Comparisons of precipitable water vapor and zenith total delay derived from GNSS measurements, radiosondes, and ERA5 reanalysis data in the contiguous United States
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引用次数: 0
Abstract
Precipitable water vapor (PWV) is an important parameter in studying hydrological cycles on a regional or global scale and monitoring local weather changes. Here, PWV and zenith total delay (ZTD) datasets were derived from Global Navigation Satellite System (GNSS) measurements at 430 stations in the contiguous United States from 2013 through 2020. These GNSS-derived ZTD and PWV datasets were assessed based on radiosonde (RS) data at 48 RS-GNSS collocated sites from 2013 through 2020 and ERA5 reanalysis products at 430 sites covering the same periods. Comparisons show that the GNSS-derived PWV dataset obtains overall accuracies in terms of root-mean-square (RMS) errors of 2.3 mm and 1.8 mm with respect to the RS measurements and ERA5 reanalysis products, respectively. Moreover, the GNSS-derived ZTD dataset achieves overall RMS errors of 1.4 cm and 1.0 cm in contrast to the RS data and ERA5 atmosphere products, respectively. In general, the quality of the GNSS-derived PWV dataset in the regions of interest mainly depends on the accuracy of ZTD estimations obtained from GNSS observations. Furthermore, mean values and seasonal variations of PWV time series derived from GNSS observations are in good agreement with those extracted from the ERA5 reanalysis products across the contiguous United States. The mean values of PWV time series in the southeastern regions vary from 20 mm to 45 mm and they are larger than those in the western regions, which is due to the topography distribution over the contiguous United States.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.