MRI: Development of an Airborne Stabilized Platform for InfraRed Experiments (ASPIRE)

MRI：开发用于红外实验的机载稳定平台 (ASPIRE)

• 批准号: 1919809
• 负责人: Jenna Samra
• 金额: $ 69.8万
• 依托单位: Smithsonian Institution Astrophysical Observatory
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-08-15 至 2022-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1919809&HistoricalAwards=false
• 关键词: MRI; Development; Airborne; Stabilized; Platform

The main purpose of this three-year MRI project is to design and build a solar-tracking platform for the NSF/NCAR Gulfstream-V (GV) aircraft, and demonstrate its capabilities by flying two focal plane instruments during the 2020 total solar eclipse across South America. The Airborne Stabilized Platform for InfraRed Experiments (ASPIRE) builds on the success of the Airborne InfraRed Spectrometer (AIR-Spec), turning the GV into a solar-viewing platform for rapid prototyping of solar and atmospheric instruments. By adding a stabilized solar feed to the GV aircraft, the project team will create an airborne platform for infrared remote sensing that will be a valuable resource for both the solar and atmospheric communities. In solar physics, the 20cm feed would enable many applications on and off the solar disk. During the upcoming eclipse mission, for example, the ASPIRE will provide enough throughput to make polarimetric measurements with an airborne version of the Coronal Multichannel Polarimeter (CoMP). The project team will deliver the ASPIRE interface documentation to NSF and NCAR in first quarter 2021. The ASPIRE project will provide research training for at least three REU students at the Smithsonian Institution Astrophysical Observatory (SAO) over its lifetime. The team will involve a Boston-based undergraduate in the ASPIRE development and bring this student to Chile to participate in various EPO activities. Summer test flights in 2020 and 2021 will provide field testing experience for two REU students. Combining a total solar eclipse with the GV research aircraft is an excellent way to captivate public interest. As both the 2019 and 2020 eclipses cross South America, the SAO and NCAR staff will reach out to U.S. Embassy personnel to arrange tours of the unique GV aircraft and give talks on eclipse science.The main goal of this three-year MRI project is to develop the ASPIRE, which will provide a 20cm diameter solar feed, stabilized to 5 arcsec RMS over a 3 second exposure time. The platform is well-suited for infrared investigations of the Sun, as it can operate above the influence of Earth's atmosphere, and for atmospheric measurements of trace gases obtained by observing sunlight transmitted through atmospheric absorption bands. The ASPIRE will provide broadband visible and infrared transmission from 0.45 to 10 microns, compatible with all of the GV's IR-transmissive viewports. During its 2020 commissioning flight, ASPIRE will feed a 13cm telescope with two complementary focal plane instruments: AIR-Spec (an imaging spectrometer) and a new narrowband imager centered on the AIR-Spec 1.43 micron Si X line. AIR-Spec was designed to characterize five magnetically sensitive coronal emission lines between 1.4 and 4 microns and assess whether they are useful probes of coronal magnetism. It observed all five of its target lines during the 2017 total solar eclipse, detecting the 2.84 micron Fe IX for the first time. The strong Si X line was observed up to 0.6 solar radii from the limb and provided line-of-sight velocity measurements with a resolution of 5 km/s. The larger telescope aperture enabled by ASPIRE will improve the AIR-Spec SNR by a factor of 1.5 compared to its 2019 observation (6x improvement over 2017), allowing the project team to explore the coronal density and temperature measurements, flows, and oscillations that are on the edge of detection with the current AIR-Spec instrumentation. The Si X context imager will reduce the need for rastering the slit, allowing us to improve SNR by summing 'sit and stare' slit data for more than a minute. The research and EPO agenda of this project supports the Strategic Goals of the AGS Division in discovery, learning, diversity, and interdisciplinary research.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

这个为期三年的 MRI 项目的主要目的是为 NSF/NCAR Gulfstream-V (GV) 飞机设计和建造一个太阳跟踪平台，并通过在 2020 年日全食期间飞行两台焦平面仪器来展示其能力。南美洲。 机载红外实验稳定平台 (ASPIRE) 建立在机载红外光谱仪 (AIR-Spec) 的成功基础上，将 GV 转变为太阳观测平台，用于太阳和大气仪器的快速原型设计。 通过为 GV 飞机添加稳定的太阳能馈源，项目团队将创建一个用于红外遥感的机载平台，这将成为太阳能和大气界的宝贵资源。 在太阳物理学中，20 厘米的馈源将使太阳盘内外的许多应用成为可能。 例如，在即将到来的日食任务中，ASPIRE 将提供足够的吞吐量，以便使用机载版本的日冕多通道旋光计 (CoMP) 进行旋光测量。 项目团队将于 2​​021 年第一季度向 NSF 和 NCAR 提供 ASPIRE 接口文档。ASPIRE 项目将在其生命周期内为史密森学会天体物理观测站 (SAO) 的至少三名 REU 学生提供研究培训。 该团队将让一名波士顿的本科生参与 ASPIRE 的开发，并将该学生带到智利参加各种 EPO 活动。 2020 年和 2021 年的夏季试飞将为两名 REU 学生提供现场测试经验。 将日全食与 GV 研究飞机结合起来是吸引公众兴趣的绝佳方式。 随着 2019 年和 2020 年日食穿越南美洲，SAO 和 NCAR 工作人员将与美国大使馆人员联系，安排参观独特的 GV 飞机并就日食科学进行讲座。这个为期三年的 MRI 项目的主要目标是开发 ASPIRE，它将提供直径 20 厘米的太阳能馈电，在 3 秒曝光时间内稳定至 5 弧秒 RMS。 该平台非常适合对太阳进行红外研究，因为它可以在地球大气层的影响之外运行，并且可以通过观察透过大气吸收带的阳光来获得痕量气体的大气测量。 ASPIRE 将提供 0.45 至 10 微米的宽带可见光和红外传输，与 GV 的所有红外传输视口兼容。 在 2020 年调试飞行期间，ASPIRE 将为 13 厘米望远镜提供两个互补的焦平面仪器：AIR-Spec（成像光谱仪）和以 AIR-Spec 1.43 微米 Si X 线为中心的新型窄带成像仪。 AIR-Spec 旨在表征 1.4 至 4 微米之间的 5 个磁敏日冕发射线，并评估它们是否是日冕磁性的有用探针。 它在 2017 年日全食期间观测了所有 5 条目标线，首次探测到 2.84 微米的 Fe IX。 在距肢体 0.6 个太阳半径的范围内观测到强 Si X 线，并提供分辨率为 5 km/s 的视线速度测量结果。与 2019 年的观测相比，ASPIRE 实现的更大望远镜孔径将使 AIR-Spec 信噪比提高 1.5 倍（比 2017 年提高 6 倍），使项目团队能够探索日冕密度和温度测量、流动和振荡。处于当前 AIR-Spec 仪器检测的边缘。 Si X 上下文成像仪将减少对狭缝进行光栅化的需要，使我们能够通过对一分钟多的“坐着凝视”狭缝数据进行求和来提高信噪比。 该项目的研究和 EPO 议程支持 AGS 部门在发现、学习、多样性和跨学科研究方面的战略目标。该奖项反映了 NSF 的法定使命，并通过使用基金会的智力价值和更广泛的影响进行评估，被认为值得支持审查标准。