Empirical modeling of the upper transition height for low and middle latitudes.

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F01%3A04010040" target="_blank" >RIV/68378289:_____/01:04010040 - 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

Empirical modeling of the upper transition height for low and middle latitudes.

Original language description

Ion composition data measured by the Bennett mass spectrometer during the ACTIVE mission (perigee 500 km, apogee 2500 km, maximum of solar cycle 22) and from AE satellites from the minimum of solar cycle 21 was used to study the solar activity influenceon the global behaviour of the upper transition height. In a first approximation the invariant latitude and magnetic local time dependence is considered and described by spherical harmonics up to the 6th order. Submodels for equinox and solstices for high and low solar activity are presented.

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

BL - Plasma physics and discharge through gases

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)

Publication year

2001

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

27

Issue of the periodical within the volume

1

Country of publishing house

GB - UNITED KINGDOM

Number of pages

4

Pages from-to

111-114

UT code for WoS article

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EID of the result in the Scopus database

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