Articles | Volume 26, issue 17
https://doi.org/10.5194/acp-26-12887-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Ice core insights into the morphology and composition of mineral dust deposited in the tropical Peruvian Andes
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- Final revised paper (published on 14 Sep 2026)
- Supplement to the final revised paper
- Preprint (discussion started on 08 Jul 2026)
- Supplement to the preprint
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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RC1: 'Comment on egusphere-2026-3846', Anonymous Referee #1, 20 Jul 2026
- AC1: 'Reply on RC1', Austin Weber, 02 Aug 2026
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RC2: 'Comment on egusphere-2026-3846', Anonymous Referee #2, 04 Aug 2026
- AC2: 'Reply on RC2', Austin Weber, 18 Aug 2026
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Austin Weber on behalf of the Authors (25 Aug 2026)
Author's response
Author's tracked changes
Manuscript
ED: Publish as is (28 Aug 2026) by Mingjin Tang
AR by Austin Weber on behalf of the Authors (01 Sep 2026)
Post-review adjustments
AA – Author's adjustment | EA – Editor approval
AA by Austin Weber on behalf of the Authors (10 Sep 2026)
Author's adjustment
Manuscript
EA: Adjustments approved (10 Sep 2026) by Mingjin Tang
This manuscript provides a morphological and mineralogical characterisation of dust particles found in ice cores collected in the tropical Peruvian Andes and discusses their potential sources. Overall, I found the manuscript well written, and the discussion of potential dust sources is thorough. I only have a few minor comments.
I was wondering whether it would be possible to identify or use accessory minerals that can be specifically linked to the granodiorite, tonalite, and Chicama Formation. These could provide additional constraints for source attribution.
Carbonates were not observed in the analysed particles. Could the absence of carbonates help to exclude or support specific potential dust sources?
Do the particles show any coatings or internal mixing that could support atmospheric processing during long-range transport? Since the manuscript discusses the possibility of a North African contribution, I was wondering whether the particles show any evidence of atmospheric ageing that could provide additional support for their long-range transport.
In the Introduction, the authors mention the role of iron oxides as strong light absorbers, including after deposition on glaciers. However, the iron oxide content is not really highlighted or discussed in the rest of the manuscript. If iron oxides were identified, I think it would be interesting to briefly discuss their abundance and potential implications.