Fall 2016 Graduate Courses
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.
Planetary Global Tectonics (3)
PTYS Graduate Core Course. Application of the physics of solid-state deformation to global tectonics of the terrestrial planets and icy moons of the solar system. Modes of topographic support, isostasy and implications for gravity/topography ratios on one-plate planets. Theory of floating elastic plates as an approximation to the lithosphere. Use of seismic data to determine the interior structure and composition and modes of heat conduction in planets.
Asteroids, Comets and Kuiper Belt Objects (3)
This is an introduction to the "minor planets," the asteroids, comets and Kuiper Belt objects. The focus will be on origin and evolution (including current evolution), as well as techniques of study. It will include an evening at the telescope of an asteroid search program. Graduate-level requirement includes some original work or calculations in the paper/project submitted and to research one of the primary topics and lead the class discussion of it. May be co-convened with PTYS 416.
(001) Malhotra | Course Page
Instrumentation and Statistics (3)
Radiant energy; signals and noise; detectors and techniques for imaging, photometry, polarimetry and spectroscopy. Examples from stellar and planetary astronomy in the x-ray, optical, infrared and radio. Graduate-level requirements include an in-depth research paper. Identical to ASTR 518. ASTR is home department.
Physics of the Earth (3)
Fundamentals of the physics of the solid earth, including thermodynamics, rheology, geomagnetism, gravity, and plate tectonics. Graduate-level requirements include a term paper in publication format on some aspect of a major course topic. Identical to: GEOS 519; GEOS is home department. May be convened with: PTYS 419. Usually offered: Spring.
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.
Remote Sensing of Planetary Surfaces (3)
Remote-sensing based exploration of planetary surfaces, including that of the Earth as relevant to other planets. Emphasis will be on compositional, geologic, and geophysical interpretations via remote sensing throughout the electromagnetic spectrum. Course will cover basic principles, image and spectroscopic analysis techniques, case studies in planetary remote sensing, and many examples from past, current, and potential future spacecraft missions. Equivalent to/crosslisted GEOS 551. PTYS is home department.
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.
(001) Hamilton | Course Page
Special Topics in Planetary Science (2-3)
Methods in Computational Astrophysics (3)
The course is a "hands-on" introduction to computer use for research by scientists in astrophysics and related areas. The course begins with a survey of and introduction to tools available on Linux systems, web-based tools, and open-source software widely used in astrophysics. Standard methods for integration, iteration, differential and difference equations, and Monte Carlo simulations, are discussed, in one to four dimensions. Historically important methods of radiative transfer, reaction networks, and hydrodynamics are presented, and contrasted with presently-used methods. Parallel programming is introduced, and discussed in terms of new and future computer systems. Special topics are added to reflect new developments. The course is task-oriented, with individual and team work projects, and class participation determining grades. Most of the work is done on the student's own personal computer (Linux or Mac operating systems are preferred). Identical to ASTR/PHYS 596B. ASTR is home department. Equivalent to ASTR 596B and PHYS 596B; ASTR is home department. Typically Offered Spring. Regular or Alternative Grades: ABCDE or SPCDE.
Atmospheric Radiation and Remote Sensing (3)
Theory of atmospheric radiative transfer processes; specific methods for solving the relevant equations; applications to problems in radiative transfer; theoretical basis for remote sensing from the ground and from space; solutions to the "inverse" problem. Identical to ATMO 656A; ATMO is home department.