TY - JOUR
T1 - Interhemispheric Observations of ULF Waves Caused by Foreshock Transients Under Quiet Solar Wind Conditions
AU - Noh, Sung Jun
AU - Kim, Hyomin
AU - Ozturk, Dogacan
AU - Kuzichev, Ilya
AU - Xu, Zhonghua
AU - Zhang, Hui
AU - Vu, Andrew
AU - Liu, Terry
AU - Weygand, James M.
AU - Hartinger, Michael D.
AU - Shi, Xueling
AU - Engebretson, Mark
AU - Gerrard, Andrew
AU - Kim, Eun Hwa
AU - Lessard, Marc
AU - Russell, Christopher T.
N1 - Publisher Copyright:
©2023. The Authors.
PY - 2023/9
Y1 - 2023/9
N2 - 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.
AB - 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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U2 - 10.1029/2023JA031596
DO - 10.1029/2023JA031596
M3 - Article
AN - SCOPUS:85170524353
SN - 2169-9380
VL - 128
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 9
M1 - e2023JA031596
ER -