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Outstanding questions in magnetospheric plasma physics: The pollenzo view
| Indexado |
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| DOI | 10.1016/J.JASTP.2020.105377 | ||||
| Año | 2020 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Based on discussions held at a workshop in Bra-Pollenzo, Italy, this paper elaborates upon 19 outstanding questions of plasma physics in the Earth's magnetosphere. The questions are grouped according to (a) driving processes, (b) radiation belt and ring current issues, (c) auroral physics, (d) internal plasma processes, and (e) magnetosphere-ionosphere mapping issues. Future needs for magnetospheric plasma physics (measurements, techniques, simulations, theories, studies) are outlined.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Borovsky, Joseph E. | Hombre |
Space Science Institute - Estados Unidos
Space Sci Inst - Estados Unidos |
| 2 | Delzanno, Gian Luca | Hombre |
Los Alamos National Laboratory Theoretical Division - Estados Unidos
Los Alamos Natl Lab - Estados Unidos |
| 3 | Valdivia, Juan Alejandro | Hombre |
Universidad de Chile - Chile
|
| 4 | MOYA-FUENTES, PABLO SEBASTIAN | Hombre |
Los Alamos National Laboratory Theoretical Division - Estados Unidos
Universidad de Chile - Chile |
| 5 | STEPANOVA-SSA, MARINA VLADIMIROVNA | Mujer |
Universidad de Santiago de Chile - Chile
|
| 6 | Birn, Joachim | Hombre |
Space Science Institute - Estados Unidos
Space Sci Inst - Estados Unidos |
| 7 | Blum, Lauren W. | Mujer |
NASA Goddard Space Flight Center - Estados Unidos
NASA - Estados Unidos |
| 8 | Lotko, William | Hombre |
The Earth and Sun Systems Laboratory - Estados Unidos
Natl Ctr Atmospher Res - Estados Unidos |
| 9 | Hesse, Michael | Hombre |
Universitetet i Bergen - Noruega
Southwest Research Institute - Estados Unidos Univ Bergen - Noruega Southwest Res Inst - Estados Unidos |
| Fuente |
|---|
| FONDECYT |
| National Science Foundation |
| AFOSR |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| NSF |
| Air Force Office of Scientific Research |
| U.S. Department of Energy |
| NASA |
| National Aeronautics and Space Administration |
| Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| National Nuclear Security Administration |
| Los Alamos National Laboratory |
| U.S. Department of Energy (DOE) |
| University of Bergen |
| NASA Heliophysics Guest Investigator Program |
| Laboratory Directed Research and Development |
| ANID |
| Universitetet i Bergen |
| NSF GEM Program |
| NSF SHINE program |
| Laboratory Directed Research and Development program at Los Alamos National Laboratory (LANL) |
| NASA Heliophysics LWS TRT program |
| ANID Chile through FONDECyT Grant |
| Tommaso Alberti |
| Elizaveta Antonova |
| Agradecimiento |
|---|
| The authors thank Tommaso Alberti, Elizaveta Antonova, Jacob Bortnik, Lunjin Chen, Enrico Camporeale, Seth Claudepierre, Giuseppe Consolini, Greg Cunningham, Mick Denton, Reiner Friedel, Steve Fuselier, Marty Goldman, Jesper Gjerloev, Matina Gkioulidou, Melvyn Goldstein, Gerhard Haerendel, Rod Heelis, Mike Henderson, Mary Hudson, Linda Hunt, Raluca Ilie, Maria Elena Innocenti, Therese Moretto Jorgensen, Shri Kanekal, Andreas Keiling, Wayne Keith, Larry Kepko, Craig Kletzing, Giovanni Lapenta, Mike Liemohn, Larry Lyons, Stefano Markidis, Victor Mu?os, Antonius Otto, Slava Pilipenko, Geoff Reeves, Jean-Francois Ripoll, Vadim Roytershteyn, Andrei Runov, Drew Turner, Maria Usanova, Brian Walsh, Lynn Wilson III, Eftyhia Zesta, Hui Zhang, Qiugang Zong for their contributions to the discussions in Bra-Pollenzo. JEB was supported by NASA Heliophysics LWS TRT program via grant NNX14AN90G, by the NSF GEM Program via award AGS-1502947, by the NASA Heliophysics Guest Investigator Program via grant NNX17AB71G, and by the NSF SHINE program via award AGS-1723416. GLD was supported by the Laboratory Directed Research and Development program at Los Alamos National Laboratory (LANL) under projects 20200276ER and 20200073DR. LANL is operated by Triad National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy (DOE) (Contract No. 89233218CNA000001). JAV thanks the support of Fondecyt Grant 1190703. PSM is grateful for the support of ANID Chile through FONDECyT Grant No. 1191351. MS acknowledges the support of AFOSR No. FA9550-19-1-0384. JB supported by NASA grants 80NSSC18K1452 and 80NSSK0834, and NSF grant 1602655. LB acknowledges support from the NASA Heliophysics Guest Investigator program, Grants 17-HGIMAG17_2?0022 and 80NSSC17K0579. MH was supported by the University of Bergen. |
| The authors thank Tommaso Alberti, Elizaveta Antonova, Jacob Bortnik, Lunjin Chen, Enrico Camporeale, Seth Claudepierre, Giuseppe Consolini, Greg Cunningham, Mick Denton, Reiner Friedel, Steve Fuselier, Marty Goldman, Jesper Gjerloev, Matina Gkioulidou, Melvyn Goldstein, Gerhard Haerendel, Rod Heelis, Mike Henderson, Mary Hudson, Linda Hunt, Raluca Ilie, Maria Elena Innocenti, Therese Moretto Jorgensen, Shri Kanekal, Andreas Keiling, Wayne Keith, Larry Kepko, Craig Kletzing, Giovanni Lapenta, Mike Liemohn,, Larry Lyons, Stefano Markidis, Victor Mu~nos, Antonius Otto, Slava Pilipenko, Geoff Reeves, Jean-Francois Ripoll, Vadim Roytershteyn, Andrei Runov, Drew Turner, Maria Usanova, Brian Walsh, Lynn Wilson III, Eftyhia Zesta, Hui Zhang, Qiugang Zong for their contributions to the discussions in BraPollenzo. JEB was supported by NASA Heliophysics LWS TRT program via grant NNX14AN90G, by the NSF GEM Program via award AGS-1502947, by the NASA Heliophysics Guest Investigator Program via grant NNX17AB71G, and by the NSF SHINE program via award AGS-1723416. GLD was supported by the Laboratory Directed Research and Development program at Los Alamos National Laboratory (LANL) under projects 20200276ER and 20200073DR. LANL is operated by Triad National Security, LLC, for the National Nuclear Security Administration of U.S. Department of Energy (DOE) (Contract No. 89233218CNA000001). JAV thanks the support of Fondecyt Grant 1190703. PSM is grateful for the support of ANID Chile through FONDECyT Grant No. 1191351. MS acknowledges the support of AFOSR No. FA9550-19-1-0384. JB supported by NASA grants 80NSSC18K1452 and 80NSSK0834, and NSF grant 1602655. LB acknowledges support from the NASA Heliophysics Guest Investigator program, Grants 17-HGIMAG17_2-0022 and 80NSSC17K0579. MH was supported by the University of Bergen. |
