Measuring the magnetic field of a trans-equatorial loop system using coronal seismology (Corrigendum)

D. M. Long; G. Valori; D. Pérez–Suárez; R. J. Morton; A. M. Vásquez

doi:10.1051/0004-6361/201730413e

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Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 607, November 2017


Article Number		C3
Number of page(s)		1
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361/201730413e
Published online		16 November 2017

A&A 607, C3 (2017)

Measuring the magnetic field of a trans-equatorial loop system using coronal seismology (Corrigendum)

D. M. Long¹, G. Valori¹, D. Pérez–Suárez¹, R. J. Morton² and A. M. Vásquez³^,4

¹ UCL–Mullard Space Science Laboratory, Holmbury House, Holmbury St. Mary, Dorking, Surrey, RH5 6NT, UK
e-mail: david.long@ucl.ac.uk
² Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, NE1 8ST, UK
³ Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Buenos Aires, Argentina
⁴ Facultad de Ciencias Exactas y Naturales (FCEN), UBA, Buenos Aires, Argentina

This article has no abstract.

Key words: Sun: corona / Sun: magnetic fields / Sun: oscillations / errata, addenda

Erratum to: A&A 603, A101 (2017), DOI: 10.1051/0004-6361/201730413

© ESO, 2017

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