Simulation files for "Feedback-limited accretion: variable luminosity from growing planets"
收藏资源简介:
Fargo simulation files and plotting routines to study the variability of the gas accretion rate into the planet. Plotting_FeedbackVariability_FULLPLOTS.ipynb has routines to plot the accretion rate over time, as well as other physical quantities such as density and vortensity, from the fargo files in each compressed folder. Due to size constraints we only include the most meaningful simulations with/without planetary feedback (A10_E100_M10 and A10_E000_M10), and with/without orbital eccentricity of 0.1 (with/without the final E10 tag), for a jupiter mass planet with and accretion timescale of 1 orbit. Plotting_FeedbackVariability.ipynb has routines specific to plot the accretion variability from the summarized files in the folder "VariabilityData".
用于探究行星气体吸积率变化特性的Fargo模拟文件与绘图例程。 其中Plotting_FeedbackVariability_FULLPLOTS.ipynb 包含用于从各压缩文件夹内的Fargo文件中绘制吸积率随时间变化曲线,以及密度、涡度(vortensity)等其他物理量的绘图例程。 受存储空间限制,本次仅纳入最具研究价值的模拟场景:包含存在/不存在行星反馈的两组(对应标识分别为A10_E100_M10与A10_E000_M10),以及轨道偏心率为0.1(对应后缀E10)或偏心率为0的场景,模拟对象为质量等于木星、吸积时标为1个轨道周期的行星。 Plotting_FeedbackVariability.ipynb 则包含用于从"VariabilityData"文件夹内的汇总文件中绘制吸积变化特性的专用绘图例程。



