Programme/Approved Electives for 2022/23
None
Available as a Free Standing Elective
No
This module explores the physical processes governing the structure and circulation of atmospheres, including thermodynamics, radiative transfer, dynamics and waves. While primarily concentrating on the Earth's atmosphere, the physics explored will, nevertheless, be relevant to the study of the atmospheres of other planets in our Solar System and elsewhere. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics.
Aims
This module aims to develop an understanding, at the undergraduate level, of how physics is applied to explain the properties and phenomenology of atmospheres. The concepts from core studies of mechanics, electromagnetism and thermodynamics will be used and extended as applied to the study of atmospheres.
Intended Learning Outcomes
describe quantitatively the structure and dynamics of atmospheres. will be achieved by assessments: 1,2use the principles of thermodynamics to determine the structure of atmospheres. will be achieved by assessments: 1,2solve the equation of radiative transfer to evaluate the effect of radiation on atmospheric structure. will be achieved by assessments: 1,2apply the laws of motion to describe atmospheric dynamics and waves. will be achieved by assessments: 1,2
Lectures: 24 hoursTutorials: 12 hoursProblem Sheets: 24 hoursPrivate Study and Directed Reading: 90 hours
Description of Module Assessment
1: Problem Sheets weighted 30%Four assessed problem sheetsFour assessed problem sheets covering the topics taught in this module.
2: Unseen Exam weighted 70%2-hour unseen written examinationUnseen examination with questions based on a mix of factual knowledge, understanding and problem solving.