Skip navigation
Skip navigation

New view on exoplanet transits: Transit of Venus described using three-dimensional solar atmosphere STAGGER-grid simulations

Pere, C; Chiavassa, A; Faurobert, M; Ricort, G; Tanga, P; Magic, Z; Collet, Remo; Asplund, Martin


Context. An important benchmark for current observational techniques and theoretical modeling of exoplanet atmospheres is the transit of Venus (ToV). Stellar activity and, in particular, convection-related surface structures, potentially cause fluctuations that can affect the transit light curves. Surface convection simulations can help interpreting the ToV as well as other transits outside our solar system. Aims. We used the realistic three-dimensional (3D) radiative hydrodynamical (RHD)...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201425256
Access Rights: Open Access


File Description SizeFormat Image
01_Pere_New_view_on_exoplanet_2015.pdf3.19 MBAdobe PDF

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  17 November 2022/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator