The effect of tidal locking on the magnetospheric and atmospheric evolution of ``Hot Jupiters''

By J. Grießmeier, A. Stadelmann, T. Penz, H. Lammer, F. Selsis, I. Ribas, E. Guinan, U. Motschmann, H. Biernat, W. Weiss. 2004

182 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The Sun in Time: Activity and Environment (2007, background): “85 7.2.10 Hot Jupiters: Mass Evolution by Evaporation?”
Stellar winds on the main-sequence - II. The evolution of rotation and winds (2015, background): “More recent models for the evolution of the solar wind have concentrated on the influences of these mechanisms (Grießmeier et al. 2004; Holzwarth & Jardine 2007; Sterenborg et al. 2011; Suzuki et al. 2013).”
Tidal obliquity evolution of potentially habitable planets (2011, background): “A widely spread misapprehension is that a tidally locked body permanently turns one side to its host (e.g. inNeron de Surgy & Laskar 1997; Joshi et al. 1997; Grießmeier et al. 2004; Khodachenko et al. 2007).”
Predicting low-frequency radio fluxes of known extrasolar planets (2007, background): “The different scaling laws are compared, e.g., by Farrell et al. (1999)1, Grießmeier et al. (2004) and Grießmeier (2006).”
What makes a planet habitable? (2009, methodology): “Based on the formulas given by Grießmeier et al. (2005) one can calculate the”
Magnetic energy fluxes in sub-Alfvénic planet star and moon planet interactions (2013, background): “Grießmeier et al. (2004, 2005, 2007) investigate SPI with particular emphasis on the radio emission from extrasolar planets and their detectability from Earth depending on various parameters such as stellar wind properties.”