Senior Recital: Anthony Newman, cello

This recital is presented in partial fulfillment of requirements for the degree Bachelor of Music in Music Education. Mr. Newman studies cello with Charae Krueger.https://digitalcommons.kennesaw.edu/musicprograms/2006/thumbnail.jp

Non-degree Recital: Ruth Bearden, flute and piccolo

Ms. Bearden studies flute with Cecilia Price.https://digitalcommons.kennesaw.edu/musicprograms/1996/thumbnail.jp

OcTUBAfest! 2017

Octubafest! 2017 recital featuring performances by KSU low brass faculty and students, along with guest artist Brian Meixnert, euphonium.https://digitalcommons.kennesaw.edu/musicprograms/1971/thumbnail.jp

Screening and Addressing Fatigue Symptoms in Patients with Orthopedic Problems Using the PROMIS Fatigue Scale

In the primary care setting, fatigue is a common complaint, outnumbered only by cough. 41.9% of patients in an outpatient physical therapy setting reported unacceptable fatigue. Fatigue scores are weakly correlated to physical function and pain interference (using Patient Reported Outcome Measurement Information Systems [PROMIS]). Therefore, detecting fatigue and addressing it directly is necessary

Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies

Flare frequency distributions represent a key approach to addressing one of the largest problems in solar and stellar physics: determining the mechanism that counter-intuitively heats coronae to temperatures that are orders of magnitude hotter than the corresponding photospheres. It is widely accepted that the magnetic field is responsible for the heating, but there are two competing mechanisms that could explain it: nanoflares or Alfv\'en waves. To date, neither can be directly observed. Nanoflares are, by definition, extremely small, but their aggregate energy release could represent a substantial heating mechanism, presuming they are sufficiently abundant. One way to test this presumption is via the flare frequency distribution, which describes how often flares of various energies occur. If the slope of the power law fitting the flare frequency distribution is above a critical threshold, $\alpha=2$ as established in prior literature, then there should be a sufficient abundance of nanoflares to explain coronal heating. We performed $>$600 case studies of solar flares, made possible by an unprecedented number of data analysts via three semesters of an undergraduate physics laboratory course. This allowed us to include two crucial, but nontrivial, analysis methods: pre-flare baseline subtraction and computation of the flare energy, which requires determining flare start and stop times. We aggregated the results of these analyses into a statistical study to determine that $\alpha = 1.63 \pm 0.03$. This is below the critical threshold, suggesting that Alfv\'en waves are an important driver of coronal heating.Comment: 1,002 authors, 14 pages, 4 figures, 3 tables, published by The Astrophysical Journal on 2023-05-09, volume 948, page 7