A Model/Simulation to learn about changes in Earth’s climate caused by variations in the solar energy received by the planet over geological time scales and to understand the role of the orbital parameters (obliquity, precession, and eccentricity) in causing ice age cycles (Milankovitch cycles) on Earth.
Students can vary orbital parameters (eccentricity, obliquity, longitude of the perihelion) of Earth to observe the corresponding effect on the incoming solar radiation (insolation). They can also compare the global and seasonal distribution of insolation at two different points in time, and observe orbital data for particular times in the past and future (based on the paper by Laskar et al.).
As a teacher of Mathematics/ Statistics, you can use this resource to teach your students how to write code for different simulations of Earth’s long term climate fluctuations due to changes in orbital parameters. Detailed instructions are provided by the author of the model. This code is in the “shiny” package of R.
This resource consists of ten components:
Use this tool to help your students find answers to:
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TROP ICSU is a project of the International Union of Biological Sciences and Centre for Sustainability, Environment and Climate Change, FLAME University.