Characteristics of the Heliospheric Current Sheets at the Sector Boundaries: Wind Observations from 1995–2020
Open Access
- 1 October 2021
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 920 (1), 39
- https://doi.org/10.3847/1538-4357/ac1586
Abstract
We report results of a statistical study of 1197 heliospheric current sheet (HCS) events associated with the sector boundaries observed by the Wind spacecraft between 1995 and 2020. The average property of the HCS events can be characterized as follows: (1) The width of the current sheets ranges between similar to 600 km and 1.1 x 10(6) km, with an average width of 1.06 +/- 2.37 x 10(5) km; (2) The longitude (in Geocentric Solar-Ecliptic coordinate) of the HCS normal shows a large peak at similar to 210 degrees (0 degrees sunward pointing) and a longer tail at smaller angles; (3) The latitudinal angle (inclination) of the HCS normal shows a near symmetric distribution (peak and average similar to 0 degrees); (4) The yearly occurrence rate is relatively constant (similar to 46 or 3.4 events per solar rotation), without showing a clear solar cycle dependence; (5) There are solar cycle variations in the properties of the plasma and field within the current sheets and these variations follow closely with the background solar wind plasma and field; (6) A mild (similar to 10%) proton temperature increase within the HCS, suggesting that heating of the solar wind proton can occur within the current sheet; and (7) A sudden decrease in the proton temperature anisotropy (T (parallel to)/T (perpendicular to)) toward unity within similar to 3 hr of the HCS was identified. These results suggest that on the large scale the HCS at 1 au is a relatively stable and persistent solar wind structure throughout the solar cycle. On the small scale the HCS property is probably controlled by the dynamics of the current system, which is still poorly known.Funding Information
- NASA (80HQTR19T0062)
- NASA (80HQTR18T0023)
- NASA (80HQTR20T0067)
This publication has 63 references indexed in Scilit:
- Signatures of kinetic instabilities in the solar windJournal of Geophysical Research: Space Physics, 2013
- Prevalence of extended reconnection X‐lines in the solar wind at 1 AUGeophysical Research Letters, 2009
- Observations of Magnetic Reconnection in the Turbulent High-Speed Solar WindThe Astrophysical Journal, 2007
- Evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AUGeophysical Research Letters, 2007
- Solar wind proton temperature anisotropy: Linear theory and WIND/SWE observationsGeophysical Research Letters, 2006
- Absence of energetic particle effects associated with magnetic reconnection exhausts in the solar windGeophysical Research Letters, 2005
- The heliospheric current sheetJournal of Geophysical Research, 2001
- An analytical theory of the morphology, flows, and shock compressions at corotating interaction regions in the solar windJournal of Geophysical Research, 2000
- The determination of interplanetary magnetic field polarities around sector boundaries using E > 2 keV electronsGeophysical Research Letters, 1994
- A test of source‐surface model predictions of heliospheric current sheet inclinationJournal of Geophysical Research, 1994