GOES Geostationary Lightning Mapper Tools
glmtools requires Python 3.5+ and provides a conda environment.yml
for the key dependencies.
See the documentation in docs/index.rst
for complete installation instructions.
Compatible data:
glmtools automatically reconstitutes the parent-child relationships implicit in the L2 GLM data and adds traversal information to the dataset:
xarray's dimension-aware indexing lets you quickly reduce the dataset to flashes of interest, as described below.
glmtools can restore the GLM event geometry using a built-in corner-point lookup table, which allows for gridding of the imagery at finer resolutions that accurately represent the full footprint of each event, group, and flash.
The methods are described in Bruning et al. (2019):
Use the script in examples/grid/make_GLM_grids.py
. See the documentation in docs/index.rst
for complete instructions and example commands.
See the examples folder. basic_read_plot.ipynb
is a good place to start.
from glmtools.io.glm import GLMDataset
filename = 'OR_GLM-L2-LCFA_G16_s20180040537000_e20180040537200_c20180040537226.nc'
glm = GLMDataset(filename)
flash_id_list = glm.dataset.flash_id[20:30]
smaller_dataset = glm.get_flashes(flash_id_list)
See glmtools.io.glm.GLMDataset.subset_flashes
.
The logic implemented above is pretty simple, and below shows how to adapt it to find large flashes.
from glmtools.io.glm import GLMDataset
filename = 'OR_GLM-L2-LCFA_G16_s20180040537000_e20180040537200_c20180040537226.nc'
glm = GLMDataset(filename)
fl_idx = glm.dataset['flash_area'] > 2000
flash_ids = glm.dataset[{glm.fl_dim: fl_idx}].flash_id.data
smaller_dataset = glm.get_flashes(flash_ids)
print(smaller_dataset)