1. Identity statement | |
Reference Type | Conference Paper (Conference Proceedings) |
Site | mtc-m21d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34T/4878MFH |
Repository | sid.inpe.br/mtc-m21d/2022/12.13.19.19 |
Metadata Repository | sid.inpe.br/mtc-m21d/2022/12.13.19.19.29 |
Metadata Last Update | 2023:01.03.16.46.27 (UTC) administrator |
Secondary Key | INPE--PRE/ |
Citation Key | KepoNSTWDRBCHLPDPD:2022:NeInGe |
Title | On the need for an International Geospace Systems Program (IGSP) |
Year | 2022 |
Access Date | 2024, May 14 |
Secondary Type | PRE CI |
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2. Context | |
Author | 1 Kepo, Larry 2 Nakamura, Rumi 3 Saito, Yoshifumi 4 Taylor, Matt 5 Wang, Chi 6 Donovan, Eric 7 Rae, Jonathan 8 Blanco-Cano, Xochitl 9 Chakrabarty, Dibyendu 10 Hwang, Junga 11 Lavraud, Benoit 12 Petrukovich, Anatoli A. 13 Denardini, Clezio Marcos 14 Palmroth, Minna 15 Daglis, Ioannis A. |
Group | 1 2 3 4 5 6 7 8 9 10 11 12 13 DICEP-CGCE-INPE-MCTI-GOV-BR |
Affiliation | 1 NASA Goddard Space Flight Center 2 Space Research Institute 3 JAXA Japan Aerospace Exploration Agency 4 European Space Agency 5 CSSAR, CAS 6 University of Calgary 7 University College London 8 UNAM 9 Physical Research Laboratory 10 KAIST Korea Advanced Institute of Science and Technology 11 IRAP 12 Space Research Institute RAS 13 Instituto Nacional de Pesquisas Espaciais (INPE) 14 Finnish Meteorological Institute 15 National and Kapodistrian University of Athens |
Author e-Mail Address | 1 2 3 4 5 6 7 8 9 10 11 12 13 clezio.denardin@inpe.br |
Conference Name | AGU Fall Meeting |
Conference Location | Chicago, IL |
Date | 12-16 Dec. 2022 |
Publisher | AGU |
History (UTC) | 2022-12-13 19:19:29 :: simone -> administrator :: 2023-01-03 16:46:27 :: administrator -> simone :: 2022 |
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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 |
Abstract | Earths magnetosphere is vast, and too large to be studied by any single space agency or mission in any comprehensive manner. ISTP, although revolutionary for its time, provided only a low-fidelity picture of how the magnetosphere as a whole responds to the unceasing solar wind that continuously buffets it. We have learned from ISTP and the missions that followed that the magnetosphere acts as a System of Systems. Each magnetospheric system the magnetotail, inner magnetosphere (itself a system of systems with plasmasphere, ring current, and radiation belts), magnetopause, magnetosheath, and ionosphere-thermosphere-mesosphere (another system of systems) has its own dynamics and characteristics that can be, and have been, studied separately. Yet, there is a clear need to study the way the systems within the larger geospace system interact with each other: for example, how magnetotail dynamics lead to ring current enhancements; how ionospheric outflow modifies magnetospheric response; how meso- and macro-scale reconnection and boundary waves regulates the transfer of energy from the solar wind and foreshock/bow shock into the magnetosphere. This cross-scale, system science currently relies on ad-hoc and chance alignments of largely uncoordinated missions. Therefore, while great progress has been made on targeted mission science objectives, a broader, cohesive, and intentional program to study the entire systems of systems has potential to revolutionize our understanding in ways not possible today. With the revelation that mesoscale dynamics (~1-3 RE in scale) are both ubiquitous and central to magnetospheric dynamics, the science questions are dictating that we need a large undertaking to answer these questions. Such an undertaking would involve multiple constellations of spacecraft in key regions to resolve the missing middle of the mesoscales, combined with remote imaging measurements, ground-based measurements, and advanced numerical modeling, all coordinated and working in concert to study Geospace holistically, as a system, at the scale sizes that we now know are driving the overall dynamics. It would move beyond the limited view afforded by ISTP and the current ad hoc heliophysics system observatory to provide critically needed understanding of our dynamic space environment. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > On the need... |
doc Directory Content | there are no files |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
User Group | simone |
Visibility | shown |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/46KTFK8 |
Host Collection | urlib.net/www/2021/06.04.03.40 |
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6. Notes | |
Empty Fields | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume |
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7. Description control | |
e-Mail (login) | simone |
update | |
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