IJRTI
International Journal for Research Trends and Innovation
International Peer Reviewed & Refereed Journals, Open Access Journal
ISSN Approved Journal No: 2456-3315 | Impact factor: 8.14 | ESTD Year: 2016
Scholarly open access journals, Peer-reviewed, and Refereed Journals, Impact factor 8.14 (Calculate by google scholar and Semantic Scholar | AI-Powered Research Tool) , Multidisciplinary, Monthly, Indexing in all major database & Metadata, Citation Generator, Digital Object Identifier(DOI)

Call For Paper

For Authors

Forms / Download

Published Issue Details

Editorial Board

Other IMP Links

Facts & Figure

Impact Factor : 8.14

Issue per Year : 12

Volume Published : 11

Issue Published : 118

Article Submitted : 21653

Article Published : 8541

Total Authors : 22459

Total Reviewer : 811

Total Countries : 159

Indexing Partner

Licence

This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License
Published Paper Details
Paper Title: THE INFLUENCE OF SOLAR CORONAL MASS EJECTIONS AND INTERPLANETARY MAGNETIC FIELDS ON FORBUSH DECREASES IN COSMIC RAY INTENSITY DURING SOLAR CYCLE 24
Authors Name: Dhanraj , Anita Shukla , Laxmikant
Download E-Certificate: Download
Author Reg. ID:
IJRTI_205413
Published Paper Id: IJRTI2507103
Published In: Volume 10 Issue 7, July-2025
DOI: https://doi.org/10.56975/ijrti.v10i7.205413
Abstract: We studied the Forbush decreases of cosmic rays intensity during the Solar Cycle 24 using the Moscow Neutron Monitor. Forbush decreases (FDs) are sudden, short-term reductions in cosmic ray intensity observed on Earth, commonly triggered by solar events such as Coronal Mass Ejections (CMEs), solar flare (SFs) and Interplanetary Magnetic Fields (IMFs). We will explore the effects of major causes of Forbush decreases such as solar coronal mass injection, solar flares and Interplanetary Magnetic Field (IMF) to understand how the Fds in cosmic ray intensity are caused by them. This paper explores the effect of solar CME, SF and IMF on Forbush decreases as well as their interaction and investigates the underlying mechanisms responsible for the modulation of cosmic ray intensity during these events.In this study report, we have gathered a total of 56 Forbush decreases of magnitude ≥3% from the Moscow Neutron Monitor during Solar Cycle 24. This study uses observational data from Moscow neutron monitors, Omniweb, National Oceanic and Atmospheric Administration (NOAA) and the Solar and Heliospheric Observatory (SOHO) to examine how the IMF, solar flares, and CMEs impact FDs during SC 24. 94% of Fds are linked to solar flares, and the majorities are linked to halo CME and partial halo CME, according to our observations. The magnitude of Fds and the speed of CME were shown to be positively correlated, with a coefficient of 0.28. Also, all the Forbush decreases are associated with IMF. We observe a positive correlation between the magnitude of Fds and the peak value of IMF, with a correlation coefficient of 0.24. We found a positive correlation between the magnitude of Fds and the magnitude of IMF, with a correlation coefficient of 0.25. We concluded that the CME associated with IMF and SF are responsible for the Forbush decreases.
Keywords: Forbush decreases (Fds), Coronal Mass Ejections (CMEs), Interplanetary magnetic fields (IMF), Solar Flare (SF), Solar Cycle (SC), Cosmic Rays (CR)
Cite Article: "THE INFLUENCE OF SOLAR CORONAL MASS EJECTIONS AND INTERPLANETARY MAGNETIC FIELDS ON FORBUSH DECREASES IN COSMIC RAY INTENSITY DURING SOLAR CYCLE 24", International Journal for Research Trends and Innovation (www.ijrti.org), ISSN:2455-2631, Vol.10, Issue 7, page no.b9-b17, July-2025, Available :http://www.ijrti.org/papers/IJRTI2507103.pdf
Downloads: 000424
ISSN: 2456-3315 | IMPACT FACTOR: 8.14 Calculated By Google Scholar| ESTD YEAR: 2016
An International Scholarly Open Access Journal, Peer-Reviewed, Refereed Journal Impact Factor 8.14 Calculate by Google Scholar and Semantic Scholar | AI-Powered Research Tool, Multidisciplinary, Monthly, Multilanguage Journal Indexing in All Major Database & Metadata, Citation Generator
Publication Details: Published Paper ID: IJRTI2507103
Registration ID:205413
Published In: Volume 10 Issue 7, July-2025
DOI (Digital Object Identifier): https://doi.org/10.56975/ijrti.v10i7.205413
Page No: b9-b17
Country: -, -, India
Research Area: Engineering
Publisher : IJ Publication
Published Paper URL : https://www.ijrti.org/viewpaperforall?paper=IJRTI2507103
Published Paper PDF: https://www.ijrti.org/papers/IJRTI2507103
Share Article:

Click Here to Download This Article

Article Preview
Click Here to Download This Article

Major Indexing from www.ijrti.org
Google Scholar ResearcherID Thomson Reuters Mendeley : reference manager Academia.edu
arXiv.org : cornell university library Research Gate CiteSeerX DOAJ : Directory of Open Access Journals
DRJI Index Copernicus International Scribd DocStoc

ISSN Details

ISSN: 2456-3315
Impact Factor: 8.14 and ISSN APPROVED, Journal Starting Year (ESTD) : 2016

DOI (A digital object identifier)


Providing A digital object identifier by DOI.ONE
How to Get DOI?

Conference

Open Access License Policy

This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License

Creative Commons License This material is Open Knowledge This material is Open Data This material is Open Content

Important Details

Join RMS/Earn 300

IJRTI

WhatsApp
Click Here

Indexing Partner