6533b82ffe1ef96bd1295bb3
RESEARCH PRODUCT
Mean Interplanetary Magnetic Field Measurement Using the ARGO-YBJ Experiment
X. X. LiZhenyong FengL. ZhangB. D'ettorre PiazzoliL. XueG. MancarellaQ. B. GouA. CappaM. ZhaF. R. ZhuM. PanareoB. Z. DaiM. IacovacciPiero VallaniaP. CretiDanzengluobuF. RuggieriA. K. Calabrese MelcarneL. PerroneP. SalviniR. CardarelliG. MarsellaQ. Q. ZhuY. Q. GuoP. BranchiniH. Y. JiaG. AielliR. SantonicoH. H. HeC. BacciC. BacciS. M. MariS. M. MariZhengguo CaoX. C. YangB. S. WangA. PagliaroQ. Y. YangBingwei XuP. F. ZhangE. GirolettiSeverino Angelo Maria BussinoSeverino Angelo Maria BussinoS. W. CuiHongbo HuA. SurdoC. F. FengX. J. BiH. R. WuI. De MitriX. R. MengC. StanescuIrina JamesIrina JamesA. F. YuanChang-chun NingZhaoyang FengJ. Y. LiJilong ZhangT. Di GirolamoF. ShiJianli ZhangT. L. ChenH. M. ZhangG. Di SciascioCarlo VigoritoCarlo VigoritoP. CelioC. Y. WuM. Y. LiuM. De VincenziM. De VincenziHaibing HuR. GarganaI. BologninoB. BartoliH. J. LiX. D. ShengC. BleveY. B. ChenS. Z. ChenL. SaggeseY. ZhangB. LibertiPaolo BernardiniD. MartelloX. B. QuX. H. DingLabacirenJ. K. K. LiuP. PistilliP. PistilliX. X. ZhouG. D'alí StaitiG. D'alí StaitiY. H. TanP. GaleottiP. GaleottiQ. HuangX. Y. ZhangC. LiuX. H. MaG. LiguoriG. LiguoriC. X. LiuZhaxisangzhuS. CatalanottiZ. G. YaoY. X. YanE. RossiM. DattoliM. DattoliH. LuPaolo MontiniPaolo MontiniR. IuppaAnd G. ZizziP. CamarriH. W. WangS. VernettoF. GaleazziA. BudanoS. MastroianniC. CattaneoP. R. Shensubject
Solar SystemField (physics)media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldCosmic rayHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Settore FIS/05 - Astronomia E AstrofisicaShadowAstrophysics::Solar and Stellar AstrophysicsInterplanetary magnetic fieldcosmic raySolar and Stellar Astrophysics (astro-ph.SR)media_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCosmic Rays Gamma Sources Extended Air Showers Solar windMagnetic fieldSolar windAstrophysics - Solar and Stellar Astrophysicssolar windSpace and Planetary ScienceSkyPhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadescription
The sun blocks cosmic ray particles from outside the solar system, forming a detectable shadow in the sky map of cosmic rays detected by the ARGO-YBJ experiment in Tibet. Because the cosmic ray particles are positive charged, the magnetic field between the sun and the earth deflects them from straight trajectories and results in a shift of the shadow from the true location of the sun. Here we show that the shift measures the intensity of the field which is transported by the solar wind from the sun to the earth.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2011-01-01 |