Front. Astron. Space Sci. Frontiers in Astronomy and Space Sciences Front. Astron. Space Sci. 2296-987X Frontiers Media S.A. 1197352 10.3389/fspas.2023.1197352 Astronomy and Space Sciences Correction Corrigendum: Magnetic field reconstruction for a realistic multi-point, multi-scale spacecraft observatory Broeren et al. 10.3389/fspas.2023.1197352 Broeren T. 1 * Klein K. G. 2 TenBarge J. M. 3 Dors Ivan 4 Roberts O. W. 4 Verscharen D. 5 6 1 Department of Applied Mathematics, University of Arizona, Tucson, AZ, United States 2 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, United States 3 Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ, United States 4 Space Research Institute, Austrian Academy of Sciences, Graz, Austria 5 Mullard Space Science Laboratory, University College London, Surrey, United Kingdom 6 Space Science Center, University of New Hampshire, Durham, NH, United States

Edited and reviewed by: Georgios Balasis, National Observatory of Athens, Greece

 *Correspondence: T. Broeren, broeren@email.arizona.edu 24 10 2023 2023 10 1197352 30 03 2023 02 08 2023 Copyright © 2023 Broeren, Klein, TenBarge, Dors, Roberts and Verscharen. 2023 Broeren, Klein, TenBarge, Dors, Roberts and Verscharen

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 A Corrigendum on Magnetic field reconstruction for a realistic multi-point, multi-scale spacecraft observatory by Broeren T, Klein KG, TenBarge JM, Dors I, Roberts OW and Verscharen D (2021). Front. Astron. Space Sci. 8:727076. doi: 10.3389/fspas.2021.727076 plasma physics magnetic fields spacecraft vector field reconstruction space physics curlometer space mission analysis multi-spacecraft analysis section-at-acceptance Space Physics

In the published article, there was an error in Figures 8–10. The word “Turbulence” was misspelled in all these figures titles as “Trubulance”. Additionally in Figure 8, in this six-panel figure, the bottom-left panel was a duplicate of the top-right panel. The correct bottom-left panel has the title “ M 1.4 Reconstruction”.

Computation error (defined in Eq. 7) at all points on the z = 0 plane of the turbulent magnetic field (from the Gkeyll Simulation), using the swarm configuration at hour 94 of the HelioSwarm DRM. The layout is identical to Figure 4.

Computation error (defined in Eq. 7) at all points on the z = 0 plane of the turbulent magnetic field (from the Gkeyll Simulation), using the swarm configuration at hour 144 of the HelioSwarm DRM. The layout is identical to Figure 4.

Computation error (defined in Eq. 7) at all points on the z = 0 plane of the turbulent magnetic field (from the Gkeyll Simulation), using the swarm configuration at hour 205 of the HelioSwarm DRM. The layout is identical to Figure 4.

In the published article, there was an error in Figure 2 as published. The data that was used to generate this figure was slightly mismatched with the data that was used throughout the rest of the paper to carry out the calculations.

Elongation and planarity of the 126 tetrahedron associated with the three nine-spacecraft configurations under consideration, with characteristic lengths shown in color.

The corrected figures appear below.

In the published article, there was a typo in the second paragraph of Section 2.3.2 there is a typo in one of the inline equations (the definition of proton thermal velocity). The correct equation is below: v t p = 2 T p / m p .

Subsequently, a correction has been made to Section 2.3.2, paragraph 2.

The corrected sentence appears below:

“Lengths are normalized to the proton gyroradius ρ p = v t p / Ω p , the ratio of the proton thermal speed v t p = 2 T p / m p and the proton cyclotron frequency Ω p = q p B / m p .”

The authors apologize for these errors and state that this does not change the scientific conclusions of the article in any way. The original article has been updated.

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