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The code they are developing helps address issues in the data that made it difficult for proper analysis. Hugo Mettes is working with mentors at the National Center for Atmospheric Research’s High Altitude Observatory to modernize data from Skylab, a 1973 NASA mission that collected some of the first data on coronal mass ejections.

The model will help scientists understand the complex physics that take place in Earth’s plasmasphere. This summer, Max Doering is developing a machine-learning model at LASP to predict high-energy particles in space.

Machine-learning models are becoming increasingly important for predicting space phenomena.

Reese Van Putten is spending the summer at LASP developing a new conductance model that will allow scientists to systematically asses the model’s accuracy and limitations. (1987) empirical model has been widely applied by the space physics community to study auroral electron precipitation, the accuracy of its formulas remains unclear. This package will be used to process data coming from the upcoming Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission.

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While working at the Southwest Research Institute, Bryce Walbridge is developing a new universal polarization-resolving software package for solar coronal and heliospheric observations.This method can be applied to coronal observations from future instruments, such as DKIST Cryo-NIRSP. Kaitlyn Hemauer is working at the National Center for Atmospheric Research’s High Altitude Observatory to investigate the line-of-sight effects that manifest when observing coronal eruptions.These are difficult to observe but can provide insight into the energy and configuration of the magnetic field from eruptive solar events. While working at the National Solar Observatory, Carter Woodson is utilizing code to synthesize polarized coronal emission spectra.National Solar Observatory student Garrett Zills is investigating the wavelength variability diagnostics in the chromosphere to help gain a better understanding of its magnetic structure. Understanding the long-term variability in the Sun’s chromosphere is necessary to improve our knowledge of flares and other solar phenomena.Student Mackenzie Baird is working with National Solar Observatory scientists to investigate the Sun’s high-degree acoustic mode frequencies during multiple solar cycles to improve our understanding of the connection between the Sun’s interior and its atmosphere.During the final two weeks, the students are meeting in person in Boulder, where they’re completing their research projects and presenting their results in oral and poster sessions.

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The students spent the following weeks conducting research online and participating in professional development sessions, covering topics such as how to apply to graduate school and creating “elevator pitches” for their projects. This year, the program began virtually, with students spending the first week participating in an intense solar and space physics summer school to cover the basics of their research projects. This program, which began in 2007, is managed by the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado Boulder and the National Solar Observatory and involves eight solar-science institutes in the region. This summer 18 students are participating in the Boulder Solar Alliance Research Experience for Undergraduates (BSA REU) program, which offers students from a wide variety of backgrounds the opportunity to participate in scientific research guided by professional mentors.