Open AccessAn analysis of thermospheric density response to solar flares during 2001–2006
Author(s) -
Le Huijun,
Liu Libo,
Wan Weixing
Publication year - 2012
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2011ja017214
Subject(s) - extreme ultraviolet lithography , thermosphere , solar flare , physics , solar minimum , flare , flux (metallurgy) , atmospheric sciences , astrophysics , solar cycle , extreme ultraviolet , atmosphere (unit) , solar maximum , ionosphere , astronomy , plasma , meteorology , optics , solar wind , materials science , laser , quantum mechanics , metallurgy
Previous studies show there are significant thermospheric responses to the two great solar flares on October 28, 2003 (X17.2) and November 4, 2003 (X28). In the present study, we further explored the thermospheric response to all X‐class solar flares during 2001–2006. The observed results show that X5 and stronger solar flares can induce an average enhancement of 10–13% in thermospheric density in latitude 50°S‐50°N within ∼4 h after the flare onset. Many important lines and continua in solar EUV region are optically thick, thus EUV enhancements are smaller for flares located near the solar limb due to absorption by the solar atmosphere. Limb flares induce smaller thermospheric responses, due to the limb effect of solar EUV. The thermospheric density enhancement is much more correlated with integrated EUV flux than with peak EUV flux, with a high correlation coefficient of 0.91, which suggests that thermospheric response is strongly dependent on the total integrated energy into the thermosphere.