Home
World Journal of Advanced Research and Reviews
International Journal with High Impact Factor for fast publication of Research and Review articles

Main navigation

  • Home
    • Journal Information
    • Editorial Board Members
    • Reviewer Panel
    • Abstracting and Indexing
    • Journal Policies
    • Our CrossMark Policy
    • Publication Ethics
    • Issue in Progress
    • Current Issue
    • Past Issues
    • Instructions for Authors
    • Article processing fee
    • Track Manuscript Status
    • Get Publication Certificate
    • Join Editorial Board
    • Join Reviewer Panel
  • Contact us
  • Downloads

eISSN: 2581-9615 || CODEN: WJARAI || Impact Factor 8.2 ||  CrossRef DOI

Research and review articles are invited for publication in April 2026 (Volume 30, Issue 1) Submit manuscript

Cosmic ray intensity for minimum phase of 24 solar cycle

Breadcrumb

  • Home
  • Cosmic ray intensity for minimum phase of 24 solar cycle

Rani Ghuratia 1, * and Achyut Pandey 2

1 Govt. Model Science College, Rewa, M.P., India.
2 Department of Physics, Govt. T.R.S. College, Rewa, M. P., India.
 
Research Article
World Journal of Advanced Research and Reviews, 2024, 22(03), 324-330
Article DOI: 10.30574/wjarr.2024.22.3.1661
DOI url: https://doi.org/10.30574/wjarr.2024.22.3.1661
 
Received on 20 April 2024; revised on 02 June 2024; accepted on 05 June 2024
 
In this paper, we study the cosmic ray intensity behavior over the declining phase of the solar cycle 24, with the ground based ATHN neutron monitor (NM). For this purpose, we have considered the three parameters solar flare index (SFI), sunspot number (SSN) and magnitude of the magnetic field vector B. During the declining phase of cycle 24 the results shows that the cosmic ray intensity has moderate anticorrelation with the parameters SFI, SSN and field vector B having correlation coefficient -0.44, -0.43 and -0.51 respectively. From 2014 to 2019 sunspot numbers are going to be decreased, the maximum sunspot number was found in April 2014. Further we analyzed the sunspot number variation with solar flare index and magnetic field vector magnitude B and found that the sunspot number was directly related with these parameters, the correlative results showed that the SSN have strong positive correlation with SFI and field vector B with coefficient 0.72 and 0.62 of these two. Conclusively the cosmic ray intensity variation is not responsible for the variation in the considered parameters but sunspot number cycle does effect on different solar and interplanetary conditions.
 
Cosmic ray intensity; SSN; Solar flare index; field vector B.
 
https://wjarr.com/sites/default/files/fulltext_pdf/WJARR-2024-1661.pdf

Preview Article PDF

Rani Ghuratia and Achyut Pandey. Cosmic ray intensity for minimum phase of 24 solar cycle. World Journal of Advanced Research and Reviews, 2024, 22(3), 324-330. Article DOI: https://doi.org/10.30574/wjarr.2024.22.3.1661

Copyright © Author(s). All rights reserved. This article is published under the terms of the Creative Commons Attribution 4.0 International License (CC BY 4.0), which permits use, sharing, adaptation, distribution, and reproduction in any medium or format, as long as appropriate credit is given to the original author(s) and source, a link to the license is provided, and any changes made are indicated.


All statements, opinions, and data contained in this publication are solely those of the individual author(s) and contributor(s). The journal, editors, reviewers, and publisher disclaim any responsibility or liability for the content, including accuracy, completeness, or any consequences arising from its use.

Get Certificates

Get Publication Certificate

Download LoA

Check Corssref DOI details

Issue details

Issue Cover Page

Editorial Board

Table of content

Copyright © 2026 World Journal of Advanced Research and Reviews - All rights reserved

Developed & Designed by VS Infosolution