Erratum: Redefining flux ropes in heliophysics

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doi:10.3389/fspas.2023.1212561

ERRATUM article

Front. Astron. Space Sci. , 09 May 2023

Sec. Space Physics

Volume 10 - 2023 | https://doi.org/10.3389/fspas.2023.1212561

This article is part of the Research Topic The Future of Space Physics 2022 View all 66 articles

Erratum: Redefining flux ropes in heliophysics

This article is an erratum on:

Redefining flux ropes in heliophysics
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An Erratum on
Redefining flux ropes in heliophysics

by Nieves-Chinchilla T, Pal S, Salman TM, Carcaboso F, Guidoni SE, Cremades H, Narock A, Balmaceda LA, Lynch BJ, Al-Haddad N, Rodríguez-García L, Narock TW, Dos Santos LFG, Regnault F, Kay C, Winslow RM, Palmerio E, Davies EE, Scolini C, Weiss AJ, Alzate N, Jeunon M and Pujadas R (2023). Front. Astron. Space Sci. 10:1114838. doi: 10.3389/fspas.2023.1114838

Due to a production error, we failed to update “Figure 1” to this newer version provided to us. The publisher apologizes for this mistake. The original version of this article has been updated.

FIGURE 1

FIGURE 1. Example featuring the process of connecting the remote-sensing observations (from STEREO/EUVI and STEREO/COR2 and COR1) of a FR (left) and its local in-situ measurements (right) to infer the global internal structure and heliospheric evolution (middle). The two top images are reproduced from Nieves-Chinchilla et al. (2020) and the bottom cartoon is an adapted version of the Figure 4.5 in Carcaboso Morales (2021).

Keywords: sun, heliosphere, magnetic field, flux rope, coronal mass ejection, solar wind

Citation: Frontiers Production Office (2023) Erratum: Redefining flux ropes in heliophysics. Front. Astron. Space Sci. 10:1212561. doi: 10.3389/fspas.2023.1212561

Received: 26 April 2023; Accepted: 26 April 2023;
Published: 09 May 2023.

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Erratum: Redefining flux ropes in heliophysics

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