| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZGivnJVY/M3js3 |
| Repository | sid.inpe.br/mtc-m16@80/2006/08.03.14.12 (restricted access) |
| Last Update | 2006:08.03.14.12.51 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m16@80/2006/08.03.14.12.52 |
| Metadata Last Update | 2018:06.05.01.16.56 (UTC) administrator |
| Secondary Key | INPE-13952--PRE/9128 |
| ISSN | 0038-0938 1573-093X |
| Citation Key | TrottetCorAulYanKau:2006:34UT |
| Title | Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT  |
| Year | 2006 |
| Month | June |
| Access Date | 2024, Oct. 31 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 474 KiB |
| 2. Context | |
| Author | 1 Trottet, G. 2 Correia, Emilia 3 Aulanier, G. 4 Yan, Y. 5 Kaufmann, P. |
| Resume Identifier | 1 2 8JMKD3MGP5W/3C9JH2C |
| Group | 1 2 DAS-INPE-MCT-BR |
| Affiliation | 1 Observatoire de Paris, Section de Meudon 2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS) 3 Observatoire de Paris, Section de Meudon 4 National Astronomical Observatories, Chinese Academy of Sciences 5 CRAAM, Universidade Presbiteriana Mackenzie |
| Journal | Solar Physics |
| Volume | 236 |
| Number | 1 |
| Pages | 75-95 |
| History (UTC) | 2006-08-03 14:12:52 :: simone -> administrator :: 2018-06-05 01:16:56 :: administrator -> marciana :: 2006 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | HARD X-RAY RECONNECTING CURRENT SHEETS DOUBLE-LOOP CONFIGURATION GAMMA-RAY MAGNETIC-FIELD GYROSYNCHROTRON RADIATION TIME STRUCTURES MICROWAVE RADIO MILLIMETER |
| Abstract | This paper deals with a detailed analysis of spectral and imaging observations of the November 5, 1998 (H alpha 1B, GOES M1.5) flare obtained over a large spectral range, i.e., from hard X-rays to radiometric wavelengths. These observations allowed us to probe electron acceleration and transport over a large range of altitudes that is to say within small-scale (a few 10(3) km) and large-scale (a few 10(5) km) magnetic structures. The observations combined with potential and linear force-free magnetic field extrapolations allow us to show that: (i) Flare energy release and electron acceleration are basically driven by loop-loop interactions at two independent, low lying, null points of the active region magnetic field; (ii) < 300 keV hard X-ray-producing electrons are accelerated by a different process (probably DC field acceleration) than relativistic electrons that radiate the microwave emission; and (iii) although there is evidence that hard X-ray and decimetric/metric radio-emitting electrons are produced by the same accelerator, the present observations and analysis did not allow us to find a clear and direct magnetic connection between the hard X-ray emitting region and the radio-emitting sources in the middle corona. |
| Area | CEA |
| 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 | Electron acceleration and transport.pdf |
| User Group | administrator simone |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
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