| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | plutao.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | J8LNKAN8RW/3C63LQL |
| Repository | dpi.inpe.br/plutao/2012/06.21.18.39 (restricted access) |
| Last Update | 2012:08.30.18.47.49 (UTC) secretaria.cpa@dir.inpe.br |
| Metadata Repository | dpi.inpe.br/plutao/2012/06.21.18.39.30 |
| Metadata Last Update | 2018:06.05.00.01.44 (UTC) administrator |
| Secondary Key | INPE--PRE/ |
| DOI | 10.1007/s11207-012-0040-7 |
| ISSN | 0038-0938 1573-093X |
| Label | lattes: 1272123236892781 5 KaufmannHSGCFSMP:2012:UnEmVa |
| Citation Key | KaufmannHSGCFSMP:2012:UnEmVa |
| Title | Unusual emissions at various energies prior to the impulsive phase of the large solar flare and coronal mass ejection of 4 november 2003  |
| Year | 2012 |
| Access Date | 2024, May 26 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 772 KiB |
| 2. Context | |
| Author | 1 Kaufmann, P. 2 Holman, G. D. 3 Su, Y. 4 Giménez de Castro, C. G. 5 Correia, Emilia 6 Fernandes, L. O. T. 7 Souza, Rodney V de 8 Marun, A. 9 Pereyra, P. |
| Resume Identifier | 1 2 3 4 5 8JMKD3MGP5W/3C9JH2C |
| Group | 1 2 3 4 5 DAS-CEA-INPE-MCTI-GOV-BR |
| Affiliation | 1 Escola de Engenharia, CRAAM, Universidade Presbiteriana Mackenzie, São Paulo, SP 01302970 2 ·National Aeronautics and Space Administration, Goddard Space Flight Center, Code 671, Greenbelt 3 Department of Physics, The Catholic University of America, Washington, DC 20064, USA 4 CRAAM, Universidade Presbiteriana Mackenzie, São Paulo, SP 01302970 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Escola de Engenharia, CRAAM, Universidade Presbiteriana Mackenzie, São Paulo, SP 01302970 7 Escola de Engenharia, CRAAM, Universidade Presbiteriana Mackenzie, São Paulo, SP 01302970 8 Complejo Astronômico El Leoncito, CONICET, San Juan, Argentina 9 ·Complejo Astronômico El Leoncito, CONICET, San Juan, Argentina |
| Author e-Mail Address | 1 2 3 4 5 ecorreia@craam.mackenzie.br |
| e-Mail Address | ecorreia@craam.mackenzie.br |
| Journal | Solar Physics |
| Volume | 279 |
| Number | 2 |
| Pages | 465-475 |
| Secondary Mark | B1_ASTRONOMIA_/_FÍSICA B1_BIOTECNOLOGIA B2_CIÊNCIA_DA_COMPUTAÇÃO B1_ENGENHARIAS_IV A1_GEOCIÊNCIAS A2_INTERDISCIPLINAR |
| History (UTC) | 2012-06-22 00:10:59 :: lattes -> administrator :: 2012 2012-07-26 23:08:23 :: administrator -> secretaria.cpa@dir.inpe.br :: 2012 2012-08-30 18:47:57 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012 2012-10-19 13:19:50 :: administrator -> secretaria.cpa@dir.inpe.br :: 2012 2013-01-20 15:35:39 :: secretaria.cpa@dir.inpe.br -> banon :: 2012 2013-01-20 15:36:35 :: banon -> administrator :: 2012 2013-01-20 15:53:10 :: administrator -> secretaria.cpa@dir.inpe.br :: 2012 2013-01-23 16:58:32 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012 2018-06-05 00:01:44 :: administrator -> marciana :: 2012 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Version Type | publisher |
| Keywords | solar flares CME submillimeter emission RHESSI X-ray emissions |
| Abstract | This article broadly reviews our knowledge of solar flares. There is a particular focus on their global properties, as opposed to the microphysics such as that needed for magnetic reconnection or particle acceleration as such. Indeed solar flares will always remain in the domain of remote sensing, so we cannot observe the microscales directly and must understand the basic physics entirely via the global properties plus theoretical inference. The global observables include the general energeticsradiation in flares and mass loss in coronal mass ejections (CMEs)and the formation of different kinds of ejection and global wave disturbance: the type II radio-burst exciter, the Moreton wave, the EIT wave, and the sunquake acoustic waves in the solar interior. Flare radiation and CME kinetic energy can have comparable magnitudes, of order 1032 erg each for an X-class event, with the bulk of the radiant energy in the visible-UV continuum. We argue that the impulsive phase of the flare dominates the energetics of all of these manifestations, and also point out that energy and momentum in this phase largely reside in the electromagnetic field, not in the observable plasma. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Unusual emissions at... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | Kaufmann-SolPhys-fulltext[1].pdf |
| User Group | administrator banon lattes secretaria.cpa@dir.inpe.br |
| Visibility | shown |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| Update Permission | not transferred |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |