Symmetrie Cosmic Ray Intensity Decreases in Relation with Coronal Mass Ejections and Disturbances In Solar Wind Plasma Parameters

15th International Congress on Plasma Physics; 13th Latin American Workshop on Plasma Physics

Verma, P.L.^1 ; Tripathi, Omkar^2 ; Vishwkarma, Ashok Kumar^2

Department of Physics, Govt. Vivekanand P.G. College, Maihar, Satna, M.P., India^1

Research Scholar Govt. P.G. College, Satna, M.P., India^2

关键词: Association rates;    Coronal mass ejection;    Correlation coefficient;    Cosmic ray intensity;    Interplanetary shocks;    Neutron monitors;    Solar wind plasmas;    Wind temperature;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/511/1/012058/pdf
DOI  :  10.1088/1742-6596/511/1/012058

来源: IOP

【 摘 要 】

We have studied symmetric cosmic ray intensity decreases (V Shape, and U Shape) magnitude ≥ 2.0%, observed at Oulu super neutron monitor, during the period of 1986-2006 with coronal mass ejections CMEs), interplanetary shocks and disturbances in solar wind plasma parameters (solar wind temperature, velocity, density). We have found that 76.92% V shape symmetric cosmic ray intensity decreases are associated with halo and partial halo coronal mass ejections (CMEs). The association rate between halo and partial halo coronal mass ejections are found 40.00%and 60.00% respectively. Most of the V Shape symmetric cosmic ray intensity decreases are related to interplanetary shocks (61.53%) and the related shocks are forward shocks. We have also found positive co-relation with co-relation co-efficient 0.54 between magnitude of V shape symmetric cosmic ray intensity decreases and speed of associated coronal mass ejections. From the further study it is concluded that V shape symmetric cosmic ray decreases are strongly related to the disturbances in solar wind plasma parameters. Negative co-relation has been found between magnitudes of V Shape symmetric cosmic ray intensity decreases and magnitude of jump in solar wind plasma density of associated JSWD events with co-relation co-efficient -0.152 between these two events. Negative co-relation has also been found between magnitude of V Shape asymmetric cosmic ray intensity decreases and magnitude of jump in solar wind plasma velocity of the associated JSWV events with co-relation co-efficient -0.48 between these two events. From the study of U Shape symmetric cosmic ray intensity decreases and disturbances in solar wind plasma parameters, we found negative co-relation with correlation coefficient, -0.473 between magnitude of U shape symmetric cosmic ray intensity decreases and magnitude of jump in solar wind plasma temperature of associated JSWT events, -0.468 between magnitude of U shape symmetric cosmic ray intensity decreases and magnitude of jump in solar wind plasma density of associated JSWD events and -0.26 between U shape symmetric cosmic ray intensity decreases and magnitude of jump in solar wind plasma velocity of associated JSWV events.