Multi-point galactic cosmic ray measurements between 1 and 4.5&thinsp;AU over a full solar cycle

Honig, Thomas; Witasse, Olivier G.; Evans, Hugh; Nieminen, Petteri; Kuulkers, Erik; Taylor, Matt G. G. T.; Heber, Bernd; Guo, Jingnan; Sánchez-Cano, Beatriz

doi:https://doi.org/10.5194/angeo-37-903-2019

Articles | Volume 37, issue 5

https://doi.org/10.5194/angeo-37-903-2019

© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-37-903-2019

© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 37, issue 5

Regular paper

|

25 Sep 2019

Regular paper |

| 25 Sep 2019

Multi-point galactic cosmic ray measurements between 1 and 4.5 AU over a full solar cycle

Thomas Honig, Olivier G. Witasse, Hugh Evans, Petteri Nieminen, Erik Kuulkers, Matt G. G. T. Taylor, Bernd Heber, Jingnan Guo, and Beatriz Sánchez-Cano

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Final revised paper (published on 25 Sep 2019)
Preprint (discussion started on 10 May 2019)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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SC1: 'Comments on angeo-2019-68 (Multi-point galactic cosmic rays measurements between 1 and 4.5 AU over a full Solar cycle)', Elias Roussos, 14 May 2019
- AC3: 'Reply to SC1', Olivier Witasse, 07 Aug 2019
SC2: 'Comment on Multi-point galactic cosmic rays measurements between 1 and 4.5 AU over a full Solar cycle', Charlotte Götz, 20 May 2019
- AC1: 'Reply to Charlotte Goetz', Olivier Witasse, 01 Jul 2019
- AC4: 'Updated reply to SC2', Olivier Witasse, 07 Aug 2019
RC1: 'Review on Multi-point galactic cosmic rays measurements between 1 and 4.5 AU over a full Solar cycle by Honig et al.', Anonymous Referee #1, 04 Jun 2019
- AC2: 'Reply to referee #1', Olivier Witasse, 07 Aug 2019
RC2: 'Report on the manuscript Angeo-2019-68: “Multi-point galactic cosmic rays measurements between 1 and 4.5 AU over a full Solar cycle” by Thomas Honig et al. et al', Anonymous Referee #2, 29 Jun 2019
- AC5: 'Reply to referee #2', Olivier Witasse, 07 Aug 2019

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

ED: Publish as is (26 Aug 2019) by Manuela Temmer

AR by Olivier Witasse on behalf of the Authors (26 Aug 2019) Author's response Manuscript

Short summary

We analysed data from radiation monitors aboard different spacecraft such as Rosetta and Integral. From the data, we extracted the evolution of galactic cosmic rays as a function of time (over a full solar cycle) and position (from 1 to 4.5 AU). In the main results, we confirm the overall evolution (anti-correlation) of the fluxes with respect to the solar activity. We found a surprising result, which is a decrease in the flux of galactic cosmic rays around comet 67P.