On the Star-Magnetosphere Interaction of Close-in Exoplanets

By W. Ip, A. Kopp, Juei-Hwa Hu. 2004

144 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/439f931aae91ca1bbe66cebf51e2224c10612380

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In Astronomy and Astrophysics

1. E. Shkolnik
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Citations in the corpus

• Magnetic energy fluxes in sub-Alfvénic planet star and moon planet interactions (2013, background): “This effect has been noted by Ip et al. (2004) and Kopp et al. (2011), but not investigated quantitatively.”
• Hot Jupiters and Hot Spots: The Short- and Long-Term Chromospheric Activity on Stars with Giant Planets (2004, background): “…between the location of the heating spot in the chromosphere and the position of the hot jupiter might be caused by the entangled or rotationally spiraled magnetic fields connecting directly between the hot jupiter and the star (Rubenstein & Schaefer 2000, Saar et al. 2004, Ip et al. 2004).”
• The On/Off Nature of Star-Planet Interactions (2007, background): “…interaction proposes that the planet induces reconnec- tion events as it travels through the large stellar magnetic loops (Cuntz et al. 2000, Ip et al. 2004), implying that the resulting activity should depend on the star’s magnetic field, the planet’s magnetic field and the orbital…”
• Plasma interactions of exoplanets with their parent star and associated radio emissions (2006, methodology): “Ip et al. (2004) have studied via MHD simulations the shape of magnetospheric (obstacle) field lines as a function of the orientation of the magnetic field embedded in the plasma flow.”
• SUPERFLARES ON SOLAR-TYPE STARS OBSERVED WITH KEPLER. I. STATISTICAL PROPERTIES OF SUPERFLARES (2013, background): “It has also been proposed that hot Jupiters have an important effect on stellar magnetic activity (Rubenstein & Schaefer 2000; Cuntz et al. 2000; Ip et al. 2004) and that superflares occur only on G-type dwarfs with hot Jupiters.”
• Can Superflares Occur on Our Sun (2012, background): “Ip, Kopp, and Hu (2004) studied the star–hot Jupiter interaction, and found that it leads to energy release via reconnection, which is comparable to that of typical solar flares.”