日出 III：天文台与仪器概览
摘要
2024 年 7 月，日出 III 成功完成第三次科学飞行。日出 III 天文台在2009 年和2013 年的两次成功飞行后进行了显著升级。三个全新的仪器专注于从可观测光谱层到色素层高度的小尺度物理过程及其复杂相互作用。探索之前 poorly 探索的光谱区域和线，构建对太阳大气层的三维图景，具有前所未有的完整性和细节水平。所有三个仪器都捕获完整的偏振信息，以揭示磁场与流体力学过程之间的相互作用。两个基于孔道的光谱偏振仪器，日出紫外光谱偏振仪器与成像仪 (SUSI) 和日出染色体红外光谱偏振仪器 (SCIP)，分别聚焦于近紫外和近红外区域；可调磁力仪 (TuMag) 同时获取可见光中光场全景 Mm 的photosphere 和 chromosphere 的图图。仪器以编排模式运行，受益于新的 Image Stabilization and Light Distribution unit (ISLiD) 的帮助， Correlating Wavefront Sensor (CWS) 提供自动焦距控制，图像稳定性小于 0.005 英寸的均方根值。新建造的吊舱显著改善了天文台指向稳定性，这是实现持续数小时观测所必需的。日出 III 于 2024 年 7 月 10 日从挪威 Kiruna 附近的 Esrange 太空中心成功发射。飞行持续 6.5 天后，抵达加拿大 Mackenzie 河与 Great Bear Lake 之间 between landing site。本文提供日出 III 天文台及其仪器的概览。
引用
@article{arxiv.2502.06483,
title = {Sunrise III: Overview of Observatory and Instruments},
author = {Andreas Korpi-Lagg and Achim Gandorfer and Sami K. Solanki and Jose Carlos del Toro Iniesta and Yukio Katsukawa and Pietro Bernasconi and Thomas Berkefeld and Alex Feller and Tino L. Riethmüller and Alberto Álvarez-Herrero and Masahito Kubo and Valentín Martínez Pillet and H. N. Smitha and David Orozco Suárez and Bianca Grauf and Michael Carpenter and Alexander Bell and María-Teresa Álvarez-Alonso and Daniel Álvarez García and Beatriz Aparicio del Moral and Daniel Ayoub and Francisco Javier Bailén and Eduardo Bailón Martínez and Maria Balaguer Jiménez and Peter Barthol and Montserrat Bayon Laguna and Luis R. Bellot Rubio and Melani Bergmann and Julian Blanco Rodríguez and Jan Bochmann and Juan Manuel Borrero and Antonio Campos-Jara and Juan Sebastián Castellanos Durán and María Cebollero and Aitor Conde Rodríguez and Werner Deutsch and Harry Eaton and Ana Belen Fernández-Medina and German Fernandez-Rico and Agustin Ferreres and Andrés García and Ramón María García Alarcia and Pilar García Parejo and Daniel Garranzo-García and José Luis Gasent Blesa and Karin Gerber and Dietmar Germerott and David Gilabert Palmer and Laurent Gizon and Miguel Angel Gómez Sánchez-Tirado and David Gonzalez and Alejandro Gonzalo Melchor and Sam Goodyear and Hirohisa Hara and Edvarda Harnes and Klaus Heerlein and Frank Heidecke and Jan Heinrichs and David Hernández Expósito and Johann Hirzberger and Johannes Hoelken and Sangwon Hyun and Francisco A. Iglesias and Ryohtaroh T. Ishikawa and Minwoo Jeon and Yusuke Kawabata and Martin Kolleck and Hugo Laguna and Julian Lomas and Antonio C. López Jiménez and Paula Manzano and Takuma Matsumoto and David Mayo Turrado and Thimo Meierdierks and Stefan Meining and Markus Monecke and José Miguel Morales-Fernández and Antonio Jesús Moreno Mantas and Alejandro Moreno Vacas and Marc Ferenc Müller and Reinhard Müller and Yoshihiro Naito and Eiji Nakai and Armonía Núñez Peral and Takayoshi Oba and Geoffrey Palo and Isabel Pérez-Grande and Javier Piqueras Carreño and Tobias Preis and Damien Przybylski and Carlos Quintero Noda and Sandeep Ramanath and Jose Luis Ramos Más and Nour Raouafi and María-Jesús Rivas-Martínez and Pedro Rodríguez Martínez and Manuel Rodríguez Valido and Basilio Ruiz Cobo and Antonio Sánchez Rodríguez and Antonio Sánchez Gómez and Esteban Sanchis Kilders and Kamal Sant and Pablo Santamarina Guerrero and Erich Schulze and Toshifumi Shimizu and Manuel Silva-López and Azaymi L. Siu-Tapia and Thomas Sonner and Jan Staub and Hanna Strecker and Angel Tobaruela and Ignacio Torralbo and Alexandra Tritschler and Toshihiro Tsuzuki and Fumihiro Uraguchi and Reiner Volkmer and Angelos Vourlidas and Dušan Vukadinović and Stephan Werner and Andreas Zerr},
journal= {arXiv preprint arXiv:2502.06483},
year = {2025}
}
备注
74 pages, 26 figures. Published as part of the Solar Physics Topical Collection "The Sunrise III Solar Observatory" (https://link.springer.com/collections/jegdciedig)