Sun radio interferometer space experiment (SunRISE): Tracking particle acceleration and transport in the inner heliosphere

F. Alibay, J. Kasper, T. Lazio, T. Neilsen
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引用次数: 15

Abstract

The authors present a space-based array designed to localize and track the radio emission associated with coronal mass ejections (CMEs) from the Sun. Radio emission from CMEs is a direct tracer of the particle acceleration in the inner heliosphere and potential magnetic connections from the lower solar corona to the larger heliosphere. These questions are among those highlighted in the current Solar Decadal Servey, e.g., “Discover and characterize fundamental processes that occur both within the heliosphere and throughout the Universe.” Furthermore, CME radio emission is quite strong, such that only a relatively small number of antennas is required, and a small mission would make a fundamental advancement in our scientific understanding. Indeed, the current state-of-the-art for tracking CME radio emission is defined by single antennas (Wind/WAVES, Stereo/SWAVES) in which the tracking is accomplished by assuming a frequency-to-density mapping. This type of heliophysics mission has been studied several times in the past, but had so far been found to be cost prohibitive, due to the inherent complexity of building multiple spacecraft and flying them in constellation. However, with the increased popularity and success of CubeSat concepts, accompanied by the miniaturization of subsystem components, a range of missions are now being enabled at lower cost than ever before. The paper presents the science requirements for a Small Explorer (SMEX)-class (typically < ∼$100M, including all lifecycle costs) mission concept, and walks through the major features of the SunRISE mission study. SunRISE is composed of six 6U (where 1U is defined as a 10 by 10 by 10cm form-factor) CubeSats placed in an orbit slightly above the Geostationary Equatorial Orbit (GEO) to achieve the aforementioned science goals. The spacecraft fly in a passive formation, which allows them to form an interferometer while minimizing the impact on operations complexity. The paper provides an overview of the mission and spacecraft design, as well as the concept of operations for the mission. Finally, it discusses how the SunRISE mission concept could serve as a stepping stone in demonstrating space-based interferometry and enable more complex mission concepts in the future.
太阳射电干涉仪空间实验(SunRISE):跟踪内日球层的粒子加速和输运
作者提出了一种基于空间的阵列,用于定位和跟踪与太阳日冕物质抛射(cme)相关的无线电发射。日冕物质抛射的射电辐射是内日球层粒子加速和从较低日冕层到较大日球层的潜在磁连接的直接示踪剂。这些问题是当前太阳年代际观测中突出的问题之一,例如,“发现和描述发生在日球层和整个宇宙中的基本过程。”此外,日冕物质抛射的射电辐射非常强,因此只需要相对较少数量的天线,而一个小任务将在我们的科学理解方面取得根本性的进步。事实上,目前跟踪CME射电发射的最先进技术是由单天线(风/波,立体声/波)定义的,其中跟踪是通过假设频率到密度的映射来完成的。这种类型的太阳物理任务在过去已经研究了几次,但到目前为止,由于建造多个航天器并在星座中飞行的固有复杂性,被发现成本过高。然而,随着立方体卫星概念的日益普及和成功,伴随着子系统组件的小型化,一系列任务现在以比以往更低的成本实现。本文提出了小型探索者(SMEX)级(通常< ~ 1亿美元,包括所有生命周期成本)任务概念的科学要求,并介绍了SunRISE任务研究的主要特征。SunRISE由6颗6U(其中1U被定义为10 × 10 × 10cm的尺寸)立方体卫星组成,放置在地球静止赤道轨道(GEO)略高于地球静止赤道轨道(GEO)的轨道上,以实现上述科学目标。航天器以被动编队飞行,这使它们能够形成干涉仪,同时最大限度地减少对操作复杂性的影响。本文提供了任务和航天器设计的概述,以及任务的操作概念。最后,它讨论了SunRISE任务概念如何作为展示天基干涉测量的垫脚石,并在未来实现更复杂的任务概念。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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