Posts by Max Grover
- 02 December 2021
The Project Pythia Python Tutorial Seminar Series continues with the Intake-ESM Tutorial on Wednesday, December 8 at 1 PM Mountain Standard Time. This session will be led by Max Grover.
The content for this tutorial is hosted in the
.ipynb notebook file(s) within the
tutorial directory of this repository.
- 02 December 2021
November was an active month! There were a couple of ESDS Forum talks, a variety of answered Python questions during office hours, and a Python tutorial!
Check out the following ESDS update for the month of November 2021.
- 19 November 2021
A common component of people’s workflows is calculating annual averages, which helps reduce the frequency of datasets, making them easier to work with. Two of the data frequencies you may be looking to convert to annual include:
Daily (365 days in each year)
- 12 November 2021
There is a weather station located at the Mesa Lab, situated along the Foothills of the Rockies in Boulder, Colorado!
By the end of this post, you will be able to plot an interactive visualization of the weather data collected at the Mesa Lab, as shown below!
- 28 October 2021
October has been an active month! There were a variety of talks, a variety of answered Python questions during office hours, and a Python tutorial!
Check out the following ESDS update for the month of October 2021.
- 22 October 2021
Last week, Anderson Banihirwe added a new feature to intake-esm, enabling users to add “derived variables” to catalogs! This is an exciting addition, and although this has not been included in a release yet, you are welcome to test out the functionality!
Keep in mind that this is an initial prototype and the API is likely to change.
- 15 October 2021
The typical data workflow within the Python ecosystem when working with Weather Research and Forecasting (WRF) data is to use the wrf-python package! Traditionally, it can be difficult to utilize the
xarray data model with WRF data, due to a few challenges:
WRF data not being CF-compliant (which makes it hard for xarray to properly construct the dataset out of the box using xr.open_dataset)
- 08 October 2021
This Jupyter Notebook demonstrates how one might use the NCAR Community Earth System Model v2 (CESM2) Large Ensemble (CESM2-LE) data hosted on AWS S3. The notebook shows how to reproduce figure 2 from the Kay et al. (2015) paper describing the CESM LENS dataset (doi:10.1175/BAMS-D-13-00255.1), with the LENS2 dataset.
There was a previous notebook which explored this use case, put together by Joe Hamman and Anderson Banihirwe, accessible on the Pangeo Gallery using this link. The specific figure we are replicating is shown below.
- 01 October 2021
The first ESDS “meeting” took place in mid March 2021, with the kickoff event being the CGD town hall (here is the blog post detailing the topics at that meeting). Since that meeting, we have moved forward, holding a variety of Work in Progress talks, partnering with Xdev to offer Python Tutorials, and publish a series of blog posts aimed at documenting scientific workflows here at NCAR.
Most of our blog posts thus far have been focused on Python tutorials, workflow examples, or conference summaries. One new type of post we will be posting now are monthly summaries on ESDS activities. Since we have not posted one yet, we grouped up all of our activities since early March. Going forward, we will post on a monthly basis!
- 24 September 2021
Typically, diagnostics packages are written with following structure, using script-based workflows
Read files and do some preprocessing
- 17 September 2021
In this example, we will look at how long reading data from the Community Earth System Model (CESM), applying calculations, and visualizing the output takes using the following packages:
- 10 September 2021
In this example, we will cover how to leverage a useful package from the Pangeo Ecosystem, xESMF. One important note when using this package, is make sure you are using the most up-to-date documentation/version, a few years ago, development moved to the pangeo-data branch of the package, installable using the following:
For this example, we will download a file from the World Ocean Atlas, which includes a variety of ocean observations assembled from the World Ocean Database.
- 27 August 2021
Comparing models and observations is a critical component of climate diagnostic packages. This process can be challenging though - given the number of observational datasets to compare against, and the difference in spatiotemporal resolutions. In the previous iteration of the diagnostics package used for atmospheric data from the Community Earth System Model (CESM), they used pre-computed, observational datasets stored in a directory on the GLADE filesystem (
Within this example, we walk though generating an
intake-esm catalog from the observational data, reading in CESM data, and compare models and observations
- 20 August 2021
In previous weeks, we have looked at building Intake-ESM catalogs from history files and visualizing CESM output using Holoviews and Datashader, but this week we are putting together a few of those pieces to visualize a comparison between model runs.
One of the first ESDS blog posts looked at building an interactive dashboard to look at plots, using high resolution ocean model output as the dataset. One of the limitations of that approach is that the images are static - we are pulling in
pngs, and rending on the page, as opposed to more interactive options. In this example, we will read in data generated from ecgtools, from a directory only accessible via NCAR’s high performance computing center.
- 13 August 2021
This week, during Xdev office hours, Steve Yeager raised a question regarding plotting unstructured grid data within Python. He was interested in plotting output from the Community Atmosphere Model, which supports unstructured grids, essentially a combination of triangles allowing for higher resolution in certain parts of the domain. This can be adventageous when wanting to achieve the benefits of high resolution within the primary domain, while maintaining the global scale of the model. This week, NCAR Science tweeted a great explanation of how revolutionary this capability is in the context of resolving processes over Greenland.
Unstructured grids can be difficult to plot directly within Python since they do not follow the typical
lon (x, y) convention. There is some preprocessing that needs to be applied before plotting.
- 06 August 2021
In mid June, the CESM2 Large Ensemble dataset was made available to the public. This model was run in collaboration with the IBS Center for Climate Physics and the National Center for Atmospheric Research This dataset includes 100 ensemble members, at one degree spatial resolution, with each ensemble member including data from 1850 to 2100. If you are interested in learning more about how this ensemble was setup, be sure to check out the main webpage or read the pre-print of Rodgers et al. 2021 which describes this dataset in detail.
