On the scaling of the solar incident flux

Varotsos, C. A.; Lovejoy, S.; Sarlis, N. V.; Tzanis, C. G.; Efstathiou, M. N.

doi:https://doi.org/10.5194/acp-15-7301-2015

Articles | Volume 15, issue 13

https://doi.org/10.5194/acp-15-7301-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

https://doi.org/10.5194/acp-15-7301-2015

© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.

Articles | Volume 15, issue 13

Research article

|

07 Jul 2015

Research article |

| 07 Jul 2015

On the scaling of the solar incident flux

C. A. Varotsos, S. Lovejoy, N. V. Sarlis, C. G. Tzanis, and M. N. Efstathiou

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Final revised paper (published on 07 Jul 2015)
Preprint (discussion started on 15 Apr 2015)

Interactive discussion

Status: closed

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

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- Supplement

RC C2119: 'On the scaling of the solar 1 incident flux', Anonymous Referee #2, 30 Apr 2015
RC C2416: 'On the scaling of the solar incident flux', Anonymous Referee #1, 10 May 2015
AC C2653: 'Authors' responses to referees' comments', Costas Varotsos, 16 May 2015

Peer-review completion

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

AR by Costas Varotsos on behalf of the Authors (18 Jun 2015) Author's response

ED: Publish as is (22 Jun 2015) by Andreas Hofzumahaus

AR by Costas Varotsos on behalf of the Authors (22 Jun 2015)

Short summary

Varotsos et al. (Theor. Appl. Climatol., 114, 725–727, 2013) found that the solar ultraviolet (UV) wavelengths exhibit 1/f-type power-law correlations. In this study, we show that the residues of the spectral solar incident flux with respect to the Planck law over a wider range of wavelengths (i.e. UV-visible) have a scaling regime too.