cappallo, R. J. | en_US |
dc.contributor.author | Corey, B. E. | en_US |
dc.contributor.author | Deshpande, A. | en_US |
dc.contributor.author | Emrich, D. | en_US |
dc.contributor.author | Goeke, R. | en_US |
dc.contributor.author | Hazelton, B. J. | en_US |
dc.contributor.author | Johnston-Hollitt, M. | en_US |
dc.contributor.author | Kaplan, D. L. | en_US |
dc.contributor.author | Kasper, J. C. | en_US |
dc.contributor.author | Kratzenberg, E. | en_US |
dc.contributor.author | Lonsdale, C. J. | en_US |
dc.contributor.author | Lynch, M. J. | en_US |
dc.contributor.author | McWhirter, S. R. | en_US |
dc.contributor.author | Mitchell, D. A. | en_US |
dc.contributor.author | Morales, M. F. | en_US |
dc.contributor.author | Morgan, E. | en_US |
dc.contributor.author | Ord, S. M. | en_US |
dc.contributor.author | Prabu, T. | en_US |
dc.contributor.author | Roshi, A. | en_US |
dc.contributor.author | Shankar, N. Udaya | en_US |
dc.contributor.author | Srivani, K. S. | en_US |
dc.contributor.author | Subrahmanyan, R. | en_US |
dc.contributor.author | Wayth, R. B. | en_US |
dc.contributor.author | Waterson, M. | en_US |
dc.contributor.author | Webster, R. L. | en_US |
dc.contributor.author | Whitney, A. R. | en_US |
dc.contributor.author | Williams, A. | en_US |
dc.contributor.author | Williams, C. L. | en_US |
dc.date.accessioned | 2020-10-13T15:57:02Z | - |
dc.date.available | 2020-10-13T15:57:02Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 2045-2322 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27778 | - |
dc.description.abstract | Type III solar radio bursts are the Sun's most intense and frequent nonthermal radio emissions. They involve two critical problems in astrophysics, plasma physics, and space physics: how collective processes produce nonthermal radiation and how magnetic reconnection occurs and changes magnetic energy into kinetic energy. Here magnetic reconnection events are identified definitively in Solar Dynamics Observatory UV-EUV data, with strong upward and downward pairs of jets, current sheets, and cusp-like geometries on top of time-varying magnetic loops, and strong outflows along pairs of open magnetic field lines. Type III bursts imaged by the Murchison Widefield Array and detected by the Learmonth radiospectrograph and STEREO B spacecraft are demonstrated to be in very good temporal and spatial coincidence with specific reconnection events and with bursts of X-rays detected by the RHESSI spacecraft. The reconnection sites are low, near heights of 5-10 Mm. These images and event timings provide the long-desired direct evidence that semi-relativistic electrons energized in magnetic reconnection regions produce type III radio bursts. Not all the observed reconnection events produce X-ray events or coronal or interplanetary type III bursts; thus different special conditions exist for electrons leaving reconnection regions to produce observable radio, EUV, UV, and X-ray bursts. | en_US |
dc.language.iso | eng | en_US |
dc.title | Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1038/s41598-018-19195-3 | en_US |
dc.identifier.scopus | 2-s2.0-85041130117 | en_US |
dc.identifier.isi | 000423428300004 | en_US |
dc.identifier.url | https://www.nature.com/articles/s41598-018-19195-3 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 8 | en_US |
dc.relation.firstpage | 1676 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | SCIENTIFIC REPORTS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018NatSR...8.1676C | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 2045-2322 | - |
crisitem.journal.ance | E206229 | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0002-0916-7443 | - |
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