ASHI:全天空日光层成像仪:2022年8月22日至26日,NASA气球飞行和图像数据简化分析

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Bernard V. Jackson, Matthew Bracamontes, Andrew Buffington, Stuart Volkow, Stephen White, Mario M. Bisi, Edward Stephan, Philippe Leblanc, Ron Quillin
{"title":"ASHI:全天空日光层成像仪:2022年8月22日至26日,NASA气球飞行和图像数据简化分析","authors":"Bernard V. Jackson,&nbsp;Matthew Bracamontes,&nbsp;Andrew Buffington,&nbsp;Stuart Volkow,&nbsp;Stephen White,&nbsp;Mario M. Bisi,&nbsp;Edward Stephan,&nbsp;Philippe Leblanc,&nbsp;Ron Quillin","doi":"10.1007/s11207-025-02448-6","DOIUrl":null,"url":null,"abstract":"<div><p>We have conceived, designed, and evaluated components for an All Sky Heliospheric Imager (ASHI), suitable for flight on future space missions both in Earth orbit and in deep space. ASHI was tested in the summer of 2022 on a NASA-sponsored topside balloon flight; in this paper, we highlight the images taken and the current state of the data reduction from this instrument’s successful overnight flight. The data reduction involves the removal of starlight, zodiacal light, and atmospheric glow to enable the measurements of the outward flow of heliospheric structures. A key photometric specification for ASHI is better than 0.05% differential photometry in one-degree sky bins at 90° elongation. The ASHI balloon flight exceeded expectations and reached to a background white light level of small-scale solar wind structure variations beyond ∼ 60° from the Sun considerably lower than this. Used as a simple, light weight (∼ 8 kg) and relatively inexpensive spaceflight instrument, ASHI has the principal objective of providing a minute-by-minute and day-by-day near real time acquisition of precision Thomson-scattering photometric maps of the inner heliosphere over nearly a hemisphere of sky starting a few degrees from the Sun. This has large potential benefits for improving space-weather nowcast and forecast capabilities of small heliospheric structures.</p></div>","PeriodicalId":777,"journal":{"name":"Solar Physics","volume":"300 3","pages":""},"PeriodicalIF":2.7000,"publicationDate":"2025-03-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s11207-025-02448-6.pdf","citationCount":"0","resultStr":"{\"title\":\"ASHI: The All Sky Heliospheric Imager: August 22 – 26, 2022, NASA Balloon Flight and Image Data Reduction Analysis\",\"authors\":\"Bernard V. Jackson,&nbsp;Matthew Bracamontes,&nbsp;Andrew Buffington,&nbsp;Stuart Volkow,&nbsp;Stephen White,&nbsp;Mario M. Bisi,&nbsp;Edward Stephan,&nbsp;Philippe Leblanc,&nbsp;Ron Quillin\",\"doi\":\"10.1007/s11207-025-02448-6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>We have conceived, designed, and evaluated components for an All Sky Heliospheric Imager (ASHI), suitable for flight on future space missions both in Earth orbit and in deep space. ASHI was tested in the summer of 2022 on a NASA-sponsored topside balloon flight; in this paper, we highlight the images taken and the current state of the data reduction from this instrument’s successful overnight flight. The data reduction involves the removal of starlight, zodiacal light, and atmospheric glow to enable the measurements of the outward flow of heliospheric structures. A key photometric specification for ASHI is better than 0.05% differential photometry in one-degree sky bins at 90° elongation. The ASHI balloon flight exceeded expectations and reached to a background white light level of small-scale solar wind structure variations beyond ∼ 60° from the Sun considerably lower than this. Used as a simple, light weight (∼ 8 kg) and relatively inexpensive spaceflight instrument, ASHI has the principal objective of providing a minute-by-minute and day-by-day near real time acquisition of precision Thomson-scattering photometric maps of the inner heliosphere over nearly a hemisphere of sky starting a few degrees from the Sun. This has large potential benefits for improving space-weather nowcast and forecast capabilities of small heliospheric structures.</p></div>\",\"PeriodicalId\":777,\"journal\":{\"name\":\"Solar Physics\",\"volume\":\"300 3\",\"pages\":\"\"},\"PeriodicalIF\":2.7000,\"publicationDate\":\"2025-03-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1007/s11207-025-02448-6.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Solar Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s11207-025-02448-6\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s11207-025-02448-6","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

我们已经构思,设计和评估了全天空日光层成像仪(ASHI)的组件,适合在未来的太空任务中在地球轨道和深空飞行。ASHI于2022年夏天在美国宇航局赞助的顶部气球飞行中进行了测试;在本文中,我们重点介绍了该仪器成功的夜间飞行所拍摄的图像和数据缩减的现状。数据缩减包括去除星光、黄道光和大气辉光,以便测量日球层结构的向外流动。在伸长率为90°的1度天空箱中,ASHI的关键光度规格优于0.05%的差分光度。ASHI的气球飞行超出了预期,并达到了距离太阳60°以上的小尺度太阳风结构变化的背景白光水平,远低于这一水平。作为一种简单,重量轻(约8公斤)和相对便宜的航天仪器,ASHI的主要目标是提供每分钟和每天的近实时获取距离太阳几度的天空近一个半球的内日球层的精确汤姆森散射光度图。这对于提高空间天气临近预报和小型日球层结构的预报能力有很大的潜在好处。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
ASHI: The All Sky Heliospheric Imager: August 22 – 26, 2022, NASA Balloon Flight and Image Data Reduction Analysis

We have conceived, designed, and evaluated components for an All Sky Heliospheric Imager (ASHI), suitable for flight on future space missions both in Earth orbit and in deep space. ASHI was tested in the summer of 2022 on a NASA-sponsored topside balloon flight; in this paper, we highlight the images taken and the current state of the data reduction from this instrument’s successful overnight flight. The data reduction involves the removal of starlight, zodiacal light, and atmospheric glow to enable the measurements of the outward flow of heliospheric structures. A key photometric specification for ASHI is better than 0.05% differential photometry in one-degree sky bins at 90° elongation. The ASHI balloon flight exceeded expectations and reached to a background white light level of small-scale solar wind structure variations beyond ∼ 60° from the Sun considerably lower than this. Used as a simple, light weight (∼ 8 kg) and relatively inexpensive spaceflight instrument, ASHI has the principal objective of providing a minute-by-minute and day-by-day near real time acquisition of precision Thomson-scattering photometric maps of the inner heliosphere over nearly a hemisphere of sky starting a few degrees from the Sun. This has large potential benefits for improving space-weather nowcast and forecast capabilities of small heliospheric structures.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信