Design status of ASPIICS, an externally occulted coronagraph for PROBA-3

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389021%3A_____%2F15%3A00458300" target="_blank" >RIV/61389021:_____/15:00458300 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1117/12.2186962" target="_blank" >http://dx.doi.org/10.1117/12.2186962</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/12.2186962" target="_blank" >10.1117/12.2186962</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Design status of ASPIICS, an externally occulted coronagraph for PROBA-3

Popis výsledku v původním jazyce

The sonic region of the Sun corona remains extremely difficult to observe with spatial resolution and sensitivity sufficient to understand the fine scale phenomena that govern the quiescent solar corona, as well as phenomena that lead to coronal mass ejections (CMEs), which influence space weather. Improvement on this front requires eclipse-like conditions over long observation times. The space-borne coronagraphs flown so far provided a continuous coverage of the external parts of the corona but their over-occulting system did not permit to analyse the part of the white-light corona where the main coronal mass is concentrated. The proposed PROBA-3 Coronagraph System, also known as ASPIICS (Association of Spacecraft for Polarimetric and Imaging Investigation of the Corona of the Sun), with its novel design, will be the first space coronagraph to cover the range of radial distances between similar to 1.08 and 3 solar radii where the magnetic field plays a crucial role in the coronal dyna

Název v anglickém jazyce

Design status of ASPIICS, an externally occulted coronagraph for PROBA-3

Popis výsledku anglicky

The sonic region of the Sun corona remains extremely difficult to observe with spatial resolution and sensitivity sufficient to understand the fine scale phenomena that govern the quiescent solar corona, as well as phenomena that lead to coronal mass ejections (CMEs), which influence space weather. Improvement on this front requires eclipse-like conditions over long observation times. The space-borne coronagraphs flown so far provided a continuous coverage of the external parts of the corona but their over-occulting system did not permit to analyse the part of the white-light corona where the main coronal mass is concentrated. The proposed PROBA-3 Coronagraph System, also known as ASPIICS (Association of Spacecraft for Polarimetric and Imaging Investigation of the Corona of the Sun), with its novel design, will be the first space coronagraph to cover the range of radial distances between similar to 1.08 and 3 solar radii where the magnetic field plays a crucial role in the coronal dyna

Druh

D - Stať ve sborníku

CEP obor

JA - Elektronika a optoelektronika, elektrotechnika

OECD FORD obor

—

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2015

Kód důvěrnosti údajů

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

Název statě ve sborníku

Proceedings of SPIE Vol. 9604:Solar Physics and Space Weather Instrumentation VI

ISBN

978-1-62841-770-8

ISSN

0277-786X

e-ISSN

—

Počet stran výsledku

15

Strana od-do

"96040A"-"96040A"

Název nakladatele

SPIE

Místo vydání

Bellingham

Místo konání akce

San Diego

Datum konání akce

9. 8. 2015

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000366021400008