Supporting information for v2 of ``A Transparent Window into Early-Type Stellar Variability''

These folders contain grids of main-sequence stellar models computed four different metallicities and masses varying from 0.1-60 MSun. Models were computed using MESA r15140 following commit `964e07d` in this GitHub repo: https://github.com/adamjermyn/conv_trends. Changes from the previous version include: - Fixed a bug in calculating certain averages over the convection zone. - Incorporated the effects of radiation pressure on the Rayleigh number. - Increased time resolution of models. The metallicities are as follows: main_Z_time_2022_01_18_13_56_00_sha_ef8c - Z = 0.002 (SMC) main_Z_time_2022_01_18_13_56_06_sha_adbd - Z = 0.006 (LMC) main_Z_time_2022_01_18_13_56_13_sha_e814 - Z = 0.01<br> main_Z_time_2022_01_18_13_56_19_sha_f7ec - Z = 0.014 (MW)本数据集文件夹包含针对四种不同金属丰度、质量区间为0.1至60倍太阳质量（MSun）的主序星模型网格。本数据集的模型采用MESA r15140版本，基于GitHub仓库https://github.com/adamjermyn/conv_trends的提交记录`964e07d`完成计算。 相较于此前版本，本次更新的内容包括： 1. 修复了对流区（convection zone）部分平均值的计算漏洞； 2. 纳入了辐射压对瑞利数（Rayleigh number）的影响效应； 3. 提升了模型的时间分辨率。 各金属丰度对应的数据集文件夹如下： - main_Z_time_2022_01_18_13_56_00_sha_ef8c：金属丰度Z=0.002，对应小麦哲伦星系（Small Magellanic Cloud，SMC） - main_Z_time_2022_01_18_13_56_06_sha_adbd：金属丰度Z=0.006，对应大麦哲伦星系（Large Magellanic Cloud，LMC） - main_Z_time_2022_01_18_13_56_13_sha_e814：金属丰度Z=0.01 - main_Z_time_2022_01_18_13_56_19_sha_f7ec：金属丰度Z=0.014，对应银河系（Milky Way，MW）