A method to compute a Delta representing the change in TC intensity due to climate change

Post-doctoral spring onset research

Showcasing my work throughout the years.

Routine to compute the advective energy fluxes from model results from COSMO-CLM model

GPU accelerated primitives for FESOM2.

A climate modelling data processing and analysis application designed to work with RegCM4.9

This repository contains baseconfigs & userconfigs, cGENIE outputs, Python scripts for data analysis, and figures associated with the Herho et al. (2024) manuscript.

Some data and models used for the DEC report 🌎🔥

Tool to translate weather data files to WTH format for DSSAT

Neural network training for climate in Songs of the Eons

This repository is for storing the code I have written for an internship started during the summer of 2021 at Université du Québec à Montréal (UQÀM) under the direction of professor Alejandro Di Luca. The internship concerns the evaluation of the Canadian Regional Climate Model 6 - Global Environmental Multiscale 5 (CRCM6-GEM5)'s energy balance.

Fine-tuning foundation model for severe weather event prediction in the U.S. with 3-6 months of lead time

Arctic sea ice thickness sensitivity experiments

Simple climate model simulation made for McGill Physics Hackathon 2020

A collection of Python and Bash scripts for automating runtime and trace data collection for the Isca climate model.

Calculate wetbulb temperature

Web-based application to model, analyze, visualize, and predict global surface temperature anomalies.

AMIP experiments for surface forcings (sea ice, SST, QBO, Eurasian snow)

Python scripts used for paper Warnatzsch and Reay (2019). Assessing Climate Change Projections and Impacts on Central Malawi’s Maize Yield: The Risk of Maladaptation (https://doi.org/10.1016/j.scitotenv.2019.134845). These files were created as part of a NERC funded PhD project. Erika Warnatzsch was funded by a NERC doctoral training partnership…

Atmospheric temperature profile generated by a highly simplified radiative transfer model. It calculates the temperature at a range of points (initially three) from the Earth's surface to the top of the atmosphere. The input parameters are the percentage of planetary cloud cover, the emissitivity/absorptivity of the two atmospheric layer