Spring 2026 Course Search

Physics II: Electricity and Magnetism (with Lab) — PHY4327.01

Instructor: Tim Schroeder
Days & Time: M/Th 10:00AM-11:50AM, W 8:30AM-12:10PM (Lab)
Credits: 5

How does influence travel from one thing to another? In Newton’s mechanics of particles and forces, influences travel instantaneously across arbitrarily far distances. Newton himself felt this to be incorrect, but he did not suggest a solution to this problem of “action at a distance.” To solve this problem, we need a richer ontology: The world is made not only of particles, but also of fields. As examples of the field concept, we study the theory and applications of the electric field and the magnetic field.

Third Cinema — FV2316.01

Instructor: Beatriz Santiago Muñoz
Days & Time: WE 2:10pm-5:50pm
Credits: 4

This course is a seminar focusing on films that were made by filmmakers and collectives which saw themselves as inaugurating a new kind of filmmaking modeled neither on the commercial American filmmaking, nor on the European “Auteur” Cinema, instead crafting a third position, a cinema that was implicated in anti-capitalist and anti-imperialist struggles of the time. These works challenged ideas of authorship, questioned the role of the filmmaker in political transformation, and proposed alternatives to the forms of production that filmmaking made use of.

Stars and Galaxies — PHY2106.01

Instructor: Hugh Crowl
Days & Time: MO,TH 10:00am-11:50am
Credits: 4

All but a handful of the objects you see in the night sky are stars in our Galaxy, the Milky Way. Although we know about these stars only from studying their light, we know today that they are not just points of light, but large, gravitationally‐bound balls of plasma governed by the laws of physics. Stars, together with dust, gas, and dark matter, are found in larger structures – galaxies. In turn, galaxies, are located in even larger structures called galaxy groups and galaxy clusters.

The Physics of Light and Color — PHY2114.01

Instructor: Hugh Crowl
Days & Time: TU 8:30am-12:10pm
Credits: 2

The physics of light and color initially appears simple: light is a wave and the wavelength of light determines color. While this basic physical description of light is easy to state, going deeper quickly opens up large range of questions. How do different wavelengths of light combine to make colors? How does light from different sources interfere? How does light change path when it travels through different materials? How do humans sense light both in and outside of the visible spectrum? How does our perception of color affect how we interpret our world?

The Physics of Sound — PHY2278.02

Instructor: Hugh Crowl
Days & Time: TU 8:30am-12:10pm
Credits: 2

Physically, sound is simply the compression of air around us. However, this relatively simple description obscures a much richer understanding of sound. From how different sounds are generated and perceived to how different sounds can combine to make something new to how to design acoustically pleasant spaces, the physics of sound plays a key role. This course is about the fundamentals that underlie sound and is designed to serve as an introduction to those who are interested in going further.

Robotics and STEM Education: A Workshop — EDU2107.01

Instructor: Hugh Crowl
Days & Time: FR 10:30am-12:20pm
Credits: 1

In this course, students will gain experience with using simple programmable robots and how they can be utilized in STEM education. The focus of this class will be on learning and designing lessons for K-12 students utilizing these robots. This class is accessible for students at all levels of computer programming experience (including none). 

Legacy and 3D Audio Mixing and Production — MSR4374.01

Instructor: Cristian Amigo
Days & Time: WE 10:00am-11:50am & WE 2:10pm-4:00pm
Credits: 4

This course explores the art and science of mixing and producing audio for both emergent immersive formats and traditional legacy platforms. Students will gain hands-on experience with spatial audio technologies such as Dolby Atmos, Ambisonics, and binaural mixing, while also mastering industry-standard techniques for stereo and 5.1 surround sound production.

BC Soundscape Dub Ensemble — MSR4373.01

Instructor: Cristian Amigo
Days & Time: TU 10:30am-12:20pm
Credits: 2

This ensemble-based course explores the intersection of live performance, experimental soundscapes, and dub aesthetics. Rooted in the traditions of dub music—including remix culture, delay and reverb manipulation, and bass-driven textures—students will create immersive sonic environments using a mix of acoustic instruments, electronic tools, field recordings, and live effects processing.

Readings in Sound — MSR2214.01

Instructor: Cristian Amigo
Days & Time: TU 4:10pm-6:00pm
Credits: 2

This seminar course investigates the cultural, philosophical, and aesthetic dimensions of sound through critical readings, listening exercises, and discussions. Drawing from fields such as sound studies, media theory, musicology, literature, and art, Readings in Sound challenges students to consider how sound shapes experience, knowledge, identity, and space.

Tickling the Clock — MSR4375.01

Instructor: Nicholas Brooke
Days & Time: TU 4:10pm-6:00pm
Credits: 2

An advanced course in sonic contraptions, for students who have already completed significant work in sound, visual design, or project management.  Starting with Collins’ Hardware Hacking, we’ll review soldering, circuit bending (i.e. “tickling the clock”), and associated topics, such as no-input mixing and basic circuit tinkering. We will look at alternative methods of physical sound creation through programming languages and mechanical paradigms such as solenoids and sensors.

Advanced Observing Projects — PHY4326.01

Instructor: Hugh Crowl
Days & Time: MO 3:40pm-5:30pm
Credits: 2

Students will observe using the telescopes at Stickney Observatory for a series of astronomical observing projects. After a range of initial assigned projects designed to acquaint students with the capabilities of the observing equipment and astrophysically interesting observations, students will propose and carry out their own observing projects looking at astrophysical phenomena of interest to them. As this is a projects class, it is expected that students will be able to devote significant time (mostly at night) observing on their own or in small teams.