A high-quality daily nighttime light (HDNTL) dataset for global 600+ cities (2012-2024)
Authors/Creators
Description
Data Update Notice
- The current data release features improvements based on refined spatiotemporal interpolation parameters, updated angular effect reference layer and newly uploaded flag images.
- To prevent confusion among end users, we removed images heavily obscured by clouds (percentage of invalid pixels >50%. Pixels with constant invalid values, such as water bodies, are not considered in the calculation) from the daily NTL time series. For user reference, the HDNTL_Yearly_Coverage_Stats.csv file contains the yearly count of daily data records available for each city in the HDNTL dataset.
- Additionally, we provide a flag layer indicating the source of the angular effect reference value and whether interpolation was applied. This flag is encoded as a two-digit integer. The tens digit (values 0, 1, 2, or 3) denotes the source of the nadir-group reference value: 0 for an invalid value, 1 for the mean value of nadir observations from the current year, 2 for the mean value of nadir observations from the current year and its two adjacent years (except for boundary years such as 2012 or 2024, where only one adjacent year is available), and 3 for the annual mean value of all valid observations from the current year. The units digit (values 0 or 1) indicates the interpolation status: 0 for no interpolation and 1 for an interpolated value. The storage structure of this flag is consistent with that of the HDNTL data product.
Introduction
Nighttime light (NTL) data at daily scales presents an innovative foundation for monitoring human activities, offering vast potential across various research domains such as urban planning and management, disaster monitoring, and energy consumption. The VNP46A2 dataset, sourced from NPP/VIIRS, has been providing globally corrected daily NTL data since 2012. However, persistent challenges, such as fluctuations in daily NTL series due to spatial mismatch and angular effects, as well as missing data holes, have significantly impacted the accuracy and comprehensiveness of extracting daily NTL changes. To address these challenges, a dataset production framework focusing on error correction, interpolation, and validation was developed. This framework led to the creation of a high-quality daily NTL dataset from 2012 to 2024, named HDNTL, which specifically targets 653 cities with populations predictably exceeding one million in 2025. Comparative analysis with the VNP46A2 dataset revealed that the HDNTL dataset effectively mitigates instability in daily series caused by spatial mismatch and angular effects observed in VNP46A2, improving data comparability across time and space dimensions. This dataset enhances the ability of the NTL to reflect the ground events, providing a more accurate reference for daily-scale nighttime light research.
Data description
1. Data Overview
This product is generated based on the NASA Black Marble VNP46A2 dataset, inheriting its spatial resolution of 15 arc-seconds (approximately 500 meters). The data is provided in GeoTIFF format with a scale factor of 0.1.
2. File Structure
The data is organized in descending order of projected city population in 2025, with every 10 cities stored in a zip archive. For example, the zip archive named 001-010 contains data for the first to the tenth cities in the sequence. The city serial number can be referenced in the data table provided in the file “WUP2018-Pop2025_Cities_Over_1M_v2.xlsx”. Each folder within a compressed package contains HDNTL data for a city from 2012 to 2024, comprising 13 HDNTL images and 13 flag images. File names use underscores _ as separators, following the format below:
Example of HDNTL Image Name:
088_204586_Kitakyushu-Fukuoka_2022
Field Descriptions:
- Field 1: City serial number, ranked by projected population in 2025, ranging from 001 to 653 (refer to the “WUP2018-Pop2025_Cities_Over_1M_v2.xlsx” ).
- Field 2: City code (refer to the “WUP2018-Pop2025_Cities_Over_1M_v2.xlsx” ).
- Field 3: Urban Agglomeration Name (refer to the “WUP2018-Pop2025_Cities_Over_1M_v2.xlsx” ).
- Field 4: Year.
Example of Flag Image Name:
088_204586_Kitakyushu-Fukuoka_2022_Flag
3. Image Internal Structure
Each image contains multiple bands, with each band corresponding to one day of data. The band naming format is “NTLYYYY_MM_DD”, where:
- YYYY represents the year,
- MM represents the month,
- DD represents the day.
Example:
NTL2022_01_01 represents NTL data for January 1, 2022.
4. Data Usage Recommendations
- Data content: This dataset provides only the NTL value.
- Quality Control: Quality control, cloud cover, and snow flag information are inherited from the corresponding bands of VNP46A2.
- Viewing zenith angle: Users can refer to the band “Sensor_Zenith” of VNP46A1.
