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Reconciling Observational Challenges to the Impulsive-Piston Shock-Excitation Scenario. II. Shock Waves Produced in CME-Less Events with a Null-Point Topology
Authors:Grechnev  V V  Kiselev  V I  Uralov  A M  Myshyakov  I I
Institution:1.NorthWest Research Associates, Boulder, CO, USA
;2.Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi, Japan
;3.W.W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA, USA
;4.Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
;5.Rosseland Centre for Solar Physics, University of Oslo, Blindern, Oslo, Norway
;6.LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon, France
;7.University of Michigan, Ann Arbor, MI, USA
;
Abstract:Solar Physics - The problem of bias, meaning over- or under-estimation, of the component perpendicular to the line-of-sight $B_{\perp }$ ] in vector magnetic-field maps is discussed. Previous...
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