Note: The CfA Solar REU program now uses Zenodo to archive past student presentations. All presentations are
archived as PDF files, and movies, Powerpoint, and Keynote files can be found at the "Zenodo archive" link. |
Amanda Bacon: "The Prevalence of O IV Density Diagnostics in UV Burst Spectra"
Austin Czyzewski: "Modeling Sigmoidal NOAA Active Region 12665 Using Non Linear Force Free Field"
Marcus Dupont: "Comparative Study of the Solar Wind: Modeling Charge State Distributions in the Heliosphere
Sierra Garza: "The Relationship Between Solar Surface Magnetic Field and Coronal Soft X- Ray Spectra"
Marissa Menzel: "Upgrading Stability of an Airborne Infrared Spectrometer (AIR-Spec) for Coronal Observations"\
Maya Merhi: "Where's That Flare: A Comprehensive Hard X-Ray Solar Flare Catalog"
Paula Moraga: "Constructing a User Interface for the Alignment of CAT Gratings"
Christian Nieves: "Angular Response Characterization of the REgolith X-ray Imaging Spectrometer (REXIS) Solar X-\
ray Monitor (SXM)"
Crisel Suarez: "Solar Flare Plasma Transport Inferred from Elemental Abundance Changes using soft X-ray Spectra"\
German Vazquez Perez: "Improving the Sprectal Fit for the Diffuse Soft X-Ray Background Using ATOMDB Charge Exchange Models"
John Waczak: "Nonequilibrium Ionization Analysis of a Coronal Shock Driven by a Coronal Mass Ejection"
Caption: Two full disk images taken by the X-Ray Telescope
aboard Hinode are taken one solar rotation apart. In the center of the
left hand image are NOAA active regions 10931 and 10932. A rotation
later the active regions have disappeared, but their effect is still
noticeable in the long quiet sun loops. Yohkoh experts can comment on
whether this was commonly seen by SXT. This type of evolution was seen
in Skylab, though not this clearly (1982; ApJ 259, 359-365).