Summer 2022 REU Projects

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Project type and supervisor
  Project title and brief description
(Click title for details)
ribbon oscillation
Outreach project with  
Angela Des Jardins
  Solar Physics Education: Research and Project Development
Dr. Des Jardins leads the Nationwide Eclipse Ballooning Project (NEBP), which will involve thousands of college students in hands-on research for the October 14, 2023 annular and April 8, 2024 total solar eclipses. In this project, student will develop online modules that the NEBP participants will use to learn about the sun and eclipses.  
reconnection
Data analysis with 
Jiong Qiu
  Properties of Magnetic Reconnection in Solar Flares
Solar flares release a large amount of energy stored in the Sun's magnetic field by a mechanism called magnetic reconnection. In this project, student will analyze state-of-the-art observations of flares by the Solar Dynamics Observatory spacecraft, and measure properites of magnetic reconnection that governs energy release in flares.
Optical instrumentation with
Joe Shaw
  Experimental Studies of Moonlight and Sky Polarization
Dr. Shaw's group has pioneered the use of polarization imaging for atmospheric science. In this project, we will measure scattered moonlight with polarization imaging, and use these measurements to study the atmosphere. Student will participating in making observational measurements and data analysis.
xrt
Data analysis with  
Aki Takeda
  Solar X-ray Irradiance with Hinode/XRT
Our Sun is a variable star, and the amount of its radiation rises and falls every 11 years or so. The radiation from the Sun received at the earth (irradiance) varies over the activity cycle, and also varies with the observing wavelength. In this project, we will derive the long-term variation of the Sun's irradiance in soft X-rays, using a series of full-Sun images observed with the X-Ray Telescope (XRT) aboard the Hinode satellite, which is an international space mission among Japan/US/UK.
flare
Data analysis with 
Chunming Zhu
  Understanding Flare Heating With Multi-wavelength Observations
A solar Flare is an intense burst of radiation in the solar atmosphere. In this project, student will use a novel method developed at MSU, and analyze and model a flare observed by the Solar Dynamics Observatory spacecraft to derive flare energy, and understand heating and cooling of flare plasmas.
flare
Data analysis with 
Anne Lohfink
  Characterizing Compact Jets in Seyfert Galaxies
Accretion onto black holes is one of the most efficient processes for emitting energy from matter in the Universe. Research has shown that this accretion process is also accompanied by ejection processes (winds, relativistic outflows). These accretion and ejection processes are usually assumed to work similarly no matter the size of the black hole. In this project, the student will investigate whether the compact jets seen in accreting supermassive black holes at the centers of galaxies are just bigger versions of those seen in accreting stellar mass black holes.