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Solar Physics

, 292:149 | Cite as

Impacts on Cosmic-Ray Intensity Observed During Geomagnetic Disturbances

  • Binod Adhikari
  • Nirakar Sapkota
  • Prashrit Baruwal
  • Narayan P. Chapagain
  • Carlos Roberto Braga
Article

Abstract

Geomagnetic disturbances are the results of interplanetary causes such as high-speed streamers (HSSs), interplanetary coronal mass ejections (ICMEs), corotating interaction regions (CIRs), and magnetic clouds. During different forms of geomagnetic disturbances, we observed changes in the count rate at neutron monitors that are kept at various locations. We studied the count rates measured by neutron monitors at four stations at various latitudes during different categories of geomagnetic events and compared them. We analysed five events: a geomagnetically quiet event, a non-storm high-intensity long-duration continuous AE activity (HILDCAA) event, a storm-preceded HILDCAA event, a geomagnetic substorm event, and a geomagnetic moderate storm event. We based our analysis on geomagnetic indices, solar wind parameters, and interplanetary magnetic field (IMF) parameters. We found that the strength of the modulation was least during the quiet event and highest during the storm-preceded HILDCAA. By analysing the cause of these geomagnetic disturbances, we related each decrease in the neutron monitor data with the corresponding solar cause. For the ICME-driven storm, we observed a decrease in neutron monitor data ranging from 6% to 12% in all stations. On the other hand, we observed a decrease ranging from 2% to 5% for the HSS-driven storm. For the non-storm HILDCAA, we observed a decrease in neutron monitor data of about 1% to 1.5%. For the quiet event, the neutron monitor data fluctuated such that there was no overall decrease in all stations.

Keywords

Geomagnetic disturbances Storm Substorm Moderate storm HILDCAA Neutron monitor data 

Notes

Acknowledgements

The solar wind and interplanetary magnetic field data for this study were obtained from https://omniweb.gsfc.nasa.gov/ . The neutron monitors of the Bartol Research Institute are supported by NSF grant ATM-0527878. We downloaded the neutron data from www.neutronm.bartol.udel.edu . C.R. Braga acknowledges grants 2014/24711-6, 2013/02712-8, and 2012/05436-9 from the São Paulo Research Foundation (FAPESP).

Disclosure of Potential Conflicts of Interest

The authors declare that they have no conflicts of interest.

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Copyright information

© Springer Science+Business Media B.V. 2017

Authors and Affiliations

  • Binod Adhikari
    • 1
    • 2
  • Nirakar Sapkota
    • 2
  • Prashrit Baruwal
    • 3
  • Narayan P. Chapagain
    • 1
  • Carlos Roberto Braga
    • 4
  1. 1.Department of Physics, Patan M. CampusTribhuvan UniversityLalitpurNepal
  2. 2.Department of PhysicsSt. Xavier’s CollegeKathmanduNepal
  3. 3.Department of Physics, Amrit Science CampusTribhuvan UniversityKathmanduNepal
  4. 4.National Institute for Space Research – INPESão José dos CamposBrazil

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