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HelioSwarm: a multipoint, multiscale mission to characterize turbulence
| File | Description | Size | Format | |
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 s11214-023-01019-0.pdf | Published version | 3.25 MB | Adobe PDF | View/Open |
| Title: | HelioSwarm: a multipoint, multiscale mission to characterize turbulence |
| Authors: | Klein, KG Spence, H Alexandrova, O Argall, M Arzamasskiy, L Bookbinder, J Broeren, T Caprioli, D Case, A Chandran, B Chen, L-J Dors, I Eastwood, J Forsyth, C Galvin, A Genot, V Halekas, J Hesse, M Hine, B Horbury, T Jian, L Kasper, J Kretzschmar, M Kunz, M Lavraud, B Le Contel, O Mallet, A Maruca, B Matthaeus, W Niehof, J O’Brien, H Owen, C Retinò, A Reynolds, C Roberts, O Schekochihin, A Skoug, R Smith, C Smith, S Steinberg, J Stevens, M Szabo, A TenBarge, J Torbert, R Vasquez, B Verscharen, D Whittlesey, P Wickizer, B Zank, G Zweibel, E |
| Item Type: | Journal Article |
| Abstract: | HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at nine spacecraft with separations spanning magnetohydrodynamic and sub-ion spatial scales in a variety of near-Earth plasmas. In this paper, we describe the scientific background for the HS investigation, the mission goals and objectives, the observatory reference trajectory and instrumentation implementation before the start of Phase B. Through multipoint, multiscale measurements, HS promises to reveal how energy is transferred across scales and boundaries in plasmas throughout the universe. |
| Issue Date: | Dec-2023 |
| Date of Acceptance: | 14-Oct-2023 |
| URI: | http://hdl.handle.net/10044/1/108345 |
| DOI: | 10.1007/s11214-023-01019-0 |
| ISSN: | 0038-6308 |
| Publisher: | Springer |
| Journal / Book Title: | Space Science Reviews |
| Volume: | 219 |
| Issue: | 8 |
| Copyright Statement: | © The Author(s) 2023. Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. |
| Publication Status: | Published |
| Article Number: | 74 |
| Online Publication Date: | 2023-11-03 |
| Appears in Collections: | Space and Atmospheric Physics Physics |
This item is licensed under a Creative Commons License
