Modeling solar near-relativistic electron events - Insights into solar injection and interplanetary transport conditions

Table 4:

Derived injection components at $\sim$ 80 keV.
	Spectral	Prompt injection episode				Delayed injection episode
Event	index	Onset	Duration	Injected particles		Onset	Duration	Injection rate
	$\bar{\gamma}_{\rm s}$	(UT)	(min)	(e sr^-1 MeV^-1)	%	(UT)	(h)	(e sr^-1 MeV^-1 s^-1)
May98	$3.7\pm0.1$	13:15	14.4	$5.1\times 10^{34}$	98	-	-	-
May00	$2.7\pm 0.2$	10:20	2.4	$3.6\times 10^{34}$	75	10:36	1.2	$2.5\times 10^{30}$
Jul00	$1.7\pm0.1$	10:19	10.8	$6.4\times 10^{35}$	33	10:40	2.5	$1.4\times 10^{32}$
Nov00	$1.8\pm0.1$	-	-	-	-	22:55	3.5	$3.7\times 10^{32}$
Apr01^a	$2.1\pm0.1$	13:48	9.6	$4.4\times 10^{35}$	52	14:25	3.0	$6.1\times 10^{31}$
Dec01	$2.6\pm0.1$	-	-	-	-	05:20	3.4	$7.4\times 10^{31}$
Aug02	$2.3\pm0.1$	-	-	-	-	01:15	3.0	$2.6\times 10^{31}$
Oct02^b	$3.0\pm0.4$	14:13	6.0	$3.3\times 10^{34}$	92	15:29	2.4	$3.0\times 10^{29}$
Dec02^a	$2.6\pm0.1$	21:36	13.2	$4.2\times 10^{34}$	88	23:00	1.5	$1.1\times 10^{30}$
Sep04	$2.2\pm0.1$	-	-	-	-	17:06	3.4	$1.4\times 10^{31}$
Jun05^a	$2.1\pm0.1$	20:12	9.6	$1.2\times 10^{35}$	76	21:49	0.9	$1.2\times 10^{31}$

^a The delayed injection episode is very sparse.
^b The injection episode shows two components (well correlated with two type III radio bursts). Only the first short injection episode is included in the table.

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