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"Relation between Solar Wind Parameter and Geomagnetic Storm Condition during Cycle-23"
written by Balveer S. Rathore, Dinesh C. Gupta, K. K. Parashar ,
published by International Journal of Geosciences, Vol.5 No.13, 2014
has been cited by the following article(s):
[1]
Modeling the superstorm in the 24th solar cycle
2019
[2]
Solar wind plasma associated with Dst-50 nT during solar cycle 24
International Journal of Physical Sciences
2017
[3]
Mathematical modeling of the moderate storm on 28 February 2008
New Astronomy
2018
[4]
PENGARUH ORIENTASI MEDAN MAGNET ANTARPLANET PADA GANGGUAN GEOMAGNET DI LINTANG RENDAH
2016
[5]
Study of cosmic ray intensity and geomagnetic storms with solar wind parameters during the period 1998–2005
Astrophysics and Space Science
2017
[6]
The relation between solar radio burst types II, III and IV due to solar activities
Space Science and Communication (IconSpace), 2015 International Conference on
2015
[10]
Mathematical Analysis of the 09 March 2012 Intense Storm
2020
[11]
STUDY OF INTERPRETATION OF SEMI-DIURNAL ANISOTROPY OF THE COSMIC RAY
[12]
Study of the fractality in a magnetohydrodynamic shell model forced by solar wind fluctuations
2020
[15]
Study of the fractality in an MHD Shell model forced by solar wind fluctuations
2019
[18]
Study of Geomagnetic Storms and Solar and Interplanetary Parameters for Solar Cycles 22 and 24
Solar Physics
2018
[20]
Study of the fractality of magnetized plasma using an MHD shell model driven by solar wind data
AIP Conference Proceedings
2018
[21]
A comparative study of geomagnetic storms for solar cycles 23 and 24
Journal of Astrophysics and Astronomy
2018