A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Performance
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| Autores principales: | , , , , , , , , , , , , , , , |
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| Formato: | Preprint |
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2025
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| author | Bauza-Ruiz, Pedro Jose Blanch, Oscar Calisse, Paolo G. Campoy-Ordaz, Anna Colak, Sidika Merve Doro, Michele Font, Lluis Gaug, Markus Grau, Roger Kolar, Darko Maggio, Camilla Martinez, Manel Stanic, Samo Ubach, Santiago Zavrtanik, Marko Zivec, Miha |
| author_facet | Bauza-Ruiz, Pedro Jose Blanch, Oscar Calisse, Paolo G. Campoy-Ordaz, Anna Colak, Sidika Merve Doro, Michele Font, Lluis Gaug, Markus Grau, Roger Kolar, Darko Maggio, Camilla Martinez, Manel Stanic, Samo Ubach, Santiago Zavrtanik, Marko Zivec, Miha |
| contents | The Barcelona Raman LIDAR (BRL) will provide continuous monitoring of the aerosol extinction profile along the line of sight of the Cherenkov Telescope Array Observatory (CTAO). It will be located at its Northern site (CTAO-N) on the Observatorio del Roque de Los Muchachos. This article presents the performance of the pathfinder Barcelona Raman LIDAR (pBRL), a prototype instrument for the final BRL. Power budget simulations were carried out for the pBRL operating. under various conditions, including clear nights, moon conditions, and dust intrusions. The LIDAR PreProcessing (LPP) software suite is presented, which includes several new statistical methods for background subtraction, signal gluing, ground layer and cloud detection and inversion, based on two elastic and one Raman lines. Preliminary test campaigns were conducted, first close to Barcelona and later at CTAO-N, albeit during moonlit nights only. The pBRL, under these non-optimal conditions, achieves maximum ranges up to about 35 km, range resolution of about 50 m for strongly absorbing dust layers, and 500 m for optically thin clouds with the Raman channel only, leading to similar resolutions for the LIDAR ratios and Angstrom exponents. Given the reasonable agreement between the extinction coefficients obtained from the Raman and elastic lines independently, an accuracy of aerosol optical depth retrieval in the order of 0.05 can be assumed with the current setup. The results show that the pBRL can provide valuable scientific results on aerosol characteristics and structure, although not all performance requirements could be validated under the conditions found at the two test sites. Several moderate hardware improvements are planned for its final upgraded version [truncated]. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_17996 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Performance Bauza-Ruiz, Pedro Jose Blanch, Oscar Calisse, Paolo G. Campoy-Ordaz, Anna Colak, Sidika Merve Doro, Michele Font, Lluis Gaug, Markus Grau, Roger Kolar, Darko Maggio, Camilla Martinez, Manel Stanic, Samo Ubach, Santiago Zavrtanik, Marko Zivec, Miha Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena The Barcelona Raman LIDAR (BRL) will provide continuous monitoring of the aerosol extinction profile along the line of sight of the Cherenkov Telescope Array Observatory (CTAO). It will be located at its Northern site (CTAO-N) on the Observatorio del Roque de Los Muchachos. This article presents the performance of the pathfinder Barcelona Raman LIDAR (pBRL), a prototype instrument for the final BRL. Power budget simulations were carried out for the pBRL operating. under various conditions, including clear nights, moon conditions, and dust intrusions. The LIDAR PreProcessing (LPP) software suite is presented, which includes several new statistical methods for background subtraction, signal gluing, ground layer and cloud detection and inversion, based on two elastic and one Raman lines. Preliminary test campaigns were conducted, first close to Barcelona and later at CTAO-N, albeit during moonlit nights only. The pBRL, under these non-optimal conditions, achieves maximum ranges up to about 35 km, range resolution of about 50 m for strongly absorbing dust layers, and 500 m for optically thin clouds with the Raman channel only, leading to similar resolutions for the LIDAR ratios and Angstrom exponents. Given the reasonable agreement between the extinction coefficients obtained from the Raman and elastic lines independently, an accuracy of aerosol optical depth retrieval in the order of 0.05 can be assumed with the current setup. The results show that the pBRL can provide valuable scientific results on aerosol characteristics and structure, although not all performance requirements could be validated under the conditions found at the two test sites. Several moderate hardware improvements are planned for its final upgraded version [truncated]. |
| title | A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Performance |
| topic | Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2505.17996 |