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

机译：PROSPIA-3外部掩盖日冕仪ASPIICS的最新成果。

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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.
机译：本文介绍了太阳日冕仪ASPIICS的当前状态，这是ESA编队在轨飞行演示任务PROBA-3的主要有效载荷。仍然很难以足够的空间分辨率和灵敏度来观察太阳日冕的“声区”，以至足以了解控制静态日冕的精细尺度现象以及导致影响空间的日冕物质抛射（CME）的现象。天气。在这方面的改进要求在长时间的观察时间内出现类似日食的情况。迄今为止，飞行的星载日冕仪提供了对日冕外部的连续覆盖，但是它们的超掩星系统无法分析白光日冕中主要日冕物质所集中的部分。 PROBA-3日冕仪系统，也称为ASPIICS（太阳电晕的极化和成像研究航天器协会），被设计为经典的外部潜伏的Lyot日冕仪，但是它利用了将外部隐匿者放置在卫星上的机会。相伴航天器，相距约150m，用于对太阳内部日冕进行高分辨率成像，成像范围接近〜1.1太阳半径。图像将在地面上进行平铺和压缩后再向下链接到地面，以进行科学分析。 ASPIICS由一个大型的欧洲财团建造，该财团由来自7个国家的约20个合作伙伴在欧洲航天局的主持下进行建造。本文正在审查ASPIICS仪器接近CDR时的最新发展状况。

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