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

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Volume 507 / No 2 (November IV 2009)

A&A, 507 2 (2009) 981-993

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Table 3:

Goodness-of-fit estimator $\zeta$ and radial mean free path obtained for each scattering case: (1) isotropic; (2) $\mu$ -dependent with $\epsilon =0.10$ ; and (3) $\mu$ -dependent with $\epsilon =0.01$ , and the scattering case giving the lowest $\zeta$ .
	$\zeta \times 10$			$\lambda_{\rm r}$ (AU)			Scattering
Event	(1)	(2)	(3)	(1)	(2)	(3)	case
May98	3.6	3.4	3.3	0.08	0.08	0.08	$\mu$ -dep. $\epsilon =0.01$
May00	9.1	7.2	6.9	0.80	0.80	0.90	$\mu$ -dep. $\epsilon =0.01$
Jul00	0.35	0.34	0.36	0.13	0.13	0.10	$\mu$ -dep. $\epsilon =0.10$
Nov00	9.5	10.1	10.2	0.20	0.16	0.16	isotropic
Apr01	0.84	0.62	0.66	0.08	0.08	0.06	$\mu$ -dep. $\epsilon =0.10$
Dec01	1.5	1.4	1.3	0.16	0.20	0.24	$\mu$ -dep. $\epsilon =0.01$
Aug02	2.5	2.7	3.0	0.20	0.20	0.20	isotropic
Oct02	5.0	4.2	4.0	0.80	0.90	0.90	$\mu$ -dep. $\epsilon =0.01$
Dec02	4.1	3.3	3.1	0.13	0.13	0.13	$\mu$ -dep. $\epsilon =0.01$
Sep04	1.6	1.9	2.1	0.16	0.16	0.13	isotropic
Jun05	2.0	1.8	1.9	0.08	0.08	0.08	$\mu$ -dep. $\epsilon =0.10$

Source LaTeX | All tables | In the text

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