A case study on the origin of near-Earth plasma
收藏资源简介：
Summary of data files. This is the dataset for a paper "A case study on the origin of near-Earth Plasma"<br> submitted to JGR-space by Glocer et al The paper conducts multifluid MHD simulations of the magnetosphere by the<br> BATSRUS code, with solar wind input, ionospheric outflow by the PWOM code,<br> and ionospheric potential solver, and inner magnetospehre by the CIMI code.<br> Solutions with and without plasmasphere are considered. All plots in the paper are made with spacepy (specific fork:<br> https://github.com/aglocer/spacepy) or with tecplot The data is organized as follows Top directory:<br> imf.dat: Has the solar wind input as a simple time series. Can be read and<br> plotted with the "ImfInput" tool in spacepy tared Directories with "PS" and "noPS" tags have simulation<br> output with and without plasmasphere. Each has three subdirectories described<br> as follows: GM: Has the "Global Magnetosphere" output from BATSRUS for the images shown.<br> y=0*out are cuts in the y=0 GSM plane and the *log file is the log output<br> containing Dst. Both can be plotted with spacepy pybats. The 3d files are<br> used in a few images and are tecplot binary files and read and plotted with<br> tecplot. PW: Has the "Polar Wind" output from the PWOM code for images shown. The<br> *out files are time dependent binary output for each field line. They can be<br> read and plotted with the pybats.pwom tool in spacepy. North and South<br> indicte northern and southern hemisphere respectively IE: Has the "Ionosphere Electrodynamics" output from the potential solver for<br> plots shown. the *log files have the CPCP data as a function of time. They<br> can be read and plotted with pybats in spacepy IM: Has the "Inner Magnetosphere" output from the CIMI code. The CIMIeq.out<br> file has time dependent snapshots of the solution on the min B surface for<br> plots shown. The *log files have the total energy as a function of time for<br> each species (among other variables). Both files are read and plotted with<br> pybats and pybats.cimi code in spacepy.
