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Title: A multispacecraft event study of Pc5 ultralow-frequency waves in the magnetosphere and their external drivers

Abstract

We investigate a quiet time event of magnetospheric Pc5 ultralow-frequency (ULF) waves and their likely external drivers using multiple spacecraft observations. Enhancements of electric and magnetic field perturbations in two narrow frequency bands, 1.5–2 mHz and 3.5–4 mHz, were observed over a large radial distance range from r ~ 5 to 11 RE. During the first half of this event, perturbations were mainly observed in the transverse components and only in the 3.5–4 mHz band. In comparison, enhancements were stronger during the second half in both transverse and compressional components and in both frequency bands. No indication of field line resonances was found for these magnetic field perturbations. Perturbations in these two bands were also observed in the magnetosheath, but not in the solar wind dynamic pressure perturbations. For the first interval, good correlations between the flow perturbations in the magnetosphere and magnetosheath and an indirect signature for Kelvin-Helmholtz (K-H) vortices suggest K-H surface waves as the driver. For the second interval, good correlations are found between the magnetosheath dynamic pressure perturbations, magnetopause deformation, and magnetospheric waves, all in good correspondence to interplanetary magnetic field (IMF) discontinuities. The characteristics of these perturbations can be explained by being driven by foreshockmore » perturbations resulting from these IMF discontinuities. This event shows that even during quiet periods, K-H-unstable magnetopause and ion foreshock perturbations can combine to create a highly dynamic magnetospheric ULF wave environment« less

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3];  [1]; ORCiD logo [4]; ORCiD logo [4]; ORCiD logo [5]; ORCiD logo [6]; ORCiD logo [7]; ORCiD logo [8]
+ Show Author Affiliations
  1. Univ. of California, Los Angeles, CA (United States)
  2. Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States)
  3. Tokyo Inst. of Technology (Japan)
  4. Univ. of Minnesota, Minneapolis, MN (United States)
  5. Univ. of Iowa, Iowa City, IA (United States)
  6. Los Alamos National Lab. (LANL), Los Alamos, NM (United States); New Mexico Consortium, Los Alamos, NM (United States)
  7. Aerospace Corporation, El Segundo, CA (United States)
  8. Univ. of New Hampshire, Durham, NH (United States)
Publication Date:
Research Org.:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
National Aeronautics and Space Administration (NASA); USDOE
OSTI Identifier:
1402637
Report Number(s):
LA-UR-17-24826
Journal ID: ISSN 2169-9380; TRN: US1703016
Grant/Contract Number:  
AC52-06NA25396
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Geophysical Research. Space Physics
Additional Journal Information:
Journal Volume: 122; Journal Issue: 5; Journal ID: ISSN 2169-9380
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Heliospheric and Magnetospheric Physics

Citation Formats

Wang, Chih-Ping, Thorne, Richard, Liu, Terry Z., Hartinger, Michael D., Nagai, Tsugunobu, Angelopoulos, Vassilis, Wygant, John R., Breneman, Aaron, Kletzing, Craig, Reeves, Geoffrey D., Claudepierre, Seth G., and Spence, Harlan E. A multispacecraft event study of Pc5 ultralow-frequency waves in the magnetosphere and their external drivers. United States: N. p., 2017. Web. doi:10.1002/2016JA023610.
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Wang, Chih-Ping, Thorne, Richard, Liu, Terry Z., Hartinger, Michael D., Nagai, Tsugunobu, Angelopoulos, Vassilis, Wygant, John R., Breneman, Aaron, Kletzing, Craig, Reeves, Geoffrey D., Claudepierre, Seth G., & Spence, Harlan E. A multispacecraft event study of Pc5 ultralow-frequency waves in the magnetosphere and their external drivers. United States. https://doi.org/10.1002/2016JA023610
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Wang, Chih-Ping, Thorne, Richard, Liu, Terry Z., Hartinger, Michael D., Nagai, Tsugunobu, Angelopoulos, Vassilis, Wygant, John R., Breneman, Aaron, Kletzing, Craig, Reeves, Geoffrey D., Claudepierre, Seth G., and Spence, Harlan E. Tue . "A multispacecraft event study of Pc5 ultralow-frequency waves in the magnetosphere and their external drivers". United States. https://doi.org/10.1002/2016JA023610. https://www.osti.gov/servlets/purl/1402637.
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@article{osti_1402637,
title = {A multispacecraft event study of Pc5 ultralow-frequency waves in the magnetosphere and their external drivers},
author = {Wang, Chih-Ping and Thorne, Richard and Liu, Terry Z. and Hartinger, Michael D. and Nagai, Tsugunobu and Angelopoulos, Vassilis and Wygant, John R. and Breneman, Aaron and Kletzing, Craig and Reeves, Geoffrey D. and Claudepierre, Seth G. and Spence, Harlan E.},
abstractNote = {We investigate a quiet time event of magnetospheric Pc5 ultralow-frequency (ULF) waves and their likely external drivers using multiple spacecraft observations. Enhancements of electric and magnetic field perturbations in two narrow frequency bands, 1.5–2 mHz and 3.5–4 mHz, were observed over a large radial distance range from r ~ 5 to 11 RE. During the first half of this event, perturbations were mainly observed in the transverse components and only in the 3.5–4 mHz band. In comparison, enhancements were stronger during the second half in both transverse and compressional components and in both frequency bands. No indication of field line resonances was found for these magnetic field perturbations. Perturbations in these two bands were also observed in the magnetosheath, but not in the solar wind dynamic pressure perturbations. For the first interval, good correlations between the flow perturbations in the magnetosphere and magnetosheath and an indirect signature for Kelvin-Helmholtz (K-H) vortices suggest K-H surface waves as the driver. For the second interval, good correlations are found between the magnetosheath dynamic pressure perturbations, magnetopause deformation, and magnetospheric waves, all in good correspondence to interplanetary magnetic field (IMF) discontinuities. The characteristics of these perturbations can be explained by being driven by foreshock perturbations resulting from these IMF discontinuities. This event shows that even during quiet periods, K-H-unstable magnetopause and ion foreshock perturbations can combine to create a highly dynamic magnetospheric ULF wave environment},
doi = {10.1002/2016JA023610},
journal = {Journal of Geophysical Research. Space Physics},
number = 5,
volume = 122,
place = {United States},
year = {Tue May 09 00:00:00 EDT 2017},
month = {Tue May 09 00:00:00 EDT 2017}
}
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    Works referencing / citing this record:

    Multispacecraft Observations of Tailward Propagation of Transient Foreshock Perturbations to Midtail Magnetosheath
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