Fall 2015 Graduate Courses
|PTYS 502|| |
Analytical and Numerical Modeling in Geosciences (3)
Analytical and numerical solutions to partial differential equations and other models widely used in disparate fields of geosciences. Equivalent to: GEOS 502, ECOL 502, MCB 502; GEOS is home department. Course Requisites: MATH 129. Open to advanced undergraduates with strong mathematical backgrounds and consent of instructor and Graduate College.
Principles of Planetary Physics (3)
PTYS Graduate Core Course. Introductory physics of planetary and interplanetary gases, fluids and plasmas. Thermodynamics, kinetic theory, plasma physics, hydrodynamics, and magnetohydrodynamics with solar-system applications. This includes planetary atmospheres, turbulence, solar wind, solar-system magnetic fields, dynamo theory, and planetary magnetospheres. Students will be expected to be familiar with vector calculus and both ordinary and partial differential equations.
Principles of Planetary Physics (3)
PTYS Graduate Core Course. Quantitative investigation of the physical processes controlling planet formation, the orbital and rotational dynamics of planetary systems, the mechanical and thermal aspects of a planetary interior, and the dynamics of the Earth-Moon and other satellite systems. Sample course syllabus, Matsuyama (PDF)
|PTYS 541A|| |
Dynamic Meteorology (3)
Thermodynamics and its application to planetary atmospheres, hydrostatics, fundamental concepts and laws of dynamic meteorology. Identical to ATMO 541A. ATMO is home department.
|PTYS 545|| |
Astrophysics of Stars and Accretion (4)
Equations of hydrodynamics; hydrodynamic equilibrium; polytropes; waves, and instabilities; convection and turbulence; radiative transfer; stellar atmospheres; stellar winds; nuclear reactions; stellar structure; helioseismology; stellar evolution; supernovae; white dwarfs, neutron stars, black holes; magnetohydrodynamics; accretion flows. Identical to: ASTR 545; ASTR is home department. Usually offered: Fall.
|PTYS 550|| |
Origin of the Solar System and Other Planetary Systems (3)
This course will review the physical processes related to the formation and evolution of the protosolar nebula and of protoplanetary disks. In doing that, we will discuss the main stages of planet formation and how different disk conditions impact planetary architectures and planet properties. We will confront the theories of disk evolution and planet formation with observations of circumstellar disks, exoplanets, and the planets and minor bodies in our Solar System. This course is cross-listed with ASTR 550 and may be co-convened with PTYS 450.
Evolution of Planetary Surfaces (3)
PTYS Graduate Core Course. The geologic processes and evolution of terrestrial planet and satellite surfaces including the Galilean and Saturnian and Uranian satellites. Course includes one or two field trips to Meteor Crater or other locales. Identical to: GEOS 554. PTYS is home department. Usually offered: Spring.
|PTYS 567|| |
Inverse Problems in Geophysics (3)
Linear and nonlinear inverse theory, including least squares, generalized and maximum likelihood methods. Identical to GEOS 567 and ATMO 567. GEOS is home department.
|PTYS 594A|| |
Planetary Geology Field Studies (1)
The acquisition of first-hand experience with geologic processes and features, focusing on how those features/processes relate to the surfaces of other planets and how accurately those features/processes can be deduced from remote sensing data. This is a three- to five-day field trip to an area of geologic interest where each student gives a short presentation to the group. This trip typically involves camping and occasional moderate hiking; students need to supply their own camping materials. Students may enroll in the course up to 10 times for credit but only three enrollments will count toward the major. Trip is led by a Planetary Sciences faculty member once per semester.