Transcultural engagement with Polish memory of the Holocaust while watching Leszek Wosiewicz's Kornblumenblau

Kornblumenblau (Leszek Wosiewicz 1989) is a film that explores the experience of a Polish political prisoner interned at Auschwitz I. It particularly foregrounds issues related to Polish-Jewish relations during the Holocaust in its diegesis. Holocaust films are often discussed in relation to representation and the cultural specificity of their production context. However, this paper suggests thinking about film and topographies, the theme of this issue, not in relation to where a work is produced but in regards to the spectatorial space. It adopts a phenomenological approach to consider how, despite Kornblumenblau's particularly Polish themes, it might address the transcultural spectator and draw attention to the broader difficulties one faces when attempting to remember the Holocaust. Influenced particularly by the writing of Jennifer M. Barker and Laura U. Marks, this paper suggests that film possesses a body ¬¬- a display of intentionality, beyond those presented within the diegesis, which engages in dialogue with the spectator. During the experience of viewing Kornblumenblau, this filmic corporeality draws attention to the difficulties of confronting the Holocaust in particularly haptic ways, as the film points to the unreliability of visual historical sources, relates abject sensations to concentrationary spaces and breaks down as it confronts the scene of the gas chamber

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