机译:New view on exoplanet transits Transit of Venus described using three-dimensional solar atmosphere STAGGER-grid simulations
Univ Nice Sophia Antipolis, Observ Cote Azur, CNRS, Lab Lagrange,UMR 7293, F-06189 Nice, France;
Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark;
Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia;
planet-star interactions; Sun: granulation; techniques: photometric; stars: atmospheres; hydrodynamics; radiative transfer;