Yang Liu , Qiaoling Zhang , Tenglong Wang , Yibin Yao , Mingxian Hu , Haobo Li , Bao Zhang , Chaoqian Xu , Qingzhi Zhao
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引用次数: 0
Abstract
The Earth's troposphere delay provides valuable information for rainfall forecasting. Tropospheric delay products (e.g., Zenith Total Delay (ZTD)) derived from the Global Navigation Satellite System (GNSS) have become an indispensable approach for accessing tropospheric information. Several studies have established rainfall forecast models based on the GNSS-derived ZTD. However, the forecast predictors used in these models were all developed from the ZTD or its highly correlated parameters, resulting in high virtual forecast results. Therefore, a novel predictor, Convective Available Potential Energy (CAPE), was introduced to enhance the existing rainfall forecast model and is composed of the ZTD and CAPE rainfall (ZCR) model. The ZCR model includes six predictors: the ZTD value, ZTD variation, its derivation, CAPE value, CAPE variation, and its derivation. Hourly ZTD, CAPE, and rainfall data from three stations in Hong Kong with a time span of one year were collected to perform the experiment. The forecast accuracy of the ZCR model was evaluated using the corrected forecasted rate (CFR) and false alarm rate (FAR). The optimal thresholds of the predictors were determined using the percentile method, following the highest CFR and lowest FAR. The forecast accuracies of the ZTD and CAPE models, composed of their own three predictors, were comparable at the seasonal and monthly scales. Finally, we combined the ZTD and CAPE predictors into a ZCR model. Compared with the single ZTD or CAPE models, the combined ZCR model can significantly improve the accuracy of the FAR, with the CFR and FAR values of 93.53 % and 26.82 %, respectively. And the ZCR model also illustrates that the forecast accuracy on the monthly scale is higher than that on the seasonal scale.
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.