Interhemispheric Observations of ULF Waves Caused by Foreshock Transients Under Quiet Solar Wind Conditions

Noh, Sung Jun; Kim, Hyomin; Ozturk, Dogacan; Kuzichev, Ilya; Xu, Zhonghua; Zhang, Hui; Vu, Andrew; Liu, Terry; Weygand, James M.; Hartinger, Michael D.; Shi, Xueling; Engebretson, Mark; Gerrard, Andrew; Kim, Eun‐Hwa; Lessard, Marc; Russell, Christopher T.

doi:10.1029/2023JA031596

Title: Interhemispheric Observations of ULF Waves Caused by Foreshock Transients Under Quiet Solar Wind Conditions

Journal Article · Sat Sep 09 00:00:00 EDT 2023 · Journal of Geophysical Research. Space Physics

DOI:https://doi.org/10.1029/2023JA031596· OSTI ID:1999275

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Los Alamos National Laboratory NM Los Alamos USA, New Jersey Institute of Technology Newark NJ USA
New Jersey Institute of Technology Newark NJ USA
University of Alaska Fairbanks AK Fairbanks USA
Virginia Tech VA Blacksburg USA
Shandong University Weihai China
University of California, Los Angeles CA Los Angeles USA
Space Science Institute CO Boulder USA
Augsburg University MN Minneapolis USA
Princeton Plasma Physics Laboratory Princeton University NJ Princeton USA
University of New Hampshire NH Durham USA

Foreshock transient (FT) events are frequently observed phenomena that are generated by discontinuities in the solar wind. These transient events are known to trigger global-scale magnetic field perturbations (e.g., ULF waves). We report a series of FT events observed by the Magnetospheric Multiscale mission in the upstream bow shock region under quiet solar wind conditions. During the event, ground magnetometers observed significant Pc1 wave activity as well as magnetic impulse events in both hemispheres. Ground Pc1 wave observations show ~8 min time delay (with some time differences) from each FT event which is observed at the bow shock. We also find that the ground Pc1 waves are observed earlier in the northern hemisphere compared to the southern hemisphere. The observation time difference between the hemispheres implies that the source region of the wave is the off-equatorial region.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)

Sponsoring Organization:: USDOE Laboratory Directed Research and Development (LDRD) Program; USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA); National Science Foundation (NSF)

Grant/Contract Number:: 89233218CNA000001; 20210528CR; AGS-2027210; 80GSFC17C0018; 80NSSC18K1220; 80NSSC18K0570; OPP-1643700; 80NSSC21K0132; OPP-1744861, NSF-1602560; AGS-2133837; AC02-09CH11466

OSTI ID:: 1999275

Alternate ID(s):: OSTI ID: 2000930; OSTI ID: 2004948; OSTI ID: 2006525

Report Number(s):: LA-UR-23-23287; e2023JA031596

Journal Information:: Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics Vol. 128 Journal Issue: 9; ISSN 2169-9380

Publisher:: American Geophysical Union (AGU)Copyright Statement

Country of Publication:: United States

Language:: English

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