Erratum: "Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt" (2023, ApJS, 265, 47)

Jia Huang, J. C. Kasper, Davin E. Larson, Michael D. Mcmanus, P.

Whittlesey, Roberto Livi, Ali Rahmati, Orlando Romeo, K. G. Klein, Weijie
Sun, et al.

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To cite this version:

Jia Huang, J. C. Kasper, Davin E. Larson, Michael D. Mcmanus, P. Whittlesey, et al. Erratum: "Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt" (2023, ApJS, 265, 47). 2024, 10.3847/1538-4365/ad3246 . insu-04833991

HAL Id: insu-04833991

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Submitted on 12 Dec 2024

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# Erratum: “Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt” (2023, ApJS, 265, 47)

Jia Huang<fnref n="1" />, C. Kasper<fnref n="2" />,<fnref n="3" />, Davin E. Larson<fnref n="1" />, Michael D. McManus<fnref n="1" />, P. Whittlesey<fnref n="1" />, Roberto Livi<fnref n="1" />, Ali Rahmati<fnref n="1" />, Orlando Romeo<fnref n="1" />, K. G. Klein<fnref n="4" />, Weijie Sun<fnref n="3" />, Bart van der Holst<fnref n="3" />, Zhenguang Huang<fnref n="3" />, Lan K. Jian<fnref n="5" />, Adam Szabo<fnref n="5" />, J. L. Verniero<fnref n="5" />, C. H. K. Chen<fnref n="6" />, B. Lavraud<fnref n="7" />, Mingzhe Liu<fnref n="8" />, Samuel T. Badman<fnref n="9" />, Tatiana Niembro<fnref n="9" />, Kristoff Paulson<fnref n="9" />, M. Stevens<fnref n="9" />, A. W. Case<fnref n="9" />, Marc Pulupa<fnref n="1" />, Stuart D. Bale<fnref n="1" />,<fnref n="6" />,<fnref n="10" />,<fnref n="11" /> and J. S. Halekas<fnref n="12" />

Received 2024 February 25; published 2024 April 12

In the published article, we mistakenly used part of the alpha velocity data from encounter 5 to encounter 8 (E5–E8), thus Figures 9 and 10 therein need to be corrected accordingly.

In this erratum, we provide corrected versions of Figures 9 and 10. We note that the negative $\Delta V_{\alpha p}/V_A$ population reduces in the current figures, but the major distributions in the two figures do not change significantly, therefore the discussions and implications in the published article are not affected.

<figure><img src="image_4.png" /><figcaption>**Figure 9.** The distributions of helium abundance ($A_{He}$) vs. alpha-proton differential speed that normalized by local Alfvén speed ($\Delta V_{\alpha p}/V_A$) in streamer belt solar wind from E4 to E10. Panels (a) and (b) present the helium characteristics in the HPS and PCS solar wind, respectively. The colors indicate the occurrence ratios. The red contours in both panels represent 25% and 50% of measurements.</figcaption></figure>

<figure><img src="image_5.png" /></figure>

<footnote n="1">¹Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA; huangjia.sky@gmail.com</footnote>

<footnote n="2">²BWX Technologies, Inc., Washington, DC 20001, USA</footnote>

<footnote n="3">³Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109, USA</footnote>

<footnote n="4">⁴Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85719, USA</footnote>

<footnote n="5">⁵Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA</footnote>

<footnote n="6">⁶School of Physics and Astronomy, Queen Mary University of London, London E1 4NS, UK</footnote>

<footnote n="7">⁷Institut de Recherche en Astrophysique et Planétologie, CNRS, UPS, CNES, Université de Toulouse, Toulouse, France</footnote>

<footnote n="8">⁸LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France</footnote>

<footnote n="9">⁹Smithsonian Astrophysical Observatory, Cambridge, MA 02138, USA</footnote>

<footnote n="10">¹⁰Physics Department, University of California, Berkeley, CA 94720-7300, USA</footnote>

<footnote n="11">¹¹The Brackett Laboratory, Imperial College London, London, SW7 2AZ, UK</footnote>

<footnote n="12">¹²Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA</footnote>
<figure><img src="image_6.png" /></figure>

<figure><img src="image_7.png" /><figcaption>**Figure 10.** Temperature anisotropy distributions of PCS solar wind with different $\Delta V_{\alpha p}/V_A$ from E4 to E10. Panels (a) and (b) exhibit the temperature anisotropy ($T_{\perp p}/T_{\parallel p}$) vs. parallel plasma $\beta(\beta_{\parallel p})$ in the HPS and PCS solar winds, respectively. The different colored dashed lines are instabilities, as indicated by the legend, and the black line is the anticorrelation relationship. The red contours indicate 25% and 50% measurements.</figcaption></figure>

ORCID iDs

Jia Huang https://orcid.org/0000-0002-9954-4707

J. C. Kasper https://orcid.org/0000-0002-7077-930X

Davin E. Larson https://orcid.org/0000-0001-5030-6030

Michael D. McManus https://orcid.org/0000-0001-6077-4145

P. Whittlesey https://orcid.org/0000-0002-7287-5098

Roberto Livi https://orcid.org/0000-0002-0396-0547

Ali Rahmati https://orcid.org/0000-0003-0519-6498

Orlando Romeo https://orcid.org/0000-0002-4559-2199

K. G. Klein https://orcid.org/0000-0001-6038-1923

Weijie Sun https://orcid.org/0000-0001-5260-658X

Bart van der Holst https://orcid.org/0000-0001-5260-3944

Zhenguang Huang https://orcid.org/0000-0003-1674-0647

Lan K. Jian https://orcid.org/0000-0002-6849-5527

Adam Szabo https://orcid.org/0000-0003-3255-9071

J. L. Verniero https://orcid.org/0000-0003-1138-652X

C. H. K. Chen https://orcid.org/0000-0003-4529-3620

B. Lavraud https://orcid.org/0000-0001-6807-8494

Mingzhe Liu https://orcid.org/0000-0003-2981-0544

Samuel T. Badman https://orcid.org/0000-0002-6145-436X

Tatiana Niembro https://orcid.org/0000-0001-6692-9187

Kristoff Paulson https://orcid.org/0000-0002-5699-090X

M. Stevens https://orcid.org/0000-0002-7728-0085

A. W. Case https://orcid.org/0000-0002-3520-4041

Marc Pulupa https://orcid.org/0000-0002-1573-7457

Stuart D. Bale https://orcid.org/0000-0002-1989-3596

J. S. Halekas https://orcid.org/0000-0001-5258-6128