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Recent achievements on ASPIICS, an externally occulted coronagraph for PROBA-3

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389021%3A_____%2F16%3A00472966" target="_blank" >RIV/61389021:_____/16:00472966 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1117/12.2232695" target="_blank" >http://dx.doi.org/10.1117/12.2232695</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1117/12.2232695" target="_blank" >10.1117/12.2232695</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Recent achievements on ASPIICS, an externally occulted coronagraph for PROBA-3

  • Original language description

    This paper presents the current status of ASPIICS, a solar coronagraph that is the primary payload of ESA’s formation flying in-orbit demonstration mission PROBA-3. 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 PROBA-3 Coronagraph System, also known as ASPIICS (Association of Spacecraft for Polarimetric and Imaging Investigation of the Corona of the Sun) is designed as a classical externally occulted Lyot coronagraph but it takes advantage of the opportunity to place the external occulter on a companion spacecraft, about 150m apart, to perform high resolution imaging of the inner corona of the Sun as close as 1.1 solar radii. The images will be tiled and compressed on board in an FPGA before being down-linked to ground for scientific analyses. ASPIICS is built by a large European consortium including about 20 partners from 7 countries under the auspices of the European Space Agency. This paper is reviewing the recent development status of the ASPIICS instrument as it is approaching CDR

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BH - Optics, masers and lasers

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of SPIE Vol. 9904: Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave

  • ISBN

    978-1-5106-0187-1

  • ISSN

    0277-786X

  • e-ISSN

  • Number of pages

    3

  • Pages from-to

  • Publisher name

    SPIE-INT SOC OPTICAL ENGINEERING

  • Place of publication

    Bellingham

  • Event location

    Edinburg

  • Event date

    Jun 26, 2016

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000385794100097