z-logo
open-access-imgOpen Access
Influence of solar X-ray flares on the earth-ionosphere waveguide
Author(s) -
D. Grubor,
D. Šulić,
V. J. Žigman
Publication year - 2005
Publication title -
serbian astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.196
H-Index - 16
eISSN - 1820-9289
pISSN - 1450-698X
DOI - 10.2298/saj0571029g
Subject(s) - physics , amplitude , ionosphere , solar flare , earth–ionosphere waveguide , signal (programming language) , satellite , solar cycle , astrophysics , waveguide , remote sensing , astronomy , plasma , optics , ionospheric absorption , solar wind , geology , nuclear physics , computer science , programming language
A simultaneous analysis of solar are X-ray irradiance and VLF signal amplitude on the GQD/22.1 kHz trace was carried out. Solar are data were taken from GOES 12 satellite listings. The VLF amplitude data were recorded by means of the AbsPAL (Absolute Phase and Amplitude Logger) at the Institute of Physics, Belgrade, Serbia. It was found that solar are events from class C to class X affect the VLF signal amplitude in various ways and can be classified according to the type of effect produced in the Earth-ionosphere waveguide on the VLF propagation

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom