Zobrazeno 1 - 10
of 501
pro vyhledávání: '"S R, Verma"'
Autor:
Dr. S. R. Verma, Dr. ASHISH RAYAL
Publikováno v:
Applied Numerical Mathematics. 174:191-220
Autor:
S. R. Verma, A. Kumar
Publikováno v:
Advances in Mathematics: Scientific Journal. 10:2285-2294
In this paper, a modified Taylor wavelet method (MTWM) is developed for numerical solutions of various types of Abel's integral equations. This method is based on the modified Taylor wavelet (MTW) approximation. The purpose behind using the MTW appro
Autor:
Chaurasia Basant, S R Verma
Publikováno v:
Indian Journal of Anesthesia and Analgesia. 5:1620-1622
Publikováno v:
Indian Journal of Plant Physiology. 21:93-100
The utilization of physiological traits in genetic improvement of drought tolerance in barley (Hordeum vulgare L.) requires establishment of significant association between grain yield and the physiological traits and their genetic variations. The st
Publikováno v:
Asset Analytics ISBN: 9789811308710
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cc49715d17ead7b8a9462164202c605d
https://doi.org/10.1007/978-981-13-0872-7_10
https://doi.org/10.1007/978-981-13-0872-7_10
Autor:
S. R. Verma, Sanjay Khot
Publikováno v:
International Journal of Innovative Research in Medical Science. 3
INTRODUCTION Anaesthesia is classified into two main techniques general anaesthesia (GA) in which gaseous and/or intravenous drugs achieve central neurological depression, and regional anaesthesia, in which drugs are administered directly to the vici
Publikováno v:
AGRICULTURE UPDATE. 9:279-287
Autor:
S. R. Verma, Aradhna Sharma
Publikováno v:
International Journal of Astronomy and Astrophysics. :212-216
Solar activity refers to any natural phenomenon occurring on the sun such as sunspots, solar flare and coronal mass ejection etc. Such phenomena have their roots deep inside the sun, where the dynamo mechanism operates and fluid motions occur in a tu
Autor:
S. R. Verma, Mohan Lal
Publikováno v:
Macromolecular Symposia. 376:1700017
Autor:
S. R. Verma, Diksha Chaudhary
Publikováno v:
Journal of Astrophysics and Astronomy. 29:253-256
One of the fundamental questions in solar physics is how the solar corona maintains its high temperature of several million Kelvin above photosphere with a temperature of 6000 K.