id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
bibechana-21575	Dhakal, Sujan; Adhikari, Binod; Pudasainee, Kiran; Chapagain, Naryan Prasad; Pandit, Drabindra; Dahal, Subodh; Sapkota, Bhawani; Chhatkuli, Daya Nidhi	Correlation of solar wind velocity with different parameters during geomagnetic disturbances	2018	12	.pdf	application/pdf	4316	258	58	This disturbance may occur due to solar wind, coronal mass ejection (CME), solar flare, corotating interaction region (CIR) Solar wind is the continuous flow of plasma coming out from the sun [3].	cache/bibechana-21575.pdf	txt/bibechana-21575.txt