@article{Dhakal_Adhikari_Pudasainee_Chapagain_Pandit_Dahal_Sapkota_Chhatkuli_2018, title={Correlation of solar wind velocity with different parameters during geomagnetic disturbances}, volume={16}, url={https://www.nepjol.info/index.php/BIBECHANA/article/view/21575}, DOI={10.3126/bibechana.v16i0.21575}, abstractNote={<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>}, journal={BIBECHANA}, author={Dhakal, Sujan and Adhikari, Binod and Pudasainee, Kiran and Chapagain, Naryan Prasad and Pandit, Drabindra and Dahal, Subodh and Sapkota, Bhawani and Chhatkuli, Daya Nidhi}, year={2018}, month={Nov.}, pages={165–176} }