- Angular effect correction reference: Users can refer to the Flag images. The tens digit (values 0, 1, 2, or 3) denotes the source of the nadir-group reference value: 0 for an invalid value, 1 for the mean value of nadir observations from the current year, 2 for the mean value of nadir observations from the current year and its two adjacent years (except for boundary years such as 2012 or 2024, where only one adjacent year is available), and 3 for the annual mean value of all valid observations from the current year.
- Interpolation flag: Users can refer to the Flag images. The units digit (values 0 or 1) indicates the interpolation status: 0 for no interpolation and 1 for an interpolated value.
Please refer to the paper for other detailed information.
Acknowledgments
This study was supported by the Shenzhen Park of Hetao Shenzhen-Hong Kong Science and Technology Innovation Cooperation Zone “Theories for Spatiotemporal Intelligence and Reliable Data Analysis” (Project ID: HZQSWS-KCCYB-2024058), the Research Grants Council of Hong Kong (project No.15229222), the National Natural Science Foundation of China (No. 42401474), and the Hong Kong Polytechnic University (project No. Q-CDBP).
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Additional details
Related works
- Is published in
- Journal article: 10.5194/essd-17-5675-2025 (DOI)
References
- Hu, Y., Zhou, X., Yamazaki, D., and Chen, J.: A self-adjusting method to generate daily consistent nighttime light data for the detection of short-term rapid human activities, Remote Sens. Environ., 304, 114077, https://doi.org/10.1016/j.rse.2024.114077, 2024.
- NASA: VNP46A1 - VIIRS/NPP Daily Gridded Day Night Band 500m Linear Lat Lon Grid Night, 2012.
- NASA: VNP46A2 - VIIRS/NPP Gap-Filled Lunar BRDF-Adjusted Nighttime Lights Daily L3 Global 500 m Linear Lat Lon Grid, 2018.
- Román, M. O., Wang, Z., Sun, Q., Kalb, V., Miller, S. D., Molthan, A., Schultz, L., Bell, J., Stokes, E. C., Pandey, B., Seto, K. C., Hall, D., Oda, T., Wolfe, R. E., Lin, G., Golpayegani, N., Devadiga, S., Davidson, C., Sarkar, S., Praderas, C., Schmaltz, J., Boller, R., Stevens, J., Ramos González, O. M., Padilla, E., Alonso, J., Detrés, Y., Armstrong, R., Miranda, I., Conte, Y., Marrero, N., MacManus, K., Esch, T., and Masuoka, E. J.: NASA's Black Marble nighttime lights product suite, Remote Sens. Environ., 210, 113–143, https://doi.org/10.1016/j.rse.2018.03.017, 2018.
- Tan, X. and Zhu, X.: CRYSTAL: A novel and effective method to remove clouds in daily nighttime light images by synergizing spatiotemporal information, Remote Sens. Environ., 295, 113658, https://doi.org/10.1016/j.rse.2023.113658, 2023.
- Tan, X., Zhu, X., Chen, J., and Chen, R.: Modeling the direction and magnitude of angular effects in nighttime light remote sensing, Remote Sens. Environ., 269, 112834, https://doi.org/10.1016/j.rse.2021.112834, 2022.
- Tan, X., Chen, R., Zhu, X., Li, X., Chen, J., Sing Wong, M., Xu, S., and Xu, Y. N.: Spatial heterogeneity of uncertainties in daily satellite nighttime light time series, Int. J. Appl. Earth Obs. Geoinformation, 123, 103484, https://doi.org/10.1016/j.jag.2023.103484, 2023.
- Wang, Z, Shrestha, R., Román, M. O., 2020. NASA's Black Marble Nighttime Lights Product Suite Algorithm Theoretical Basis Document (ATBD). NASA Goddard Space Flight Center, Greenbelt, USA.
- Wang, Z., Román, M. O., Kalb, V. L., Miller, S. D., Zhang, J., and Shrestha, R. M.: Quantifying uncertainties in nighttime light retrievals from Suomi-NPP and NOAA-20 VIIRS Day/Night Band data, Remote Sens. Environ., 263, 112557, https://doi.org/10.1016/j.rse.2021.112557, 2021.
- Wu, Y. and Li, X.: Exploring the Drivers of Variations in Daily Nighttime Light Time Series From the Perspective of Periodic Factors, IEEE Geosci. Remote Sens. Lett., 21, 1–5, https://doi.org/10.1109/LGRS.2024.3358856, 2024.