FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2422074463> ?p ?o ?g. }

• W2422074463 endingPage "2366" @default.
• W2422074463 startingPage "2353" @default.
• W2422074463 abstract "We present calculations of the auroral radio powers expected from exoplanets with magnetospheres driven by an Earth-like magnetospheric interaction with the solar wind. Specifically, we compute the twin cell-vortical ionospheric flows, currents, and resulting radio powers resulting from a Dungey cycle process driven by dayside and nightside magnetic reconnection, as a function of planetary orbital distance and magnetic field strength. We include saturation of the magnetospheric convection, as observed at the terrestrial magnetosphere, and we present power law approximations for the convection potentials, radio powers and spectral flux densities. We specifically consider a solar-age system and a young (1 Gyr) system. We show that the radio power increases with magnetic field strength for magnetospheres with saturated convection potential, and broadly decreases with increasing orbital distance. We show that the magnetospheric convection at hot Jupiters will be saturated, and thus unable to dissipate the full available incident Poynting flux, such that the magnetic Radiometric Bode's Law (RBL) presents a substantial overestimation of the radio powers for hot Jupiters. Our radio powers for hot Jupiters are $sim$5-1300 TW for hot Jupiters with field strengths of 0.1-10 $B_J$ orbiting a Sun-like star, while we find that competing effects yield essentially identical powers for hot Jupiters orbiting a young Sun-like star. However, in particular for planets with weaker magnetic fields our powers are higher at larger orbital distances than given by the RBL, and there are many configurations of planet that are expected to be detectable using SKA." @default.
• W2422074463 created "2016-06-24" @default.
• W2422074463 creator A5050072202 @default.
• W2422074463 creator A5060523674 @default.
• W2422074463 date "2016-06-20" @default.
• W2422074463 modified "2023-09-26" @default.
• W2422074463 title "Stellar wind–magnetosphere interaction at exoplanets: computations of auroral radio powers" @default.
• W2422074463 cites W1514113592 @default.
• W2422074463 cites W1540141260 @default.
• W2422074463 cites W1596521250 @default.
• W2422074463 cites W1646976279 @default.
• W2422074463 cites W1847169201 @default.
• W2422074463 cites W1867591249 @default.
• W2422074463 cites W1966856590 @default.
• W2422074463 cites W1968024107 @default.
• W2422074463 cites W1968526024 @default.
• W2422074463 cites W1975426531 @default.
• W2422074463 cites W1978072444 @default.
• W2422074463 cites W1981043397 @default.
• W2422074463 cites W1984373669 @default.
• W2422074463 cites W1984600682 @default.
• W2422074463 cites W1986846568 @default.
• W2422074463 cites W1989010173 @default.
• W2422074463 cites W1990957712 @default.
• W2422074463 cites W1993092353 @default.
• W2422074463 cites W1993881149 @default.
• W2422074463 cites W1998449200 @default.
• W2422074463 cites W2003412632 @default.
• W2422074463 cites W2003679820 @default.
• W2422074463 cites W2008444642 @default.
• W2422074463 cites W2015570839 @default.
• W2422074463 cites W2018600301 @default.
• W2422074463 cites W2019836572 @default.
• W2422074463 cites W2022902363 @default.
• W2422074463 cites W2037726156 @default.
• W2422074463 cites W2045483269 @default.
• W2422074463 cites W2050344634 @default.
• W2422074463 cites W2050541856 @default.
• W2422074463 cites W2050993929 @default.
• W2422074463 cites W2054626887 @default.
• W2422074463 cites W2054674651 @default.
• W2422074463 cites W2054871050 @default.
• W2422074463 cites W2058372014 @default.
• W2422074463 cites W2061341933 @default.
• W2422074463 cites W2061751143 @default.
• W2422074463 cites W2071217802 @default.
• W2422074463 cites W2076185700 @default.
• W2422074463 cites W2077657280 @default.
• W2422074463 cites W2077698413 @default.
• W2422074463 cites W2082516044 @default.
• W2422074463 cites W2083745993 @default.
• W2422074463 cites W2084011810 @default.
• W2422074463 cites W2085643960 @default.
• W2422074463 cites W2090253495 @default.
• W2422074463 cites W2095626152 @default.
• W2422074463 cites W2096772726 @default.
• W2422074463 cites W2105088954 @default.
• W2422074463 cites W2124248640 @default.
• W2422074463 cites W2127321908 @default.
• W2422074463 cites W2136069370 @default.
• W2422074463 cites W2146664871 @default.
• W2422074463 cites W2159529540 @default.
• W2422074463 cites W2168227401 @default.
• W2422074463 cites W2169081815 @default.
• W2422074463 cites W2169306484 @default.
• W2422074463 cites W2949477719 @default.
• W2422074463 cites W3099882219 @default.
• W2422074463 cites W3100272176 @default.
• W2422074463 cites W3100566802 @default.
• W2422074463 cites W3104011290 @default.
• W2422074463 cites W3106197312 @default.
• W2422074463 cites W3122006059 @default.
• W2422074463 cites W4243024367 @default.
• W2422074463 doi "https://doi.org/10.1093/mnras/stw1430" @default.
• W2422074463 hasPublicationYear "2016" @default.
• W2422074463 type Work @default.
• W2422074463 sameAs 2422074463 @default.
• W2422074463 citedByCount "55" @default.
• W2422074463 countsByYear W24220744632016 @default.
• W2422074463 countsByYear W24220744632017 @default.
• W2422074463 countsByYear W24220744632018 @default.
• W2422074463 countsByYear W24220744632019 @default.
• W2422074463 countsByYear W24220744632020 @default.
• W2422074463 countsByYear W24220744632021 @default.
• W2422074463 countsByYear W24220744632022 @default.
• W2422074463 countsByYear W24220744632023 @default.
• W2422074463 crossrefType "journal-article" @default.
• W2422074463 hasAuthorship W2422074463A5050072202 @default.
• W2422074463 hasAuthorship W2422074463A5060523674 @default.
• W2422074463 hasBestOaLocation W24220744631 @default.
• W2422074463 hasConcept C108411613 @default.
• W2422074463 hasConcept C10899652 @default.
• W2422074463 hasConcept C115260700 @default.
• W2422074463 hasConcept C121332964 @default.
• W2422074463 hasConcept C1276947 @default.
• W2422074463 hasConcept C130443932 @default.
• W2422074463 hasConcept C140161248 @default.
• W2422074463 hasConcept C163479331 @default.

• next