Effect of the exoplanet magnetic field topology on its magnetospheric radio emission

Home

All issues

Volume 616 (August 2018)

A&A, 616 (2018) A182

Full HTML

Free Access

Table 1

Three-dimensional view of a simulation setup with northward IMF orientation: density distribution (color scale), exoplanet magnetic field lines (red lines) and IMF (pink lines).

Model	R_in	R_out	R_cr	L(10⁶ m)	R_m	η (10⁸ m² s⁻¹)	ν (10⁸ m² s⁻¹)
B250	0.6	16	1.0	2.44	1800	1.37	0.30
B1000	0.8	30	1.4	4.30	1020	2.42	0.42
B6000	2.4	75	2.8	36.59	120	25.81	5.47
Q02	2.0	65	2.5	28.58	150	16.06	4.10
Q04	1.5	50	2.0	17.82	250	10.01	1.67

Notes. Model inner boundary (Col. 2), outer boundary (Col. 3), soft coupling region (Col. 4), characteristic length (Col. 5), numerical magnetic Reynolds number (Col. 6.), and numerical magnetic diffusivity (Col. 7).

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.