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CATEcor:一种开放科学、阴影桁架、外部遮挡日冕仪。

CATEcor: An Open Science, Shaded-Truss, Externally-Occulted Coronagraph.

作者信息

DeForest Craig, Seaton Daniel B, Caspi Amir, Beasley Matt, Davis Sarah J, Erickson Nicholas F, Kovac Sarah A, Patel Ritesh, Tosolini Anna, West Matthew J

机构信息

Southwest Research Institute, Boulder, CO USA.

Independent Researcher, Boulder, CO USA.

出版信息

Sol Phys. 2024;299(6):78. doi: 10.1007/s11207-024-02314-x. Epub 2024 Jun 10.

DOI:10.1007/s11207-024-02314-x
PMID:38867765
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11164819/
Abstract

We present the design of a portable coronagraph, CATEcor (where CATE stands for Continental-America Telescope Eclipse), that incorporates a novel "shaded-truss" style of external occultation and serves as a proof-of-concept for that family of coronagraphs. The shaded-truss design style has the potential for broad application in various scientific settings. We conceived CATEcor itself as a simple instrument to observe the corona during the darker skies available during a partial solar eclipse, or for students or interested amateurs to detect the corona under ideal noneclipsed conditions. CATEcor is therefore optimized for simplicity and accessibility to the public. It is implemented using an existing dioptric telescope and an adapter rig that mounts in front of the objective lens, restricting the telescope aperture and providing external occultation. The adapter rig, including occulter, is fabricated using fusion deposition modeling (FDM; colloquially "3D printing"), greatly reducing cost. The structure is designed to be integrated with moderate care and may be replicated in a university or amateur setting. While CATEcor is a simple demonstration unit, the design concept, process, and trades are useful for other more sophisticated coronagraphs in the same general family, which might operate under normal daytime skies outside the annular-eclipse conditions used for CATEcor.

摘要

我们展示了一种便携式日冕仪CATEcor(其中CATE代表美洲大陆望远镜日食)的设计,它采用了一种新颖的“阴影桁架”式外部掩星方法,并作为该日冕仪系列的概念验证。阴影桁架设计风格在各种科学环境中具有广泛应用的潜力。我们将CATEcor本身设想为一种简单的仪器,用于在日偏食期间较暗的天空中观测日冕,或者供学生或感兴趣的业余爱好者在理想的非日食条件下探测日冕。因此,CATEcor针对简单性和公众可及性进行了优化。它是通过使用现有的折射望远镜和安装在物镜前方的适配器装置来实现的,该装置限制望远镜孔径并提供外部掩星。包括遮光器在内的适配器装置是使用熔融沉积建模(FDM;通俗地说就是“3D打印”)制造的,大大降低了成本。该结构设计为只需适度小心即可集成,并且可以在大学或业余环境中复制。虽然CATEcor是一个简单的演示装置,但设计概念、过程和权衡对于同一类别的其他更复杂的日冕仪很有用,这些日冕仪可能在CATEcor所使用的日环食条件之外的正常白天天空下运行。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/6b36de3868d7/11207_2024_2314_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/5537ee81fe5b/11207_2024_2314_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/294a14c8e9fa/11207_2024_2314_Fig2_HTML.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/a8128c300096/11207_2024_2314_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/241f68c00912/11207_2024_2314_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/2e97ec7be145/11207_2024_2314_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/0f8b18ea5d33/11207_2024_2314_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/eddff7d62f85/11207_2024_2314_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/2df2709a491a/11207_2024_2314_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/8b31d304f140/11207_2024_2314_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/732c08a0be9b/11207_2024_2314_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/6b36de3868d7/11207_2024_2314_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/5537ee81fe5b/11207_2024_2314_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/294a14c8e9fa/11207_2024_2314_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/11c9c9e4b75e/11207_2024_2314_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/a8128c300096/11207_2024_2314_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/241f68c00912/11207_2024_2314_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/2e97ec7be145/11207_2024_2314_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/0f8b18ea5d33/11207_2024_2314_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/eddff7d62f85/11207_2024_2314_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/2df2709a491a/11207_2024_2314_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/8b31d304f140/11207_2024_2314_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/732c08a0be9b/11207_2024_2314_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/482b/11164819/6b36de3868d7/11207_2024_2314_Fig12_HTML.jpg

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本文引用的文献

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Defining the Middle Corona.定义中日冕。
Sol Phys. 2023;298(6):78. doi: 10.1007/s11207-023-02170-1. Epub 2023 Jun 14.
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New Mauna Loa coronagraph systems.新型莫纳罗亚日冕仪系统。
Appl Opt. 1981 Mar 15;20(6):1094-101. doi: 10.1364/AO.20.001094.