Articles | Volume 18, issue 5
https://doi.org/10.5194/essd-18-3449-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
A temporally consistent global 500 m-resolution monthly VIIRS-like nighttime light dataset (1992–2024)
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- Final revised paper (published on 21 May 2026)
- Preprint (discussion started on 12 Mar 2026)
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 essd-2026-129', Anonymous Referee #1, 12 Mar 2026
- AC1: 'Reply on RC1', Hongquan Cheng, 18 Apr 2026
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RC2: 'Comment on essd-2026-129', Anonymous Referee #2, 18 Mar 2026
- AC2: 'Reply on RC2', Hongquan Cheng, 18 Apr 2026
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RC3: 'Comment on essd-2026-129', Anonymous Referee #3, 23 Mar 2026
- AC3: 'Reply on RC3', Hongquan Cheng, 18 Apr 2026
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Hongquan Cheng on behalf of the Authors (18 Apr 2026)
Author's response
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ED: Publish as is (22 Apr 2026) by Yuqiang Zhang
AR by Hongquan Cheng on behalf of the Authors (30 Apr 2026)
Author's response
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The paper is quite boastful and ignores the complexities of projecting VIIRS global nighttime light back to 1992. Earth Observation Group provides access to the DMSP monthly nighttime lights from 1992-2021 and VIIRS from 2012-2025. EOG's offerings are clearly the first open-access time series of monthly nighttime lights spanning 1992-2025. DMSP and VIIRS nighttime lights differ from each other in several key ways: A) VIIRS DNB pixel footprints are 42+ times smaller than DMSP. Many small lights detected by VIIRS are absent in DMSP. B) VIIRS has lower detection limits and a wider dynamic range. In contrast, DMSP nighttime light observations use 6-bit quantization and frequently saturate in bright city centers. C) The VIIRS overpass time is typically between midnight and 03:00 local time. The early DMSP record (1992-2013) had mid-evening overpass times, between 19:30 and 21:30. The DMSP extension series (2013-2021) has pre-dawn overpass times. Nighttime lights have variable diurnal patterns. This paper's data from 1992 to 2011 are speculative and cannot be recommended for quantitative use. The earliest VIIRS data are from 2012. The paper's title is thus misleading. The paper takes an ill-informed and swaggering approach to generating monthly nighttime lights from 1992-2011.