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Project Descriptions
Spring 2025

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Showing 8 projects out of 8 found. On page 1 out of 1.
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The Background and Transient Observer (BTO) for the Compton Spectrometer and Imager (COSI)

Juan Carlos Martinez Oliveros - Research Scientist, Space Sciences Laboratory

Status: Current Term Now Closed     Weekly Hours: 9-11 hrs     Location: On Campus

Much of the high-energy Universe remains an enigma, with some phenomena that have been discovered—like gamma-ray bursts, magnetar flares, and supernovae— still to be studied, analyzed and better understood. With the development of technology in the soft/medium gamma-ray regime, we are able to “see” the...

 Engineering, Design & Technologies   Mathematical and Physical Sciences

Techniques in Radio Cosmology Instrumentation

Raul Monsalve - Research Scientist, Space Sciences Laboratory

Status: Full- no new appr needed     Weekly Hours: to be negotiated     Location: Off Campus

The Radio Cosmology Group (RCG) at the Space Sciences Laboratory is a leader in the study of the first billion years of the Universe through the design and operation of state-of-the art radio frequency instrumentation to measure radio waves from space. We are seeking an undergraduate research assistant...

 Engineering, Design & Technologies   Mathematical and Physical Sciences

Data Visualization and Selection for NASA’s MMS Mission

Mitsuo Oka - Research Scientist, Space Sciences Laboratory

Status: Check back for status     Weekly Hours: to be negotiated     Location: On Campus

NASA’s Magnetospheric MultiScale (MMS) mission consists of a fleet of four spacecraft orbiting Earth. Since its launch in 2015, it has significantly advanced our understanding of Earth's plasma environment, in particular the electron-scale physics of explosive energy-release phenomena. This summer, NASA began transitioning the fleet formation from the...

 Mathematical and Physical Sciences

Flux Transfer Events in Mercury's magnetosphere

Weijie Sun - Staff Researcher, Space Sciences Laboratory

Status: Full- no new appr needed     Weekly Hours: 6-8 hrs     Location: Off Campus

Flux Transfer Events (FTEs) are transient phenomena that occur at the boundary between the solar wind and a planet’s magnetosphere, where magnetic reconnection allows the exchange of magnetic flux, plasma and energy. Mercury’s magnetosphere is the smallest and most dynamic among the terrestrial planets, due to its proximity to the...

 Mathematical and Physical Sciences

Developing a Model of Hydrogen Scattering from the Surface of the Moon

Paul Szabo - Research Scientist, Space Sciences Laboratory

Status: Current Term Now Closed     Weekly Hours: 9-11 hrs     Location: On Campus

Our Moon is continuously exposed to protons from the solar wind and Earth’s magnetosphere. Upon impact, these ions alter the Moon’s surface and contribute to the formation of water. Some of the protons end up scattered away as neutral hydrogen atoms. Instruments onboard NASA’s IBEX spacecraft have been able to...

 Engineering, Design & Technologies   Mathematical and Physical Sciences

Photon Counting Detector Technology

Anton Tremsin - Research Physicist, Space Sciences Laboratory

Status: Check back for status     Weekly Hours: to be negotiated     Location: Off Campus

The Experimental Astrophysics Group at the Space Sciences Laboratory builds UV detector technology for space-based astronomical instruments as well as supports the development of detector technology for niche, land-based applications (typ. in support of biological, materials, high-energy physics research, etc.). We are currently seeking undergraduates who would...

 Engineering, Design & Technologies   Mathematical and Physical Sciences

Improving the data-analysis pipeline of the COSI space mission with machine learning and more

Andreas Zoglauer - Staff Researcher, Space Sciences Laboratory

Status: Current Term Now Closed     Weekly Hours: 9-11 hrs     Location: On Campus

COSI, the Compton Spectrometer and Imager, is a NASA-funded gamma-ray telescope which is currently under development and scheduled for launch in 2027. It will observe Galactic nucleosynthesis and positron annihilation, as well as the most violent events in our Universe (supernovae, neutron star mergers) and the most extreme...

 Engineering, Design & Technologies   Mathematical and Physical Sciences   Digital Humanities and Data Science

GAPS Antarctic Balloon Payload to Probe Dark Matter Using Galactic Particle Signatures

Andreas Zoglauer - Staff Researcher, Space Sciences Laboratory

Status: Full- no new appr needed     Weekly Hours: 9-11 hrs     Location: On Campus

The General Antiparticle Spectrometer (GAPS) is a NASA high-altitude balloon mission designed to detect messengers of dark matter interactions in the galaxy. Apprentices are needed to participate in development and testing of both hardware and online software as GAPS prepares for a December 2024 launch from Antarctica. GAPS is...

 Engineering, Design & Technologies   Mathematical and Physical Sciences   Digital Humanities and Data Science

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