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OSPPARIS 40M: An Intro to Making: What is EE

Is a hands-on class where students learn to make stuff. Through the process of building, you are introduced to the basic areas of EE. Students build a "useless box" and learn about circuits, feedback, and programming hardware, a light display for your desk and bike and learn about coding, transforms, and LEDs, a solar charger and an EKG machine and learn about power, noise, feedback, more circuits, and safety. And you get to keep the toys you build. Prerequisite: CS 106A.
Terms: Aut, Spr | Units: 5 | UG Reqs: WAY-SMA

OSPPARIS 50M: Introductory Science of Materials

Topics include: the relationship between atomic structure and macroscopic properties of man-made and natural materials; mechanical and thermodynamic behavior of surgical implants including alloys, ceramics, and polymers; and materials selection for biotechnology applications such as contact lenses, artificial joints, and cardiovascular stents. No prerequisite.
Terms: Aut, Win, Spr | Units: 4 | UG Reqs: GER:DB-EngrAppSci, WAY-AQR, WAY-SMA

OSPPARIS 53: Electricity, Magnetism and Optics with Laboratory

How are electric and magnetic fields generated by static and moving charges, and what are their applications? How is light related to electromagnetic waves? Represent and analyze electric and magnetic fields to understand electric circuits, motors, and generators. Wave nature of light to explain interference, diffraction, and polarization phenomena; geometric optics to understand how lenses and mirrors form images. Workings and limitations of optical systems such as the eye, corrective vision, cameras, telescopes, and microscopes. Discussions based on the language of algebra and trigonometry. An integrated version of Physics 23 and 24, targeted to premedical students who are studying abroad with integrated labs. Prerequisite: PHYSICS 21 or 21S. This course meets the STEM track requirement for the Paris Program during Winter Quarter 2019-2020.
Terms: Win | Units: 5 | UG Reqs: WAY-SMA
Instructors: Desprat, N. (PI)

OSPSANTG 58: Living Chile: A Land of Extremes

Physical, ecological, and human geography of Chile. Perceptions of the Chilean territory and technologies of study. Flora, fauna, and human adaptations to regional environments. Guest lectures; field trips; workshops.
Terms: Spr, Sum | Units: 5 | UG Reqs: GER:DB-EngrAppSci, WAY-SMA
Instructors: Reid, S. (PI)

OSPSANTG 85: Marine Ecology of Chile and the South Pacific

Relationships among physical processes in the ocean, biological productivity, and the exploitation of resources by high-thropic-level predators including human beings. Characterization of ecological patterns; identification of processes operating on marine systems. Open ocean ecosystems, intertidal and benthic regions of the world's oceans, and ecological research developed along coastal regions, focusing on Chile's 4,000 km coastline.
Terms: Aut | Units: 5 | UG Reqs: GER: DB-NatSci, WAY-SMA

PEDS 51N: How Discovery and Innovation Have Transformed Medicine

Topics include the science behind vaccines and why some refuse vaccination, how antibiotics are discovered and what can be done about increasing resistance to antibiotics, stem cells and their potential use, the role of genomics in modern medicine, development of drugs to treat HIV/AIDS, discovery of surfactant, personal responsibility in health and wellness and how technology relates to the "cost conundrum" of healthcare in the U.S. Appreciate important connections between science, discovery and human health and think critically about the potential impact of new discoveries on life and death, and their ethical and spiritual boundaries.
Last offered: Spring 2016 | UG Reqs: WAY-SMA

PHIL 165: Philosophy of Physics: Quantum Mechanics (PHIL 265)

Graduate students register for 265.nnPREREQUISITES: No detailed knowledge of quantum physics or advanced mathematics is presumed. Some background in philosophy, natural science or mathematics will be helpful. Students will benefit from possession of a modicum of mathematical maturity (roughly equivalent to a familiarity with elementary single-variable calculus or the metatheory of first-order logic).
Terms: Win | Units: 4 | UG Reqs: GER:DB-Hum, WAY-A-II, WAY-SMA | Repeatable for credit

PHYSICS 14N: Quantum Information: Visions and Emerging Technologies

What sets quantum information apart from its classical counterpart is that it can be encoded non-locally, woven into correlations among multiple qubits in a phenomenon known as entanglement. We will discuss paradigms for harnessing entanglement to solve hitherto intractable computational problems or to push the precision of sensors to their fundamental quantum mechanical limits. We will also examine challenges that physicists and engineers are tackling in the laboratory today to enable the quantum technologies of the future.
Terms: Aut, Spr | Units: 3 | UG Reqs: WAY-FR, WAY-SMA

PHYSICS 15: Stars and Planets in a Habitable Universe

Is the Earth unique in our galaxy? Students learn how stars and our galaxy have evolved and how this produces planets and the conditions suitable for life. Discussion of the motion of the night sky and how telescopes collect and analyze light. The life-cycle of stars from birth to death, and the end products of that life cycle -- from dense stellar corpses to supernova explosions. Course covers recent discoveries of extrasolar planets -- those orbiting stars beyond our sun -- and the ultimate quest for other Earths. Intended to be accessible to non-science majors, material is explored quantitatively with problem sets using basic algebra and numerical estimates. Sky observing exercise and observatory field trips supplement the classroom work.
Terms: Aut, Sum | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA

PHYSICS 16: The Origin and Development of the Cosmos

How did the present Universe come to be? The last few decades have seen remarkable progress in understanding this age-old question. Course will cover the history of the Universe from its earliest moments to the present day, and the physical laws that govern its evolution. The early Universe including inflation and the creation of matter and the elements. Recent discoveries in our understanding of the makeup of the cosmos, including dark matter and dark energy. Evolution of galaxies, clusters, and quasars, and the Universe as a whole. Implications of dark matter and dark energy for the future evolution of the cosmos. Intended to be accessible to non-science majors, material is explored quantitatively with problem sets using basic algebra and numerical estimates.
Terms: Win, Sum | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA
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