Large-scale magnetic field evolution on different time scales.

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F02%3A01020179" target="_blank" >RIV/67985815:_____/02:01020179 - 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

Large-scale magnetic field evolution on different time scales.

Original language description

Horizontal transport of large-scale magnetic field in coarse of last three solar activity cycles was studied. A non-homogeneous transport of the magnetic flux over the solar sphere, superposed on the global differential rotation and meridional circulation was revealed. Long term relationship between cyclic variations of the velocity parameters and the magnetic flux values is discussed.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

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

2002

Confidentiality

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

Article name in the collection

Solar variability: from core to outer frontiers.

ISBN

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ISSN

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e-ISSN

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Number of pages

4

Pages from-to

827-830

Publisher name

ESA Publication Division

Place of publication

Noordwijk

Event location

Praha [CZ]

Event date

Sep 9, 2002

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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