Experimental Determination of Ion Acoustic Wave Dispersion Relation With Interferometric Analysis
Name:
JGR Space Physics - 2021 - Vech ...
Size:
3.544Mb
Format:
PDF
Description:
Final Published Version
Author
Vech, D.Malaspina, D.M.
Cattell, C.
Schwartz, S.J.
Ergun, R.E.
Klein, K.G.
Kromyda, L.
Chasapis, A.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2021
Metadata
Show full item recordPublisher
John Wiley and Sons IncCitation
Vech, D., Malaspina, D. M., Cattell, C., Schwartz, S. J., Ergun, R. E., Klein, K. G., Kromyda, L., & Chasapis, A. (2021). Experimental Determination of Ion Acoustic Wave Dispersion Relation With Interferometric Analysis. Journal of Geophysical Research: Space Physics.Rights
Copyright © 2021 American Geophysical Union. All Rights Reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
In this paper we study electrostatic waves with time-dependent frequency features in the terrestrial foreshock. These short (0.1–0.3 s) duration waves are characterized by a significant frequency drift where the peak wave power shifts from a few hundred Hz to 2–4,000 Hz in a few hundred milliseconds. Based on the electric field data from the Magnetospheric Multiscale Mission (MMS) we have identified 46 of these wave packets. Using four spacecraft timing approach we find that these waves have a propagation direction pointing upstream. However, their plasma frame velocity is less than the solar wind speed, therefore they are eventually convected downstream toward the bow shock. We use the double-probes of MMS and present an interferometric analysis, which allows us to obtain the dispersion relation of these waves and directly compare them to theoretical ones. We show that the measured dispersion relations are in good agreement with Doppler shifted ion acoustic waves and discuss potential mechanisms related to impulsive reflected ions that may allow the growth of these waves and cause time-dependent frequency features. © 2021. American Geophysical Union. All Rights Reserved.Note
6 month embargo; first published: 27 October 2021ISSN
2169-9380Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1029/2021JA029221