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dc.contributor.authorHodosán, G.
dc.contributor.authorHelling, Ch.
dc.contributor.authorAsensio-Torres, R.
dc.contributor.authorVorgul, I.
dc.contributor.authorRimmer, P. B.
dc.identifier.citationHodosán , G , Helling , C , Asensio-Torres , R , Vorgul , I & Rimmer , P B 2016 , ' Lightning climatology of exoplanets and brown dwarfs guided by Solar system data ' , Monthly Notices of the Royal Astronomical Society , vol. 461 , no. 4 , pp. 3927-3947 .
dc.identifier.otherPURE: 246545964
dc.identifier.otherPURE UUID: 7544c197-1e35-44bf-b516-e77d7056e616
dc.identifier.otherScopus: 84988667401
dc.identifier.otherWOS: 000383514900043
dc.descriptionWe highlight financial support of the European Community under the FP7 by an ERC starting grant number 257431. RAT thanks the Royal Astronomical Society (RAS) and the Physics Trust of the University of St Andrews for supporting his summer placement at the University of St Andrews.en
dc.description.abstractClouds form on extrasolar planets and brown dwarfs where lightning could occur. Lightning is a tracer of atmospheric convection, cloud formation and ionization processes as known from the Solar system, and may be significant for the formation of prebiotic molecules. We study lightning climatology for the different atmospheric environments of Earth, Venus, Jupiter and Saturn. We present lightning distribution maps for Earth, Jupiter and Saturn, and flash densities for these planets and Venus, based on optical and/or radio measurements from the World Wide Lightning Location Network and Sferics Timing and Ranging Network radio networks, the Lightning Imaging Sensor/Optical Transient Detector satellite instruments, the Galileo, Cassini, New Horizons and Venus Express spacecraft. We also present flash densities calculated for several phases of two volcano eruptions, Eyjafjallajökull's (2010) and Mt Redoubt's (2009). We estimate lightning rates for sample, transiting and directly imaged extrasolar planets and brown dwarfs. Based on the large variety of exoplanets, six categories are suggested for which we use the lightning occurrence information from the Solar system. We examine lightning energy distributions for Earth, Jupiter and Saturn. We discuss how strong stellar activity may support lightning activity. We provide a lower limit of the total number of flashes that might occur on transiting planets during their full transit as input for future studies. We find that volcanically very active planets might show the largest lightning flash densities. When applying flash densities of the large Saturnian storm from 2010/11, we find that the exoplanet HD 189733b would produce high lightning occurrence even during its short transit.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at:
dc.subjectAtmospheric effectsen
dc.subjectBrown dwarfsen
dc.subjectPlanetary systemsen
dc.subjectPlanets and satellites: atmospheresen
dc.subjectPlanets and satellites: individual: Earth, Venus, Jupiter, Saturnen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectAstronomy and Astrophysicsen
dc.subjectSpace and Planetary Scienceen
dc.titleLightning climatology of exoplanets and brown dwarfs guided by Solar system dataen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.description.statusPeer revieweden

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