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Title: Location of intense electromagnetic ion cyclotron (EMIC) wave events relative to the plasmapause: Van Allen Probes observations

Abstract

In this paper, we have studied the spatial location relative to the plasmapause (PP) of the most intense electromagnetic ion cyclotron (EMIC) waves observed on Van Allen Probes A and B during their first full precession in local time. Most of these waves occurred over an L range of from -1 to +2 RE relative to the PP. Very few events occurred only within 0.1 RE of the PP, and events with a width in L of < 0.2 RE occurred both inside and outside the PP. Wave occurrence was always associated with high densities of ring current ions; plasma density gradients or enhancements were associated with some events but were not dominant factors in determining the sites of wave generation. Storm main and recovery phase events in the dusk sector were often inside the PP, and dayside events during quiet times and compressions of the magnetosphere were more evenly distributed both inside and outside the PP. Superposed epoch analyses of the dependence of wave onset on solar wind dynamic pressure (Psw), the SME (SuperMAG auroral electrojet) index, and the SYM-H index showed that substorm injections and solar wind compressions were temporally closely associated with EMIC wave onset but tomore » an extent that varied with frequency band, magnetic local time, and storm phase, and location relative to the PP. Finally, the fact that increases in SME and Psw were less strongly correlated with events at the PP than with other events might suggest that the occurrence of those events was affected by the density gradient.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [2];  [2]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [5]; ORCiD logo [5]; ORCiD logo [6]; ORCiD logo [7]; ORCiD logo [8]
  1. Augsburg College, Minneapolis, MN (United States). Dept. of Physics; Univ. of Iowa, Iowa City, IA (United States). Dept. of Physics and Astronomy
  2. Augsburg College, Minneapolis, MN (United States). Dept. of Physics
  3. Univ. of New Hampshire, Durham, NH (United States). Space Science Center
  4. Dartmouth College, Hanover, NH (United States). Dept. of Physics and Astronomy
  5. Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy
  6. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  7. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
  8. The Aerospace Corporation, Los Angeles, CA (United States)
Publication Date:
Research Org.:
Augsburg College, Minneapolis, MN (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
Sponsoring Org.:
USDOE; National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
OSTI Identifier:
1402621
Report Number(s):
LA-UR-17-20105
Journal ID: ISSN 2169-9380; TRN: US1703012
Grant/Contract Number:  
AC52-06NA25396; PLR-1341493; ATM-1202267; NNX13AD65G; NAS5-01072
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Geophysical Research. Space Physics
Additional Journal Information:
Journal Volume: 122; Journal Issue: 4; Journal ID: ISSN 2169-9380
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; EMIC waves; plasmapause; magnetosphere; plasmasphere; ring current

Citation Formats

Tetrick, S. S., Engebretson, M. J., Posch, J. L., Olson, C. N., Smith, C. W., Denton, R. E., Thaller, S. A., Wygant, J. R., Reeves, G. D., MacDonald, E. A., and Fennell, J. F. Location of intense electromagnetic ion cyclotron (EMIC) wave events relative to the plasmapause: Van Allen Probes observations. United States: N. p., 2017. Web. doi:10.1002/2016JA023392.
Tetrick, S. S., Engebretson, M. J., Posch, J. L., Olson, C. N., Smith, C. W., Denton, R. E., Thaller, S. A., Wygant, J. R., Reeves, G. D., MacDonald, E. A., & Fennell, J. F. Location of intense electromagnetic ion cyclotron (EMIC) wave events relative to the plasmapause: Van Allen Probes observations. United States. https://doi.org/10.1002/2016JA023392
Tetrick, S. S., Engebretson, M. J., Posch, J. L., Olson, C. N., Smith, C. W., Denton, R. E., Thaller, S. A., Wygant, J. R., Reeves, G. D., MacDonald, E. A., and Fennell, J. F. Fri . "Location of intense electromagnetic ion cyclotron (EMIC) wave events relative to the plasmapause: Van Allen Probes observations". United States. https://doi.org/10.1002/2016JA023392. https://www.osti.gov/servlets/purl/1402621.
@article{osti_1402621,
title = {Location of intense electromagnetic ion cyclotron (EMIC) wave events relative to the plasmapause: Van Allen Probes observations},
author = {Tetrick, S. S. and Engebretson, M. J. and Posch, J. L. and Olson, C. N. and Smith, C. W. and Denton, R. E. and Thaller, S. A. and Wygant, J. R. and Reeves, G. D. and MacDonald, E. A. and Fennell, J. F.},
abstractNote = {In this paper, we have studied the spatial location relative to the plasmapause (PP) of the most intense electromagnetic ion cyclotron (EMIC) waves observed on Van Allen Probes A and B during their first full precession in local time. Most of these waves occurred over an L range of from -1 to +2 RE relative to the PP. Very few events occurred only within 0.1 RE of the PP, and events with a width in L of < 0.2 RE occurred both inside and outside the PP. Wave occurrence was always associated with high densities of ring current ions; plasma density gradients or enhancements were associated with some events but were not dominant factors in determining the sites of wave generation. Storm main and recovery phase events in the dusk sector were often inside the PP, and dayside events during quiet times and compressions of the magnetosphere were more evenly distributed both inside and outside the PP. Superposed epoch analyses of the dependence of wave onset on solar wind dynamic pressure (Psw), the SME (SuperMAG auroral electrojet) index, and the SYM-H index showed that substorm injections and solar wind compressions were temporally closely associated with EMIC wave onset but to an extent that varied with frequency band, magnetic local time, and storm phase, and location relative to the PP. Finally, the fact that increases in SME and Psw were less strongly correlated with events at the PP than with other events might suggest that the occurrence of those events was affected by the density gradient.},
doi = {10.1002/2016JA023392},
journal = {Journal of Geophysical Research. Space Physics},
number = 4,
volume = 122,
place = {United States},
year = {Fri Mar 17 00:00:00 EDT 2017},
month = {Fri Mar 17 00:00:00 EDT 2017}
}

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