5 research outputs found

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

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    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 ~1.08 and 3 solar radii where the magnetic field plays a crucial role in the coronal dynamics, thus providing continuous observational conditions very close to those during a total solar eclipse. PROBA-3 is first a mission devoted to the in-orbit demonstration of precise formation flying techniques and technologies for future European missions, which will fly ASPIICS as primary payload. The instrument is distributed over two satellites flying in formation (approx. 150m apart) to form a giant coronagraph capable of producing a nearly perfect eclipse allowing observing the sun corona closer to the rim than ever before. The coronagraph instrument is developed 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 improvements and design updates of the ASPIICS instrument as it is stepping into the detailed design phase

    East Europe\u27s cinema industries since 1989: financing structure and studios

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    Desetletne izkušnje vzhodnoevropske tranzicije je mogoče povzeti v nekaj temeljnih ugotovitvah o viharnem in globokem preoblikovanju kulturn administracije. Vzhodnoevropska kulturna industrija je bila v začetku devetdesetih let prva izpostavljena velikemu zmanjšanju sredstev in odpravi vnaprej zagotovljenega financiranja. Še posebej je bil prizadet film. V vseh vzhodnoevropskih državah je bila filmska proizvodnja podvržena nepremišljenim strukturnim spremembam ter pogosto protislovnim ukrepom v upravljanju in financiranju. Drobljenje proizvodnih postopkov je pri mnogih povzročilo ustvarjalno krizo. Značilni problemi so nepoštena konkurenca, poglabljanje generacijskega prepada ter zaton celovečernih, dokumentarnih in animiranih filmov. Hkratna kriza v filmski distribuciji in prikazovanju je pripeljala do upadanja števila gledalcev vseh vzhodnoevropskih filmov, čeprav so hkrati nekateri vzhodnoevropski filmi poželi mednarodna priznanja. Spremembe v vzhodnoevropskem filmu so potekale v obodbju negotovosti zahodnoevropskih kulturnih politik, ki so jih vodila vse bolj protiameriška čustva. Nastanek investicijskih skladov, kot sta Media 95 in Euroimage, je bil reakcija na triumf komercialnega filma. Pod vplivom prevlade ideje "novega evropskega filma" nad "nacionalnim filmom" so se povečale tudi subvencije v vzhodnoevropske studie. Članek podrobneje obravnava spremembe v vzhodnoevropski filmski proizvodnji, konec nacionalnih kinematografij, probleme koprodukcij, zlasti v povezavi z Evroimage, komercialno financiranje,odnos med domačo in tujo filmsko distribucijo in prikazovanjem ter filmske festivale.The decade worth of the East European transition allows us to sum up important lessons of the stormy and profound transformation in cultural administration. The East European cultural industries were the first ones to suffer massive cuts and withdrawal of secure funding early in the 1990s. Cinema was affected most notably. In all of the East European countries filmmaking underwent volatile structural changes and was subjected to often contradictory undertakings in administration and financing. The crumbling production routines caused a creativity crisis in many filmmakers. Problems included unfair competition, deepening generation gap, and decline in feature,documentary and animation output. The concurrent crisis in distribution and exhibition led to a sharp drop in box office indicators for all productions carrying an East European label. At the same time some East European films enjoyed an international critical acclaim internationally. The volatility in East European cinema coincided with a clearly articulated period of insecurity in West European cultural policies, driven by a growing anti-American sentiment. The establishment of such pan-European funding bodies as Media 95 and Euroimage came as a reaction to the overwhelming triumphof commercialism in cinema. The share of international subsidies for filmmaking in poverty-stricken Eastern European studios quickly increased as the concept of "national cinema" gave way to a "new European" one. The article focuses on the following topics: changes in East European production schemes, the end of national cinemas, issues of co-producing with focus on Euroimage, media and commercial financing, the questions of domestic versus foreign film distribution and exhibition, and festivals

    ASPIICS: an externally occulted coronagraph for PROBA-3. Design evolution

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    PROBA-3 is a mission devoted to the in-orbit demonstration of precise formation flying techniques and technologies for future ESA missions. PROBA-3 will fly ASPIICS (Association de Satellites pour l’Imagerie et l’Interferometrie de la Couronne Solaire) as primary payload, which makes use of the formation flying technique to form a giant coronagraph capable of producing a nearly perfect eclipse allowing to observe the sun corona closer to the rim than ever before. The coronagraph is distributed over two satellites flying in formation (approx. 150m apart). The so called Coronagraph Satellite carries the camera and the so called Occulter Satellite carries the sun occulter disc. This paper is reviewing the design and evolution of the ASPIICS instrument as at the beginning of Phase C/D

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

    No full text
    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 dynamics, thus providing continuous observational conditions very close to those during a total solar eclipse. PROBA-3 is first a mission devoted to the in-orbit demonstration of precise formation flying techniques and technologies for future European missions, which will fly ASPIICS as primary payload. The instrument is distributed over two satellites flying in formation (approx. 150m apart) to form a giant coronagraph capable of producing a nearly perfect eclipse allowing observing the sun corona closer to the rim than ever before. The coronagraph instrument is developed 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 improvements and design updates of the ASPIICS instrument as it is stepping into the detailed design phase
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