LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES

Using data from ground-based vertical sounding of the ionosphere (VS) at the station Moscow and five Japanese stations for the period from 1969 to 2015, we have examined the long-term response of the E layer to solar X-ray flares. The analysis relies on the previously developed method for estimating...

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Main Authors: G.V. Givishvili, L.N. Leshchenko
Format: Article
Language:English
Published: INFRA-M 2022-03-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/45266/view
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author G.V. Givishvili
L.N. Leshchenko
author_facet G.V. Givishvili
L.N. Leshchenko
author_sort G.V. Givishvili
collection DOAJ
description Using data from ground-based vertical sounding of the ionosphere (VS) at the station Moscow and five Japanese stations for the period from 1969 to 2015, we have examined the long-term response of the E layer to solar X-ray flares. The analysis relies on the previously developed method for estimating the ratio between rates of ionization by X-rays qx and ultraviolet radiation qu during flares. We confirmed the existence of a long-term (at least covering the 45-year observation period) increase in the proportion of X-rays in the total ionization rate of the ionospheric E layer, characterized by the ratio qx/q, where q=qx+q. The qx/q ratio is shown to increase throughout the period of interest at a rate independent of the solar activity cycle. There is also no dependence of the qx/q trend rate on the season, latitude (26°–56° N), and longitude (37°–28° E).
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spelling doaj.art-c3f750417eec46929826aa55088016fb2022-12-21T18:20:49ZengINFRA-MSolar-Terrestrial Physics2500-05352022-03-0181515710.12737/stp-81202206LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARESG.V. Givishvili0https://orcid.org/0000-0002-0577-0077L.N. Leshchenko1https://orcid.org/0000-0003-4894-9437Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAS, Moscow, Troitsk, RussiaPushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation RAS, Moscow, Troitsk, RussiaUsing data from ground-based vertical sounding of the ionosphere (VS) at the station Moscow and five Japanese stations for the period from 1969 to 2015, we have examined the long-term response of the E layer to solar X-ray flares. The analysis relies on the previously developed method for estimating the ratio between rates of ionization by X-rays qx and ultraviolet radiation qu during flares. We confirmed the existence of a long-term (at least covering the 45-year observation period) increase in the proportion of X-rays in the total ionization rate of the ionospheric E layer, characterized by the ratio qx/q, where q=qx+q. The qx/q ratio is shown to increase throughout the period of interest at a rate independent of the solar activity cycle. There is also no dependence of the qx/q trend rate on the season, latitude (26°–56° N), and longitude (37°–28° E).https://naukaru.ru/en/nauka/article/45266/viewionospheric e layervertical soundingsolar flareslong-term trend
spellingShingle G.V. Givishvili
L.N. Leshchenko
LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
Solar-Terrestrial Physics
ionospheric e layer
vertical sounding
solar flares
long-term trend
title LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
title_full LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
title_fullStr LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
title_full_unstemmed LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
title_short LONG-TERM TREND OF THE IONOSPHERIC E-LAYER RESPONSE TO SOLAR FLARES
title_sort long term trend of the ionospheric e layer response to solar flares
topic ionospheric e layer
vertical sounding
solar flares
long-term trend
url https://naukaru.ru/en/nauka/article/45266/view
work_keys_str_mv AT gvgivishvili longtermtrendoftheionosphericelayerresponsetosolarflares
AT lnleshchenko longtermtrendoftheionosphericelayerresponsetosolarflares