This article is a correction to:
Hydrogen atoms near the exobase are cold: independent observations do not support the hot exosphere concept
Dmytro Kotov1*
Oleksandr Bogomaz1,2- 1Institute of Ionosphere, Kharkiv, Ukraine
- 2State Institution National Antarctic Scientific Center of the Ministry of Education and Science of Ukraine, Kyiv, Ukraine
A Corrigendum on
Hydrogen atoms near the exobase are cold: independent observations do not support the hot exosphere concept
by Kotov D and Bogomaz O (2023). Front. Astron. Space Sci. 10:1200959. doi: 10.3389/fspas.2023.1200959
In the published article, there was an error. There was a typo in 2 Comparison to observations by independent techniques, paragraph 2, in which “hot” was used instead of “cold”. The correct sentence appears below:
“It should be noted that both the analyses by Rairden et al. and Zoennchen et al. were also conducted assuming the cold hydrogen concept, i.e., the equality of the exobase hydrogen temperature to the temperature of oxygen thermosphere.”
In the published article, there was an error. There was a typo in 2 Comparison to observations by independent techniques, paragraph 3 in which the word “of” was used instead of “or”. The corrected sentence appears below:
“Thus, despite extreme sensitivity of the high-altitude exospheric H density to change of cold hydrogen assumption to hot one (see Figure 2 b, e of Qin and Waldrop paper), comparison with other observations employing cold hydrogen approach (Zoennchen et al., 2011; Zoennchen et al., 2013) cannot be useful to refute or support hot hydrogen concept.”
The authors apologize for these errors and state that this does not change the scientific conclusions of the article in any way. The original article has been updated.
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Keywords: atomic hydrogen, exobase, hot atoms, cold atoms, independent observations
Citation: Kotov D and Bogomaz O (2023) Corrigendum: Hydrogen atoms near the exobase are cold: independent observations do not support the hot exosphere concept. Front. Astron. Space Sci. 10:1320143. doi: 10.3389/fspas.2023.1320143
Received: 11 October 2023; Accepted: 27 October 2023;
Published: 07 November 2023.
Edited and reviewed by:
Jaroslav Chum, Institute of Atmospheric Physics (ASCR), CzechiaCopyright © 2023 Kotov and Bogomaz. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Dmytro Kotov, ZG1pdHJ5a290b2ZmQGdtYWlsLmNvbQ==