1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34R/3TGF38E |
Repository | sid.inpe.br/mtc-m21c/2019/06.21.00.02 |
Last Update | 2019:06.21.00.02.21 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21c/2019/06.21.00.02.21 |
Metadata Last Update | 2020:06.02.12.18.25 (UTC) administrator |
DOI | 10.1029/2019GL082126 |
ISSN | 0094-8276 |
Citation Key | Echer:2019:InShPa |
Title | Interplanetary shock parameters near Jupiter's orbit |
Year | 2019 |
Access Date | 2024, May 17 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 605 KiB |
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2. Context | |
Author | Echer, Ezequiel |
Resume Identifier | 8JMKD3MGP5W/3C9JH3D |
Group | DIDGE-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | ezequie.echer@inpe.br |
Journal | Geophysical Research Letters |
Volume | 2019 |
Pages | 082126 |
Secondary Mark | A1_INTERDISCIPLINAR A1_GEOGRAFIA A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ENGENHARIAS_I A1_CIÊNCIAS_AMBIENTAIS A1_CIÊNCIAS_AGRÁRIAS_I A1_BIODIVERSIDADE A2_QUÍMICA A2_ENGENHARIAS_IV A2_ENGENHARIAS_II A2_CIÊNCIAS_BIOLÓGICAS_I B1_ASTRONOMIA_/_FÍSICA B2_ENSINO |
History (UTC) | 2019-06-21 00:02:21 :: simone -> administrator :: 2019-06-21 00:02:22 :: administrator -> simone :: 2019 2019-06-21 00:02:34 :: simone -> administrator :: 2019 2020-06-02 12:18:25 :: administrator -> simone :: 2019 |
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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 |
Abstract | Fast interplanetary shocks occurrence, their parameters, and drivers near Jupiter's orbit are determined in this paper. It was found that 70% of the fast shocks are forward (FS) and 30% are reverse (RS). Interplanetary coronal mass ejection‐driven FS occur more frequently in all solar cycle phases except in the declining phase, when corotating interaction region‐driven shocks predominate. Most of the shocks were quasi‐perpendicularly (65° to 70°) propagating relative to the ambient interplanetary magnetic field. The average shock magnetosonic Mach number is slightly higher for FS (2.6) than for RS (2.4), which in turn are stronger than shocks near 1 and 10 AU reported in previous works. This occurs because of the full development of corotating interaction region shocks and higher occurrence of strong interplanetary coronal mass ejections near 5 AU and that the magnetosonic speed at 5 AU has only 60% of its value at 1 AU. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Interplanetary shock parameters... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
data URL | http://urlib.net/ibi/8JMKD3MGP3W34R/3TGF38E |
zipped data URL | http://urlib.net/zip/8JMKD3MGP3W34R/3TGF38E |
Language | en |
Target File | Interplanetary Shock Parameters Near Jupiter's Orbit.pdf |
User Group | simone |
Visibility | shown |
Archiving Policy | denypublisher6 allowfinaldraft |
Read Permission | allow from all |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3EU29DP |
Citing Item List | sid.inpe.br/mtc-m21/2012/07.13.14.45.47 4 sid.inpe.br/bibdigital/2013/10.01.22.11 3 |
Dissemination | WEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS. |
Host Collection | urlib.net/www/2017/11.22.19.04 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url |
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7. Description control | |
e-Mail (login) | simone |
update | |
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