Mass of Solar Prominences Estimated from Multi-Wavelength Data
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386730" target="_blank" >RIV/67985815:_____/12:00386730 - isvavai.cz</a>
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
Mass of Solar Prominences Estimated from Multi-Wavelength Data
Original language description
The mass of selected prominences was estimated using their multi-wavelength observations: in H? by the HSFA2 spectrograph of the Ondřejov observatory, in EUV by SoHO/EIT and in the soft X-rays by Hinode XRT. The results are compared with values estimatedby other authors.
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
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)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Hinode-3: The 3rd Hinode Science Meeting
ISBN
9781583817902
ISSN
—
e-ISSN
—
Number of pages
4
Pages from-to
117-120
Publisher name
Astronomical Society otf the Pacific
Place of publication
San Francisco
Event location
Tokyo
Event date
Dec 1, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
—