Influence Of Solar Activity On Penetration Of Travelling Planetary-Scale Waves From The Troposphere Into The Thermosphere - Supporting Data

Contents:<br> averh.zip - Output data from model simulations averaged over 12 runs with high solar activity;<br> /averh/uvt400_Jan_ogw_volf.dx - Zonal, meridional wind components, temperature (structure corresponds to uvt.ctl);<br> /averh/phi.dx - Geopotential height in gpm;<br> /averh/gh_m1_1.dx, /averh/gh_m2_1.dx - Estimated PSW amplitudes and phases after the longitude-time Fourier transform of the MUAM solutions with the least squares fitting of the geopotential height (zonal wavenumber 1 and 2, respectively)<br> /averh/zw_m1_1.dx, /averh/zw_m2_1.dx, /averh/mw_m1_1.dx, /averh/mw_m2_1.dx, /averh/tp_m1_1.dx, /averh/tp_m2_1.dx - The same but for wind components and temperature, respectively<br> averl.zip - Output data from model simulations averaged over 12 runs with low solar activity; contents are similar to "averh.zip"<br> T_msis.jpg - Altitude-latitude distributions of the averaged over January-February temperature in K at the high (left) and low (center) solar activity level along with and differences between the corresponding values (right) for the NRLMSISE-00 data. <br> pw_hsa.jpg - Amplitudes of PSW geopotential height variations (in g.p.m.) with nonzero (left) and zero (right) tropospheric sources of the westward travelling PSWs with periods 4, 5, 7, 10, 16 days (a-e, respectively) under the high SA, averaged over 12-members ensembles and over January – February. The color scales for the corresponding PSWs are identical.<br> pw_lsa.jpg - The same but for the low SA conditions<br> files *.gs, *.ctl - Examples of the scripts and file descriptions for GRADS system to build figures shown in the manuscript.<br> Additional data including outputs from separate model runs are available from the authors upon request.数据集内容如下： averh.zip：包含12次高太阳活动工况下模式模拟结果的平均输出数据； /averh/uvt400_Jan_ogw_volf.dx：包含纬向风分量、经向风分量与气温场数据（文件结构与uvt.ctl一致）； /averh/phi.dx：以位势米（gpm）为单位的位势高度场； /averh/gh_m1_1.dx、/averh/gh_m2_1.dx：对MUAM模式解进行经时傅里叶变换后，通过最小二乘法拟合位势高度场得到的行星尺度驻波（PSW, Planetary Standing Wave）振幅与相位，分别对应波数1和波数2； /averh/zw_m1_1.dx、/averh/zw_m2_1.dx、/averh/mw_m1_1.dx、/averh/mw_m2_1.dx、/averh/tp_m1_1.dx、/averh/tp_m2_1.dx：含义同上，分别对应风分量与气温场的相关结果； averl.zip：包含12次低太阳活动工况下模式模拟结果的平均输出数据，内容与averh.zip类似； T_msis.jpg：展示NRLMSISE-00模式数据中，1-2月平均气温的纬度-高度分布：左图为高太阳活动水平下的结果，中图为低太阳活动水平下的结果，右图为二者的差值，气温单位为开尔文（K）； pw_hsa.jpg：高太阳活动（SA, Solar Activity）条件下，周期分别为4、5、7、10、16天（依次对应a-e子图）的西向传播行星尺度驻波，其对流层源项非零（左图）与为零（右图）时的位势高度扰动振幅（单位：位势米）分布。该结果基于12个成员集合模拟以及1-2月的平均数据，各对应行星尺度驻波的色标尺度保持一致； pw_lsa.jpg：含义同上，仅适用于低太阳活动条件； *.gs、*.ctl脚本与文件描述示例：用于GRADS（格点分析与显示系统, Grid Analysis and Display System）绘制论文手稿中所用图像的相关脚本与文件说明； 额外数据（含单次独立模式运行的输出结果）可向作者索取。