DocumentCode
1923136
Title
VLF study of Ionospheric properties during solar flares of varied intensity for a fixed propagation path
Author
Basak, Tamal ; Pal, S. ; Chakrabarti, S.K.
Author_Institution
S.N. Bose Nat. Centre for Basic Sci., Kolkata, India
fYear
2011
fDate
13-20 Aug. 2011
Firstpage
1
Lastpage
4
Abstract
Deviations of subionospheric VLF signal amplitude due to solar flares of several energy classes have been computed for the VLF signal propagating along the VTX-Kolkata baseline. Using Long Wave Propagation Capability Code (LWPC), the variation of the effective height h´ and steepness β parameters have been computed for X, M and C classes of solar flares. We compute the temporal variation of the electron number density.
Keywords
ionospheric electromagnetic wave propagation; solar flares; C class; M class; VLF signal amplitude; VLF study; VTX-Kolkata baseline; X class; effective height; electron number density; fixed propagation path; ionospheric properties; long wave propagation capability code; solar flares; steepness beta parameters; temporal variation; Computational modeling; Ionization; Ionosphere; Optimized production technology; Receivers; Satellites; Spontaneous emission;
fLanguage
English
Publisher
ieee
Conference_Titel
General Assembly and Scientific Symposium, 2011 XXXth URSI
Conference_Location
Istanbul
Print_ISBN
978-1-4244-5117-3
Type
conf
DOI
10.1109/URSIGASS.2011.6051004
Filename
6051004
Link To Document