Time Domain Structures and Dust in the Solar Vicinity: Parker Solar Probe Observations

F. S. Mozer, F. S. Mozer, O. V. Agapitov, S. D. Bale, S. D. Bale, S. D. Bale, S. D. Bale, J. W. Bonnell, K. Goetz, K. A. Goodrich, R. Gore, R. Gore, P. R. Harvey, P. J. Kellogg, D. Malaspina, M. Pulupa, G. Schumm

Research output: Contribution to journalArticlepeer-review

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Abstract

On 2019 April 5, while the Parker Solar Probe was at its 35 solar radius perihelion, the data set collected at 293 samples/s contained more than 10,000 examples of spiky electric-field-like structures with durations less than 200 milliseconds and amplitudes greater than 10 mV m-1. The vast majority of these events were caused by plasma turbulence. Defining dust events as those with similar, narrowly peaked, positive, and single-ended signatures resulted in finding 135 clear dust events, which, after correcting for the low detection efficiently, resulted in an estimate consistent with the 1000 dust events expected from other techniques. Defining time domain structures (TDS) as those with opposite polarity signals in the opposite antennas resulted in finding 238 clear TDS events which, after correcting for the detection efficiency, resulted in an estimated 500-1000 TDS events on this day. The TDS electric fields were bipolar, as expected for electron holes. Several events were found at times when the magnetic field was in the plane of the two measured components of the electric field such that the component of the electric field parallel to the magnetic field was measured. One example of significant parallel electric fields shows the negative potential that classified them as electron holes. Because the TDS observation rate was not uniform with time, it is likely that there were local regions below the spacecraft with field-aligned currents that generated the TDS.

Original languageEnglish (US)
Article number50
JournalAstrophysical Journal, Supplement Series
Volume246
Issue number2
DOIs
StatePublished - Feb 2020

Bibliographical note

Publisher Copyright:
© 2020. The Author(s). Published by the American Astronomical Society..

Copyright:
Copyright 2020 Elsevier B.V., All rights reserved.

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