Open Access

Table A1.

HSSs under this study. Sunward (anti-sunward) HSSs are emanated from solar coronal holes with negative (positive) magnetic polarity, and are characterized by positive (negative) IMF Bx and negative (positive) By components.

HSS Vp peak (km s−1) V p peak time (UT) HSS polarity
675 05 Jun 2016 22:39 Sunward
728 15 Jun 2016 07:59 Anti-sunward
564 24 Jun 2016 15:24 Sunward
486 03 Jul 2016 04:52 Sunward
670 09 Jul 2016 15:17 Anti-sunward
729 15 Jul 2016 03:17 Anti-sunward
646 29 Jul 2016 09:27 Sunward
713 05 Aug 2016 20:03 Anti-sunward
673 10 Aug 2016 09:22 Anti-sunward
607 24 Aug 2016 03:40 Sunward
748 03 Sep 2016 19:14 Anti-sunward
774 20 Sep 2016 11:50 Sunward
758 29 Sep 2016 06:35 Anti-sunward
781 17 Oct 2016 19:14 Sunward
793 25 Oct 2016 17:32 Anti-sunward
775 12 Nov 2016 18:58 Sunward
731 25 Nov 2016 20:03 Anti-sunward
761 10 Dec 2016 06:27 Sunward
784 23 Dec 2016 22:23 Anti-sunward
582 31 Dec 2016 20:55 Anti-sunward
773 06 Jan 2017 02:21 Sunward
648 19 Jan 2017 02:06 Anti-sunward
662 27 Jan 2017 10:50 Anti-sunward
790 31 Jan 2017 18:15 Sunward
612 19 Feb 2017 01:07 Anti-sunward
673 24 Feb 2017 05:39 Anti-sunward
760 03 Mar 2017 11:48 Sunward
719 22 Mar 2017 10:56 Anti-sunward
752 28 Mar 2017 04:25 Sunward
649 08 Apr 2017 16:16 Sunward
818 23 Apr 2017 20:57 Sunward
635 16 May 2017 06:06 Anti-sunward
764 20 May 2017 12:47 Sunward

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