One of these challenges with this dataset is dealing with the massive amount of output. The data are available through the NCAR Climate Data Gateway and via the IBS OpenDAP Server. There is also a subset of the dataset available on the GLADE file system on NCAR HPC resources available within the directory
- 30 July 2021
Last year, the Project Pythia team was formed to “provide a public, web-accessible training resource that will help educate current, and aspiring, earth scientists to more effectively use both the Scientific Python Ecosystem and Cloud Computing to make sense of huge volumes of numerical scientific data.”
The team is formally a collaboration between three main organizations, although contributors come from throughout the scientific Python community:
- 26 July 2021
A couple weeks ago, I had an opportunity to (virtually) attend the Scientific Computing with Python (SciPy) Conference! The conference consisted of three primary sections:
- 02 July 2021
Parellelizing Python Code
- 25 June 2021
A common step to any project is documenting your data and your data workflow. Fortunately, open tools in the scientific python ecosystem make that much easier! In this example, we will cover creating your github repo, creating the catalog, visualizing the catalog, and generating a static webpage you can share with collaborators!
This week’s post is quite detailed, so just a warning! If you would like to look at the finished product, check out the following
- 17 June 2021
Every year, NCAR holds the Community Earth System Model (CESM) Workshop which brings together the CESM community to discuss relavant updates from the working groups as well as featured speakers and cross-working group discussions.
During the Software Engineering Working Group (SEWG) session, following a variety of talks, there was an open discussion regarding the current state of CESM diagnostics and future plans for collaboration.
- 11 June 2021
A common initial task when working with a new dataset is figuring out what data is available. This is especially true when working with climate ensembles with several components and time-frequency output (ex. Community Earth System Model Large Ensemble, CESM-LE). Here, we will examine different methods of investigating this catalog
- 04 June 2021
As mentioned in a couple of ESDS posts (intake-esm and Dask, debugging intake-esm), intake-esm can be a helpful tool to work with when dealing with model data, especially CESM. One of the requirements for using intake-esm is having a catalog which is comprised of two pieces:
A table of the relevant metadata (ex. file path, variable, stream, etc.)
- 28 May 2021
Cloud optimized datasets help improve speed of analysis
Entire 4 TB datasets open up in a few seconds
- 14 May 2021
This post was motivated by a post from Steve Yeager @sgyeager, who ran into an error when attempting to read in CMIP6 data via intake-esm.
For those who are unfamiliar with intake-esm, be sure to read over the documentation! The user guide even includes an entire portion of their site on looking at CMIP6 data. These resources would be a great place to start.
- 06 May 2021
A common task when developing notebooks or packages is collaborating with others. It can be challenging to do this when using JupyterHub since two people cannot access the same notebook at same time. One solution to this is to use Visual Studio Code (VS Code) to remotely access Casper/Cheyenne, use a virtual meeting plaform (Zoom, Google Meet), and interactively collaborate on development.
This process includes a few steps:
- 28 April 2021
Within this example, we cover how to use
xarray.map_blocks to calculate the mixed-layer depth within the CESM POP model output.
This calculation is “embarassingly parallel” such that each calculation is done within a single a column. The calculation should be easily computed within each column across the model domain. This is where
map_blocks can be used to improve the performance of this metric.
- 23 April 2021
This week, there a post within the Zulip regarding how to deal with indexing CAM-SE data. The tricky part here is that is an unstructured grid, where there is only one column to the data,
Here is an example of the dataset we are working with. Notice that both lat and lon have the same dimension,
- 15 April 2021
Last week, we added posts detailing how to configure Dask using the new PBS scheduler on Casper. In this week’s example, we provide an example of the recent updates to ncar-jobqueue, added by Anderson Banihirwe, which allow users to easily configure dask on Casper without having to add many extra steps.
You must update the package to use the newest updates. You can update using conda!
- 09 April 2021
This past week, NCAR CISL updated the Casper Node to use PBS instead of Slurm for scheduling jobs. This led a post in which an example of spinning up dask clusters on the new configuration. This was also an opportunity to dig into dask, and try applying it to a sample task, specifically looking at ecosystem variables in the CESM-LE dataset, using notebooks included in Matt Long’s krill-cesm-le repository, modified by Kristen Krumhardt.
Here, we spin up our dask cluster. At first, running this notebook resulted in a
killed worker error. After further expection, we noticed that additional resources would be needed to read in the notebook since the data are so large (on the order of ~1-2 TB). Increasing the individual worker to a higher amount (ex. 256 GB) solved the issue. Scale up to as many workers as you think are neccessary for the calculation (this may take some trial and error).
- 06 April 2021
Casper will complete a transition from Slurm to the PBS Pro workload manager on April 7, 2021. This has implications for how to spin up a Dask cluster, including via the NCAR Jupyterhub.
Below is an example script suitable for the new configuration using the
PBSCluster function from
dask_jobqueue. Note that the
ncar_jobqueue package requires updating to work with the new configuration.
- 02 April 2021
One of the questions that came up during the ESDS Town Hall was how do scientists/developers get credit toward their efforts in developing open-source code? Software that is used by the wider community should received the acknowledgment and recognition it deserves.
Data and academic publication citations have become popular in the literature, but often times, software is not cited… which can be arguably just as important to the work as the data.
- 26 March 2021
Last week, there was a town hall focused on gathering input on the Earth System Data Science initiative at NCAR. The meeting began with an introduction about the initiative, the vision, goals, and how the team is planning to start working toward these goals.
The Question/Answer portion of the town hall was very informative and brought up some great topics for discussion. They have been collected from both the chat and Google Doc, sorted by category.