Connection-angle dependence of proton anisotropy in ground-level enhancement events

Open Access

Table 1.

Relevant information for the ten GLE events analyzed in this study.

#	Event	Flare	Flare	CME	Solar-wind	Conn.	Bibliographic source
GLE	date	location	class	speed	state at onset	angle	for used NM data
45	1989 Oct 24	S30W57	X5.7	1497	Disturbed^†	24.5	Mishev et al. (2023)
59	2000 Jul 14	N22W07	X5.7	2061	Inside ICME^a	36.2	Mishev & Usoskin (2016)
60	2001 Apr 15	S20W85	X14.4	1199^*	Inside ICME^a	41.5	Larsen & Mishev (2023)
65	2003 Oct 28	S16E08	X17	3128	Trail of MC^a	42.5	Mishev et al. (2024)
66	2003 Oct 29	S17N09	X10	2628	Trail of MC^a	29.6	Mishev et al. (2024)
67	2003 Nov 2	S14W56	X8.3	2733	Trail of ICME^a	21.3	Mishev et al. (2021a)
70	2006 Dec 13	S06W23	X3.4	2184	Undisturbed^a	12.5	Mishev & Usoskin (2016)
71	2012 May 17	N11W76	M5.1	1596	Inside MC^a	16.9	Mishev et al. (2021b)
72	2017 Sep 10	S09W92	X8.2	3163	Trail of ICME^b	43.7	Mishev & Usoskin (2018)
73	2021 Oct 28	S28W01	X1.0	1816	Undisturbed	77.7	Mishev et al. (2022)

Notes. ^aRouillard et al. (2016). ^bBruno et al. (2019). ^†Uncertain (no data available). ^*Partial halo CME; projected speed.

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