%0 Journal Article
%T ThreeDimensionalSimulationoftheSteadySolarWindinCarringtonRotation1935
%A XIANG
%A Changqing
%A FENG
%A Xueshang
%A YAO
%A Jiusheng
%J 空间科学学报
%P 8-13
%D 2006
%X Athree-dimensionalMHDsimulationisconductedtostudythesteadysolarwindinCarringtonRotation(CR)1935byusingthethree-dimensionalnumericalmagnetohydrodynamic(MHD)modelintroducedbyFengetal.Thenumericalresultsdemonstratethattheneutralcurrentsheethastwopeaksandtwovalleys,whichisconsistentwiththeresultofPFSSmodelatWilcoxSolarObservatory(WSO).Theobtainedprotonnumberdensityat2.5RsisofthesameorderofmagnitudeastheresultestimatedfromK-coronalbrightnessduringtheCRs1733-1742in1983madebyWeietal.TheradialvelocityprofilealongheliocentricdistanceisconsistentwiththatoflowsolarwindspeeddeducedbySheeleyandWangetal.However,itisnotabletoreproducethefast-speedflowincoronalholesandslowsolarwindinstreamersbecauseofoversimplifiedenergyequationadoptedinourmodel.Futureeffortsmustbemadetoremedythisdeficiency.
%K MHDsimulation
%K Steadysolarwind
%U http://www.cjss.ac.cn/CN/abstract/abstract895.shtml