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\field{extradatescope}{labelyear}
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\field{eid}{123}
\field{eprintclass}{astro-ph.IM}
\field{eprinttype}{arXiv}
\field{journaltitle}{aj}
\field{month}{9}
\field{number}{3}
\field{title}{{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}}
\field{volume}{156}
\field{year}{2018}
\field{pages}{123}
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\verb{eprint}
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\keyw{methods: data analysis,methods: miscellaneous,methods: statistical,reference systems,Astrophysics - Instrumentation and Methods for Astrophysics}
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\field{abstract}{Numerical simulations using a resistive MHD code are performed in order to investigate the interaction of the magnetospheres of hot Jupiters (or close-in extrasolar giant planets) with the central host stars. Because of the sub-Alfvénic nature of the stellar wind outflow at the orbital positions of these close-in exoplanets, no bow shock would form. When the orientation of the stellar coronal magnetic field is favorable to strong coupling with magnetic reconnection, the power (~1027 ergs s-1) generated could reach the level of a typical solar flare. As a particular type of star-planet atmospheric interaction, as investigated by Cuntz, Saar, & Musielak, magnetospheric interaction as studied in this Letter could lead to extensive energy injection into the auroral zones of the exoplanets, producing massive atmospheric escape process as recently detected.}
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giveni={M\bibinithyphendelim D\bibinitperiod}}}%
}
\strng{namehash}{7cf8eaf74a2659f76a70a943f2d3282a}
\strng{fullhash}{eb0c7f8a57ceed7bb9057f5463862324}
\strng{fullhashraw}{eb0c7f8a57ceed7bb9057f5463862324}
\strng{bibnamehash}{eb0c7f8a57ceed7bb9057f5463862324}
\strng{authorbibnamehash}{eb0c7f8a57ceed7bb9057f5463862324}
\strng{authornamehash}{7cf8eaf74a2659f76a70a943f2d3282a}
\strng{authorfullhash}{eb0c7f8a57ceed7bb9057f5463862324}
\strng{authorfullhashraw}{eb0c7f8a57ceed7bb9057f5463862324}
\field{sortinit}{Z}
\field{sortinithash}{96892c0b0a36bb8557c40c49813d48b3}
\field{extradatescope}{labelyear}
\field{labeldatesource}{}
\field{labelnamesource}{author}
\field{labeltitlesource}{title}
\field{eid}{747}
\field{eprintclass}{astro-ph.SR}
\field{eprinttype}{arXiv}
\field{journaltitle}{Nature Communications}
\field{month}{3}
\field{title}{{Observation of an evolving magnetic flux rope before and during a solar eruption}}
\field{volume}{3}
\field{year}{2012}
\field{pages}{747}
\range{pages}{1}
\verb{doi}
\verb 10.1038/ncomms1753
\endverb
\verb{eprint}
\verb 1203.4859
\endverb
\keyw{Astrophysics - Solar and Stellar Astrophysics,Astrophysics - Earth and Planetary Astrophysics,Astrophysics - High Energy Astrophysical Phenomena,Physics - Plasma Physics}
\endentry
\enddatalist
\endrefsection
\endinput
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