Is the Relation Between Ionospheric Parameters and Solar Proxies Stable?

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F19%3A00518979" target="_blank" >RIV/68378289:_____/19:00518979 - isvavai.cz</a>

Výsledek na webu

<a href="https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019GL085033" target="_blank" >https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019GL085033</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1029/2019GL085033" target="_blank" >10.1029/2019GL085033</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Is the Relation Between Ionospheric Parameters and Solar Proxies Stable?

Popis výsledku v původním jazyce

The relationship between ionospheric parameters and solar activity proxies is important for long‐term studies as ionospheric climatology or long‐term trends and for modeling. It has been broadly assumed that this relationship is stable with time. Using foF2 and foE of four European stations with long (1976–2014) data series, Juliusruh, Pruhonice, Rome, and Slough/Chilton, we show that it is not quite correct assumption. The dependence of yearly average values of ionospheric parameters on solar activity proxies appears to be steeper in 1996–2014 than in 1976–1995 for foF2 and steeper after 2000 for foE. Also, the relationships among solar activity proxies seem to change. Yearly values of foF2 and foE are very predominantly controlled by solar activity represented by proxies.

Název v anglickém jazyce

Is the Relation Between Ionospheric Parameters and Solar Proxies Stable?

Popis výsledku anglicky

The relationship between ionospheric parameters and solar activity proxies is important for long‐term studies as ionospheric climatology or long‐term trends and for modeling. It has been broadly assumed that this relationship is stable with time. Using foF2 and foE of four European stations with long (1976–2014) data series, Juliusruh, Pruhonice, Rome, and Slough/Chilton, we show that it is not quite correct assumption. The dependence of yearly average values of ionospheric parameters on solar activity proxies appears to be steeper in 1996–2014 than in 1976–1995 for foF2 and steeper after 2000 for foE. Also, the relationships among solar activity proxies seem to change. Yearly values of foF2 and foE are very predominantly controlled by solar activity represented by proxies.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10509 - Meteorology and atmospheric sciences

Projekt

<a href="/cs/project/GA18-01625S" target="_blank" >GA18-01625S: Vliv skleníkových plynů a dalších zdrojů na dlouhodobé trendy v systému stratosféra-mezosféra-termosféra-ionosféra</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2019

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Geophysical Research Letters

ISSN

0094-8276

e-ISSN

—

Svazek periodika

46

Číslo periodika v rámci svazku

24

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

6

Strana od-do

14208-14213

Kód UT WoS článku

000503155100001

EID výsledku v databázi Scopus

2-s2.0-85077093986