Correlation of solar wind velocity with different parameters during geomagnetic disturbances

Correlation of solar wind velocity with different parameters during geomagnetic disturbances

<p>We have studied the solar wind velocity and it’s relation with solar wind pressure, southward component of IMF-Bz, solar wind temperature (Tsw), solar wind density (Nsw) and geomagnetic indices during different geomagnetic disturbances. During disturbed days, there is a fluctuation of energ...

Full description

Bibliographic Details
Main Authors: Sujan Dhakal, Binod Adhikari, Kiran Pudasainee, Naryan Prasad Chapagain, Drabindra Pandit, Subodh Dahal, Bhanu Sapkota, Daya Nidhi Chhatkuli
Format: Article
Language:English
Published: Department of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan University 2018-11-01
Series:Bibechana
Subjects:
Geomagnetic storm
solar wind velocity
cross-correlation analysis.
Online Access:https://www.nepjol.info/index.php/BIBECHANA/article/view/21575
id doaj-74848fdb88e34964ac211202b0c87d8b
record_format Article
spelling doaj-74848fdb88e34964ac211202b0c87d8b2020-11-25T02:36:07ZengDepartment of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan UniversityBibechana2091-07622382-53402018-11-0116016517610.3126/bibechana.v16i0.2157516754Correlation of solar wind velocity with different parameters during geomagnetic disturbancesSujan Dhakal0Binod Adhikari1Kiran Pudasainee2Naryan Prasad Chapagain3Drabindra Pandit4Subodh Dahal5Bhanu Sapkota6Daya Nidhi Chhatkuli7St. Xavier’s College, Maitighar, KathmanduPatan Multiple Campus, Patandhoka, LalitpurPatan Multiple Campus, Patandhoka, LalitpurCentral Department of Physics, Tribhuvan University, Kirtipur, KathmanduSt. Xavier’s College, Maitighar, KathmanduDepartment of Physics, Himalayan College of Geomatic Engineering and LRM, KathmanduDepartment of Physics, Himalayan College of Geomatic Engineering and LRM, KathmanduDepartment of Physics, Tri-Chandra Multiple Campus, Kathmandu<p>We have studied the solar wind velocity and it’s relation with solar wind pressure, southward component of IMF-Bz, solar wind temperature (Tsw), solar wind density (Nsw) and geomagnetic indices during different geomagnetic disturbances. During disturbed days, there is a fluctuation of energy and plasma inside the magnetosphere, which changes the parameters like pressure, velocity, IMF-Bz, SYM-H and AE indices. The solar wind velocity shows very remarkable relationship with pressure. There is weak connection of solar wind pressure with IMF-Bz, although it is more geo-effective.</p><p>BIBECHANA 16 (2019) 165-176</p>https://www.nepjol.info/index.php/BIBECHANA/article/view/21575Geomagnetic stormsolar wind velocitycross-correlation analysis.
collection DOAJ
language English
format Article
sources DOAJ
author Sujan Dhakal
Binod Adhikari
Kiran Pudasainee
Naryan Prasad Chapagain
Drabindra Pandit
Subodh Dahal
Bhanu Sapkota
Daya Nidhi Chhatkuli
spellingShingle Sujan Dhakal
Binod Adhikari
Kiran Pudasainee
Naryan Prasad Chapagain
Drabindra Pandit
Subodh Dahal
Bhanu Sapkota
Daya Nidhi Chhatkuli
Correlation of solar wind velocity with different parameters during geomagnetic disturbances
Bibechana
Geomagnetic storm
solar wind velocity
cross-correlation analysis.
author_facet Sujan Dhakal
Binod Adhikari
Kiran Pudasainee
Naryan Prasad Chapagain
Drabindra Pandit
Subodh Dahal
Bhanu Sapkota
Daya Nidhi Chhatkuli
author_sort Sujan Dhakal
title Correlation of solar wind velocity with different parameters during geomagnetic disturbances
title_short Correlation of solar wind velocity with different parameters during geomagnetic disturbances
title_full Correlation of solar wind velocity with different parameters during geomagnetic disturbances
title_fullStr Correlation of solar wind velocity with different parameters during geomagnetic disturbances
title_full_unstemmed Correlation of solar wind velocity with different parameters during geomagnetic disturbances
title_sort correlation of solar wind velocity with different parameters during geomagnetic disturbances
publisher Department of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan University
series Bibechana
issn 2091-0762
2382-5340
publishDate 2018-11-01
description <p>We have studied the solar wind velocity and it’s relation with solar wind pressure, southward component of IMF-Bz, solar wind temperature (Tsw), solar wind density (Nsw) and geomagnetic indices during different geomagnetic disturbances. During disturbed days, there is a fluctuation of energy and plasma inside the magnetosphere, which changes the parameters like pressure, velocity, IMF-Bz, SYM-H and AE indices. The solar wind velocity shows very remarkable relationship with pressure. There is weak connection of solar wind pressure with IMF-Bz, although it is more geo-effective.</p><p>BIBECHANA 16 (2019) 165-176</p>
topic Geomagnetic storm
solar wind velocity
cross-correlation analysis.
url https://www.nepjol.info/index.php/BIBECHANA/article/view/21575
work_keys_str_mv AT sujandhakal correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT binodadhikari correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT kiranpudasainee correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT naryanprasadchapagain correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT drabindrapandit correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT subodhdahal correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT bhanusapkota correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
AT dayanidhichhatkuli correlationofsolarwindvelocitywithdifferentparametersduringgeomagneticdisturbances
_version_ 1724801072766124032

Similar Items