Abstract Details

Name: PRITHVI RAJ SINGH
Affiliation: A.P.S.UNIVERSITY REWA M.P.
Conference ID: ASI2015_442
Title : Variation of odd-even solar cycle’s and their effect on earth’s climate
Authors and Co-Authors : B.K.TIWARI,A.K.SAXENA PRITHVI RAJ SINGH*
Abstract Type : Poster
Abstract Category : Sun and the Solar System
Abstract : Variation of odd-even solar cycle’s and their effect on earth’s climate PRITHVI RAJ SINGH, A.K.SAXENA, B.K.TIWARI Department of Physics A.P.S.University, Rewa, M.P.-486003(INDIA) E-mail: prithvisingh77@gmail.com Abstract To Study of influence of solar activity during solar cycle 21-24 on climate change specifically the change in the global mean temperature might have been associated with the variation of some solar activity indices .The important indices are total solar irradiance (TSI),Ultraviolet(UV)radiance and radio flux have been presented. The re construction of solar irradiance in the past period before accurate measurements of solar irradiance, ultraviolet radiance and radio flux. The study the sun climate relationship by averaging solar cycle21-24 and climate date at various time scales .the term global warming is now popularly used to refer the recent increases in the mean surface temperature of earth .the sun can have obvious effect on climate change and its radiation is the main energy source for the outer envelops of our planet. The climate changes are interested in understanding the effect of variation in the total and spectral solar irradiance on earth and its climate. Variation in total solar irradiance were too small to detect with technology available before the satellite although the small fraction in ultra-violet light has recently been found to vary significantly more than previously thought over the solar cycle 21-24.UV irradiance increase causes higher ozone production, leading to stratospheric heating and to pole ward displacements in the stratospheric and tropospheric wind systems. The most likely mechanism is considered to be some combination of direct forcing by change in total solar irradiance, and indirect effects of ultraviolet (UV) radiation the stratosphere. The solar particle streaming around the Earth’s magnetosphere using the long –lasting measurements and taking into account variable orbital parameters of the spacecraft. The distribution of the upstream particles was found to depend strongly on the solar cycle.