Frontiers Production OfficeAn 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. 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.
Approved by:
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