Bayesian inversion of the Hapke model on (4) Vesta’s avalanches and ejecta: Photometric constraints on regolith evolution

Open Access

Table 2

Posterior medians and median absolute deviations for our reference four-parameter Hapke model, organized by subregion.

	Zone	ω	$\bar{θ}$ $Mathematical equation: $\[\bar{\theta}\]$$ [°]	b	c
Cornelia	Avalanche a	0.73±0.08	49.33±7.08	0.34±0.08	0.55±0.21
	Avalanche b	0.78±0.03	51.13±3.00	0.30±0.04	0.81±0.14
	Avalanche c	0.78±0.04	48.14±3.87	0.34±0.05	0.72±0.16
	Avalanche d	0.77±0.03	50.32±2.46	0.33±0.02	0.86±0.11
	Crater floor	0.55±0.05	46.46±2.97	0.34±0.03	0.71±0.16
	Opposite side	0.35±0.02	41.06±1.69	0.30±0.02	0.86±0.11

Matronalia	Small crater	0.70±0.09	41.26±7.05	0.47±0.15	0.54±0.19
	Ejecta	0.83±0.05	40.24±3.42	0.33±0.21	0.46±0.22
	Cliff slope	0.58±0.05	12.25±9.45	0.79±0.14	0.27±0.17

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.