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• W2106202577 startingPage "44" @default.
• W2106202577 abstract "The solar wind can be categorized into three types based on its freeze-in temperature (Tfreeze-in) in the coronal source: low Tfreeze-in wind mostly from coronal holes, high Tfreeze-in wind mostly from regions outside of coronal holes, including streamers (helmet streamer and pseudostreamer), active regions, etc., and transient interplanetary coronal mass ejections (ICMEs) usually possessing the hottest Tfreeze-in. The global distribution of these three types of wind has been investigated by examining the most effective Tfreeze-in indicator, the O7 +/O6 + ratio, as measured by the Solar Wind Ion Composition Spectrometer on board the Advanced Composition Explorer (ACE) during 1998–2008 by Zhao et al. In this study, we extend the previous investigation to 2011 June, covering the unusual solar minimum between solar cycles 23 and 24 (2007–2010) and the beginning of solar cycle 24. We find that during the entire solar cycle, from the ascending phase of cycle 23 in 1998 to the ascending phase of cycle 24 in 2011, the average fractions of the low O7 +/O6 + ratio (LOR) wind, the high O7 +/O6 + ratio (HOR) wind, and ICMEs at 1 AU are 50.3%, 39.4%, and 10.3%, respectively; the contributions of the three types of wind evolve with time in very different ways. In addition, we compare the evolution of the HOR wind with two heliospheric current sheet (HCS) parameters, which indicate the latitudinal standard deviation (SD) and the slope (SL) of the HCS on the synoptic Carrington maps at 2.5 solar radii surface. We find that the fraction of HOR wind correlates with SD and SL very well (slightly better with SL than with SD), especially after 2005. This result verifies the link between the production of HOR wind and the morphology of the HCS, implying that at least one of the major sources of the HOR wind must be associated with the HCS." @default.
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• W2106202577 date "2014-09-03" @default.
• W2106202577 modified "2023-09-27" @default.
• W2106202577 title "THE EVOLUTION OF 1 AU EQUATORIAL SOLAR WIND AND ITS ASSOCIATION WITH THE MORPHOLOGY OF THE HELIOSPHERIC CURRENT SHEET FROM SOLAR CYCLES 23 TO 24" @default.
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• W2106202577 doi "https://doi.org/10.1088/0004-637x/793/1/44" @default.
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