J/MNRAS/515/1788       PWRF configuration files                    (Yang+, 2022)

Simulating the night-time astronomical seeing at Dome A using Polar WRF. Yang Q., Wu X., Wang Z., Hu X., Guo Y., Qing C. <Mon. Not. R. Astron. Soc. 515, 1788-1794 (2022)> =2022MNRAS.515.1788Y 2022MNRAS.515.1788Y (SIMBAD/NED BibCode)
ADC_Keywords: Models Keywords: atmospheric effects - methods: data analysis - methods: numerical - site testing Abstract: Excellent astronomical seeing conditions above Dome A in Antarctica have been observed during nighttime (or polar winter). This study investigates the performance of the Polar-optimized version of the Weather Research and Forecasting (Polar WRF, PWRF hereafter) for simulating the night-time astronomical seeing at Dome A. The seeing values were estimated by a seeing model, which used the PWRF-simulated wind shear and temperature gradient as inputs. And three methods to obtain the boundary layer height in the seeing model have been examined The estimated seeing agree well with 50-days measurements from the KunLun Differential Image Motion Monitor at Dome A during the nighttime of 2019; the correlation coefficients range from 0.62 to 0.71. The PWRF-simulated meteorological parameters indicate that, strong temperature inversion and low wind speed (when gradient Richardson number is generally large) near the ground can lead to the good seeing condition. The results suggest that the PWRF model could be a useful tool for scheduling ground-based astronomy at Dome A during nighttime. Description: To help other researchers to duplicate the simulation, the PWRF configuration files (the so-called "namelist.wps" and "namelist.input") are provided as supplemental material to this paper. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file namelist.wps 82 36 namelist.wps for running the WRF Preprocessing system namelist.input 82 128 namelist.input for running the WRF Preprocessing system -------------------------------------------------------------------------------- See also: https://www2.mmm.ucar.edu/wrf/users/docs/user_guide_v4/contents.html : User's Guides for the Advanced Research WRF (ARW) Modeling System, Version 4 Description of file: One can see the description of the namelist variables at the WRF User's Guide, https://www2.mmm.ucar.edu/wrf/users/namelist_best_prac_wps.html (for the namelist.wps file), https://www2.mmm.ucar.edu/wrf/users/namelist_best_prac_wrf.html (for the namelist.input file). -------------------------------------------------------------------------------- History: From Qike Yang, yangqike(at)mail.ustc.edu.cn Acknowledgements: We are indebted to the NCAR and NCEP for granting access to their products (https://www2.mmm.ucar.edu/wrf/users/) and the PMG of OSU for their release of polar modifications for the WRF (Polar WRF; http://polarmet.osu.edu/PWRF/). References: Skamarock et al., 2019, A Description of the Advanced Research WRF Version 4. NCAR Tech. Note NCAR/TN-556+STR, 145 pp. doi:10.5065/1dfh-6p97 Skamarock at al., 2008, A Description of the Advanced Research WRF Version 3. NCAR Tech. Note NCAR/TN-475+STR, 113 pp. doi:10.5065/D68S4MVH
(End) Patricia Vannier [CDS] 01-Jun-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line