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PostWysłany: Sob 7:38, 22 Sty 2011    Temat postu: moncler milano A UNIFIED MODEL FOR SOLAR FLARES_23

A UNIFIED MODEL FOR SOLAR FLARES


alousresistivityinthelowercorona (withlarger7ze) requiresastrongermagneticfield, andviceversa. Ourmodelthenimpliesthatthereconnectingmagneticfieldisstrongerforthecompactflares, andweakerforthetwo-ribbonflares. SucharesultisinagreementwithShibata [. ItisnotedthattheshrinkageeffectasshowninFigure1alsoappearsinCaseB. Soourunifiedmodelfurtherpredictsthattheshrinkageeffectofthereconnectedmagneticloopmayalsooccurinthecom-pactflares. Toconclude, itistentativelysuggestedthattheusuallyclassifiedtwotypesofsolarflarescanbeunifiedintothesamereconneetionmode1. Theessenceisthattheheightofthereconnec-tionpointleadstothebifurcation, i. e. , Thereconneetionpointishighforthetwo-ribbonflares, andlowforthecompactflares. Ourunifiedmodelfurtherpredictsthattheshrinkageef-fectdiscoveredinthetwo-ribbonflaresalsoexistsinthecompactflares. 23456ReferencesPriestER. SolarFlareMHD. In: PriestER. NewYork, London, Paris: GordonandBreachSciencePublish-er8,moncler milano, 1981,1 ForbesTG, MalherbJM, PriestER. TheFormationofFlareLoopyMagneticReoonnectionandChromo-sphericAblation. SolarPhys, 1989,120:285 ChenPF, FangC,uggs kopen, TangYH, eta1. SimulationofMagneticRemnnectionwithHeatConduction. ApJ, l999,UGG Boots Outlet, 513:516 HeyvaertsJ, PriestER, RustDM. AnEmergingFluxMoldfortheSolarFlarePhenomenon. AN, 1977,216:123 MasudaS, KosugiT,asics australia, HaraH, eta1. ALoop-topHardX-raySourceinaCompactSolarFlareasEvidenceforMagneticRemnnection. Nature, 1994,371:495 ShibataK. AUnifiedMole1ofS0laxFlare. In: WatanabeTeta1. ObservationalPlasmaAstrophysics: FiveYearsofYohkohandBeyond. Dordrecht, Boston, London: KluwerAcademicPub,timberland shoes, 1998.187
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