Articles | Volume 20, issue 17
https://doi.org/10.5194/acp-20-10477-2020
https://doi.org/10.5194/acp-20-10477-2020
Research article
 | 
09 Sep 2020
Research article |  | 09 Sep 2020

Changes in the surface broadband shortwave radiation budget during the 2017 eclipse

Guoyong Wen, Alexander Marshak, Si-Chee Tsay, Jay Herman, Ukkyo Jeong, Nader Abuhassan, Robert Swap, and Dong Wu

Download

Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Guoyong Wen on behalf of the Authors (13 Jul 2020)  Author's response   Manuscript 
ED: Publish as is (21 Jul 2020) by Qiang Fu
AR by Guoyong Wen on behalf of the Authors (23 Jul 2020)  Author's response   Manuscript 
Short summary
We combine the ground-based observations and radiative transfer model to quantify the impact of the 2017 solar eclipse on surface shortwave irradiation reduction. We find that the eclipse caused local reductions of time-averaged surface flux of about 379 W m-2 (50 %) and 329 W m-2 (46 %) during the ~ 3 h course of the eclipse at the Casper and Columbia sites, respectively. We estimate that the Moon’s shadow caused a reduction of approximately 7 %–8 % in global average surface broadband SW radiation.
Altmetrics
Final-revised paper
Preprint