D10_MarsWRF_MSLddac3yrs_gridB.txt: MarsWRF-predicted dust devil activity along MSL's traverse over 3 Mars years.

Mean DDA is the Renno et al. [1998] dust devil activity at the Curiosity Rover’s location, averaged over 90° of Ls for the given period, at the time of sol shown (LTST = local true solar time). <br><br>DDA is predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br>These data are used to produce Figures 9 and 11 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>平均尘卷风活动量（Mean DDA）为Renno等人[1998]提出的尘卷风活动指标，对应好奇号火星车着陆点处的观测结果，以给定时段内对应火星日的当地真太阳时（LTST = Local True Solar Time）为基准，按90°火星太阳经度（Ls）区间取平均。 尘卷风活动量（DDA）通过基于盖尔撞击坑上空大气的火星天气研究与预报模型（MarsWRF）模拟输出进行预测。 本数据集用于生成论文《三个火星年尺度下盖尔撞击坑的对流涡旋与尘卷风预报及与MSL-REMS观测结果的对比》中的图9与图11，该论文发表于2019年《地球物理研究杂志：行星卷》（JGR-Planets），作者为C. E. Newman、H. Kahanpää、M. I. Richardson、G. M. Martinez、A. Vicente-Retortillo与M. Lemmon。