Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST

By A. Pevtsov, H. Uitenbroek. 2003

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The Solar Optical Telescope for the Hinode Mission: An Overview (2007, background): “The observational signature for either wave heating (and/or resultant shocks) or magnetic reconnection (or both) should be observed with SOT using both photospheric and chromospheric lines with co-temporal magnetograms (Ulmschneider and Musielak, 2003; Carlsson and Stein, 2004).”
On the Generation, Propagation, and Reflection of Alfvén Waves from the Solar Photosphere to the Distant Heliosphere (2004, methodology): “We adopt a 2The magnetic field is assumed to point outward—i.e., it is assumed to be of northern polarity—but the physics is the same for an inward pointing field. slightly modified version of the polar magnetic field configuration of Banaszkiewicz et al. (1998): B0 1.789 G = 2 x3 + 4.281 x5…”
The Sun’s Supergranulation (2010, background): “…solar magnetic fields, from the global solar scales to the smallest scales available to observations, may have a fractal or multifractal structure (Lawrence et al. 1995; Komm 1995; Nesme-Ribes et al. 1996; Meunier 1999; Janßen et al. 2003; Stenflo and Holzreuter 2002, 2003a, b; Abramenko 2005).”
The Daniel K. Inouye Solar Telescope – Observatory Overview (2020, background): “The deepest layers of the photosphere can be observed at a wavelength of 1.6 micron where the opacity of the solar atmosphere has a minimum (Avrett, 2003).”