Response of outer ionosphere electron temperature and density to changes in solar activity.

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F03%3A04033515" target="_blank" >RIV/68378289:_____/03:04033515 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Response of outer ionosphere electron temperature and density to changes in solar activity.

Original language description

Manifestation of solar activity variation in the electron temperature (Te) and electron density (Ne) during the solar maxima is studied. Solar activity changes are characterized by the F10.7 index. The Te and Ne response to solar activity changes is characterized by a linear dependence. This dependence, included in an empirical model of Te based on Intercosmos satellites data, is compared with Hinotori (altitude 600km), and ISIS-1 (altitude 2500km) Te data, the best agreement is found at equatorial andlow latitudes. The response of electron density to the 27 day solar flux variation is small.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

DG - Atmospheric sciences, meteorology

OECD FORD branch

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Project

Result was created during the realization of more than one project. More information in the Projects tab.

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2003

Confidentiality

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

Name of the periodical

Advances in space research

ISSN

0273-1177

e-ISSN

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Volume of the periodical

31

Issue of the periodical within the volume

3

Country of publishing house

GB - UNITED KINGDOM

Number of pages

4

Pages from-to

697-700

UT code for WoS article

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EID of the result in the Scopus database

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