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This website features work from the completion of Phase 1 of the SCALES Project.

We are currently seeking partnerships for Phase 2.

Fluid Dynamics

  • Ocean Circulation I

    Problem set for the course Atmosphere, Ocean and Climate Dynamics

    Read more: Ocean Circulation I
  • Ocean Circulation II

    Problem Set for the course Atmosphere, Ocean and Climate Dynamics

    Read more: Ocean Circulation II
  • Midterm Exam

    Midterm exam for Atmosphere, Ocean and Climate Dynamics fluid dynamics 

    Read more: Midterm Exam
  • Emission temperatures and greenhouse models

    Problem sets for the Activity: Emission temperatures and greenhouse models

    Read more: Emission temperatures and greenhouse models
  • Assignment 1 The Earth’s Radiation Budget

    The global energy balance is important for Earth's climate. When visible radiation from the Sun reaches the Earth, some of it is reflected or scattered directly back into space as shortwave radiation (the percent reflected is known as albedo) and some of it is absorbed. In the absence of clouds, absorption happens mainly at the surface. The absorbed energy warms the Earth's surface, which, in turn, emits this energy at a longer wavelength (infrared rather than visible light).

    The purpose of this assignment is to get you thinking about the Earth's radiation budget and the sorts of phenomena which may influence that budget. The description of the datasets is taken from a class taught by Schlosser, Pfirman and Ting at Columbia University.

    Read more: Assignment 1 The Earth’s Radiation Budget

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