Solar flares: observation vs simulations

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00360906" target="_blank" >RIV/67985815:_____/11:00360906 - 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

Solar flares: observation vs simulations

Original language description

In order to study the properties of faint, moderate and bright flares, we simulate the conditions of the solar atmosphere using a radiative hydrodynamic model (Abbett & Hawley, 1999). A constant beam of non-thermal electrons is injected at the apex of a1D coronal loop and heating from thermal soft X-ray emission is included. We compare the results with some observational data in Ly-? (using TRACE 1216 and 1600 A data and estimating the ?pure Ly-? emission) and in H? (data taken with a Multichannel Flare Spectrograph, at the Ondrejov Observatory).

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

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2011

Confidentiality

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

Article name in the collection

Advances in Plasma Astrophysics

ISBN

9780521197410

ISSN

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e-ISSN

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Number of pages

3

Pages from-to

182-184

Publisher name

Cambridge University Press

Place of publication

Cambridge

Event location

Giardini Naxos

Event date

Sep 6, 2010

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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