Amending Amendments: Digital Colonialism, Bill C-11, and Assessing the Call for Improvement

Media scholars Nick Couldry and Ulises Mejias (2019) define digital colonialism as the “term for the extension of a global process of extraction that started under colonialism and continues through industrial capitalism, culminating in today\u27s new form: instead of natural resources in labor, what is now being appropriated is human life through its conversion into data” (p. 22). This research will critically analyze the Canadian government’s ill-received Bill C-11: the Amended Consumer Privacy Protection Act by using digital colonialism as a conceptual framework to reveal the Bill’s essential limitations. It will consist of two sections: 1) an in-depth exploration of the definition of digital colonialism and Indigenous Subjectivity, which will inform the objective, and 2) an examination of amendment recommendations (7, 8, 11 and 15), put forth by the previous Privacy Commissioner Daniel Therrien to improve Bill C-11. By using digital colonial theory and applying it to a critical legislative case study, this research addresses the following questions: What is digital colonialism and how, from a digital colonial standpoint, can we critically unpack the recommended amendments proposed by Therrien

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