Erratum: “On the properties of Alfvénic switchbacks in the expanding solar wind: Three-dimensional numerical simulations” [Phys. Plasmas <b>29</b>, 072902 (2022)]-Reference-Cited by-同舟云学术

Erratum: “On the properties of Alfvénic switchbacks in the expanding solar wind: Three-dimensional numerical simulations” [Phys. Plasmas 29, 072902 (2022)]

Published:2022-12 Issue:12 Volume:29 Page:129902
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Johnston Zade¹^ORCID,Squire Jonathan¹^ORCID,Mallet Alfred²^ORCID,Meyrand Romain¹^ORCID

Affiliation:

1. Physics Department, University of Otago, Dunedin 9010, New Zealand

2. Space Sciences Laboratory, University of California, Berkeley, California 94720, USA

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

https://aip.scitation.org/doi/pdf/10.1063/5.0133296

Reference6 articles.

1. On the properties of Alfvénic switchbacks in the expanding solar wind: Three-dimensional numerical simulations

2. The propagation of Alfv�n waves and their directional anisotropy in the solar wind

3. ALFVÉN WAVE REFLECTION AND TURBULENT HEATING IN THE SOLAR WIND FROM 1 SOLAR RADIUS TO 1 AU: AN ANALYTICAL TREATMENT

4. Experimental constraints on pulsed and steady state models of the solar wind near the Sun

5. More accurately, if one considers the approximate radial solar-wind profile of Ref. 3, χ grows by a modest factor to the maximum in v A then decreases again, leaving its value R A similar to that at the solar surface.

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1. Switchbacks and Associated Magnetic Holes Observed near the Alfvén Critical Surface;The Astrophysical Journal;2023-11-29