Seniors | Class of \u2713

PLEASE NOTE: Where applicable, the audio has been removed from this file due to copyrighted material. The garments shown here represent the Senior Class of \u2713. The garments were created in response to the following design challenge: Senior Thesis Collection: create a collection that reflects the essence and philosophies of your personal vision

Juniors | Class of \u2713

PLEASE NOTE: Where applicable, the audio has been removed from this file due to copyrighted material. The garments shown here represent the Junior Class of \u2713. The garments were created in response to the following design challenges: Knitwear Design: explore the properties of knits and design cut-and-sew and machine-knit garments. Costume for Dance: explore the characteristics of knitted fabric as applied to the fit and movement constraints of dance costumes. These garments are displayed on the runway in a dance performance including choreography by Merce Cunningham; re-staged from Brown University\u27s MiniEvent by Daniel Squire; music by Stephan Moore. Tailoring Project: interpret traditional tailoring techniques to create a look with a jacket

Five Design Challenges

PLEASE NOTE: Where applicable, the audio has been removed from this file due to copyrighted material. The garments shown here represent the Classes of \u2713, \u2712 and \u2711 . The garments were created in response to the following five design challenges: Sophomores, Class of \u2713: Re-Innovative Design: explore the properties of recycled materials other than fabric while creating a wearable piece. Print Design Project create a garment that makes optimal use of printed fabric designed by a RISD Textiles student. Juniors, Class of \u2712: Knitwear Design: explore the properties of knits and design cut-and-sew and machine-knit garments. Tailoring Project: interpret traditional tailoring techniques to create a look with a jacket. Seniors, Class of \u2711: Cocktail Collection: design a collection of contemporary cocktail apparel in collaboration with the current RISD Museum exhibition Cocktail Culture: Ritual and Invention in American Fashion, 1920-1980

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