Evanescent acoustic-gravity modes in the isothermal atmosphere: systematization and applications to the Earth and solar atmospheres

Cheremnykh, Oleg K.; Fedorenko, Alla K.; Kryuchkov, Evgen I.; Selivanov, Yuriy A.

doi:https://doi.org/10.5194/angeo-37-405-2019

Articles | Volume 37, issue 3

https://doi.org/10.5194/angeo-37-405-2019

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

Special issue:

Solar magnetism from interior to corona and beyond

https://doi.org/10.5194/angeo-37-405-2019

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

Articles | Volume 37, issue 3

Regular paper

|

11 Jun 2019

Regular paper |

| 11 Jun 2019

Evanescent acoustic-gravity modes in the isothermal atmosphere: systematization and applications to the Earth and solar atmospheres

Oleg K. Cheremnykh, Alla K. Fedorenko, Evgen I. Kryuchkov, and Yuriy A. Selivanov

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Final revised paper (published on 11 Jun 2019)
Preprint (discussion started on 21 Jan 2019)

Interactive discussion

Status: closed

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

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- Supplement

RC1: 'Referee report', Tamaz Kaladze, 26 Feb 2019
- AC1: 'Reply to the report by Reviewer_1', Yuriy A. Selivanov, 01 Mar 2019
- EC1: 'reminder', Sergiy Shelyag, 29 Mar 2019
  - RC4: 'reply to Editor', Tamaz Kaladze, 29 Mar 2019
    - EC2: 'done', Sergiy Shelyag, 29 Mar 2019
    - AC3: 'Author's final response 1', Yuriy A. Selivanov, 02 May 2019
RC2: 'Review of "Evanescent acoustic-gravity modes in the isothermal atmosphere..."', Anonymous Referee #2, 10 Mar 2019
- AC2: 'AuthorsReply_Referee_2', Yuriy A. Selivanov, 18 Mar 2019
  - RC3: 'Acceptance', Anonymous Referee #2, 20 Mar 2019
    - AC4: 'Author's final response 2', Yuriy A. Selivanov, 02 May 2019

Peer-review completion

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

ED: Publish as is (03 May 2019) by Sergiy Shelyag

AR by Yuriy A. Selivanov on behalf of the Authors (12 May 2019) Author's response Manuscript

Short summary

The fundamental mode of oscillations of the solar atmosphere, f-mode, plays an important role in solar physics. At an early stage of observation, it was found that its frequency is related to the wavelength by a ratio characteristic of waves on the surface of deep water. Subsequent observations revealed its inaccuracy. We derived waves with a different frequency–wavelength ratio and compared them with other possible waves of this type in both the solar and terrestrial atmosphere.