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Trigger of Standard and Blowout Solar Jets: I. Parametric Studies of the Magnetic Field GeometryContext. Jets are dynamic, impulsive, well collimated plasma events developing at many different scales and in differentlayers of the solar atmosphere.Aims. Jets are believed to be induced by magnetic reconnection a process central to many astrophysical phenomena.Studying their dynamics can help us to better understand the processes acting in larger eruptive events (e.g. flares andcoronal mass ejection) as well as mass, magnetic helicity and energy transfer at all scale in the solar atmosphere. Therelative simplicity of their magnetic geometry and topology, compared with larger solar active events, makes jets idealcandidate for studying the fundamental role of reconnection in energetic events. Methods. In this study, using our state-of-the-art numerical solver ARMS, we present several parametric studies of anumerical three-dimensional magneto-hydrodynamic model of solar jet-like events. We study the impact of the magneticfield inclination and photospheric field distribution on the generation and properties of two types of observed solar jets:the so-called standard and blowout jets.Results. The present parametric studies validate our model of jets for different geometric properties of the magneticconfiguration. On one hand, a blowout jets is eventually always trigger for the range of parameters that we tested. The3D magnetic null-point configuration is a very robust structure for the energy storage and impulsive release characteristicof blowout jets. On the other hand, the existence of the standard jet depends on the magnetic geometry. We show thatthe reconnection occurring during the standard jet phase influences the properties of the trigger of the blowout jet.Conclusions. Our results allow us to better understand the energization, triggering and driving processes of standardand blowout jets. Our model allows us to predict the impulsiveness and energetics of jets in terms of the surroundingmagnetic field configuration. Finally we discuss the interpretation of standard jets and blowout jets and the physicalfactors that determine which type of jets will occur.
Document ID
20190027306
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Pariat, E.
(Observatoire de Paris Paris, France)
Dalmasse, K.
(Observatoire de Paris Paris, France)
Devore, C. R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Antiochos, S. K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Karpen, J. T.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
July 15, 2019
Publication Date
May 14, 2014
Publication Information
Publication: Astronomy & Astrophysics
Publisher: EDP Sciences
Volume: 573
ISSN: 0004-6361
e-ISSN: 1432-0746
Subject Category
Solar Physics
Report/Patent Number
GSFC-E-DAA-TN21036
Report Number: GSFC-E-DAA-TN21036
ISSN: 0004-6361
E-ISSN: 1432-0746
Distribution Limits
Public
Copyright
Other

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