Revisiting empirical solar energetic particle scaling relations - II. Coronal mass ejections

Open Access

Table 2.

Upper limit CME speeds (V_CME, upper, [km/s]) for the SEP event on AD774/775 and GLE05 derived in this work (i.e., from Eq. (1) and Eq. (6)), while Eq. (5) provides the V_CME for each event.

	AD774/775	GLE05	Fig. 3
Equation	CME speed – V_CME		line
	(km/s)

Eq. (1)	7602 $_{6773}^{8134}$ $_{6773}^{8134}$	4881 $_{4348}^{5222}$ $_{4348}^{5222}$	Dashed
Eq. (6)	5860 $_{5377}^{6162}$ $_{5377}^{6162}$	4214 $_{3867}^{4431}$ $_{3867}^{4431}$	Red

Eq. (5)	3706 $_{3322}^{3951}$ $_{3322}^{3951}$	2435 $_{2182}^{2596}$ $_{2182}^{2596}$	Blue

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