Now showing items 1-3 of 3

  • Osborne, Christopher M. J.; Heinzel, Petr; Kašparová, Jana; Fletcher, Lyndsay (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2021)
    ABSTRACT The forward fitting of solar flare observations with radiation–hydrodynamic simulations is a common technique for learning about energy deposition and atmospheric evolution during these explosive events. ...
  • Young, Peter R.; Tian, Hui; Peter, Hardi; Rutten, Robert; Nelson, Chris J.; Huang, Zhenghua; Schmieder, Brigitte; Vissers, Gregal Joan Maria; Toriumi, Shin; Rouppe van der Voort, Luc; Madjarska, Maria S.; Danilovic, Sanja; Berlicki, Arkadiusz; Chitta, Lakshmi Pradeep; Cheung, Mark C.M.; Madsen, Chad; Reardon, Kevin P.; Katsukawa, Yukio; Heinzel, Petr (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2018)
    The term “ultraviolet (UV) burst” is introduced to describe small, intense, transient brightenings in ultraviolet images of solar active regions. We inventorize their properties and provide a definition based on image ...
  • Carlsson, Mats; Fletcher, Lyndsay; Allred, Joel; Heinzel, Petr; Kašparová, Jana; Kowalski, Adam; Mathioudakis, Mihalis; Reid, Aaron; Simões, Paulo J. A. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2023)
    Context . Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These particles travel along the magnetic field ...