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https://doi.org/10.5194/angeo-2020-72
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-2020-72
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
16 Dec 2020
| 16 Dec 2020
Status: this preprint has been withdrawn by the authors.
Dynamics of He++ ions at interplanetary shocks
Abstract. Variations of parameters of twice-ionized helium ions – He++ ions or α-particles – in the solar wind plasma during the interplanetary shock front passage are investigated. We used the data measured by the BMSW (Bright Monitor of Solar Wind) instrument installed on the SPEKTR-R satellite, which operated since August 2011 to 2019 and registered 57 interplanetary shocks. According to received data, the parameters of He++ ions were calculated: velocity Vα, temperature Tα, absolute density Nα and relative density (helium abundance) Nα/Np. The correlation of changes in helium abundance Nα/Np with the parameters βi, θBn and MMS were investigated.
This preprint has been withdrawn.
How to cite. Sapunova, O. V., Borodkova, N. L., Zastenker, G. N., and Yermolaev, Y. I.: Dynamics of He++ ions at interplanetary shocks, Ann. Geophys. Discuss. [preprint], https://doi.org/10.5194/angeo-2020-72, 2020.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
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Interactive discussion
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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- Supplement
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RC1: 'Dynamics of He++ ions at interplanetary shocks', Anonymous Referee #1, 26 Jan 2021
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AC1: 'Reply on RC1', Olga Sapunova, 24 Mar 2021
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AC1: 'Reply on RC1', Olga Sapunova, 24 Mar 2021
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RC2: 'Review comments', Anonymous Referee #2, 05 Feb 2021
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AC2: 'Reply on RC2', Olga Sapunova, 24 Mar 2021
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AC2: 'Reply on RC2', Olga Sapunova, 24 Mar 2021
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RC3: 'Referee feedback', Anonymous Referee #3, 02 Mar 2021
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AC3: 'Reply on RC3', Olga Sapunova, 24 Mar 2021
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AC3: 'Reply on RC3', Olga Sapunova, 24 Mar 2021
Interactive discussion
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
- Printer-friendly version
- Supplement
-
RC1: 'Dynamics of He++ ions at interplanetary shocks', Anonymous Referee #1, 26 Jan 2021
-
AC1: 'Reply on RC1', Olga Sapunova, 24 Mar 2021
-
AC1: 'Reply on RC1', Olga Sapunova, 24 Mar 2021
-
RC2: 'Review comments', Anonymous Referee #2, 05 Feb 2021
-
AC2: 'Reply on RC2', Olga Sapunova, 24 Mar 2021
-
AC2: 'Reply on RC2', Olga Sapunova, 24 Mar 2021
-
RC3: 'Referee feedback', Anonymous Referee #3, 02 Mar 2021
-
AC3: 'Reply on RC3', Olga Sapunova, 24 Mar 2021
-
AC3: 'Reply on RC3', Olga Sapunova, 24 Mar 2021
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Olga V. Sapunova
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Natalia L. Borodkova
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Georgii N. Zastenker
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Yuri I. Yermolaev
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Short summary
The collisionless shocks are very complicated and important field of nowadays researches. We used the data measured by the plasma spectrometer BMSW (Bright Monitor of Solar Wind) to investigate variations of parameters of twice-ionized helium ions He++ in the solar wind during the interplanetary shock passage. It was shown that the changes of He++ abundance are depended of interplanetary shock parameters.
The collisionless shocks are very complicated and important field of nowadays researches. We...