Search Results - "ZANK, G"
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1
Parker Solar Probe Enters the Magnetically Dominated Solar Corona
Published in Physical review letters (17-12-2021)“…The high temperatures and strong magnetic fields of the solar corona form streams of solar wind that expand through the Solar System into interstellar space…”
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2
Faltering Steps Into the Galaxy: The Boundary Regions of the Heliosphere
Published in Annual review of astronomy and astrophysics (01-01-2015)“…The interaction of the heliosphere with the local interstellar medium (LISM) results in a complicated series of boundary regions. The Voyager 1 and 2…”
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3
Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence
Published in The Astrophysical journal (01-02-2017)“…The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed largely in the early 1990s, together with an important extension to…”
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4
Electron Acceleration from Expanding Magnetic Vortices During Reconnection with a Guide Field
Published in The Astrophysical journal (20-01-2020)“…Magnetic reconnection is believed to be responsible for the acceleration of energetic electrons with a power-law spectrum in the solar wind and solar flares…”
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5
The Origin of Switchbacks in the Solar Corona: Linear Theory
Published in The Astrophysical journal (01-11-2020)“…Abstract The origin, structure, and propagation characteristics of a switchback are compelling questions posed by Parker Solar Probe (PSP) observations of…”
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6
Compressible and Incompressible Magnetic Turbulence Observed in the Very Local Interstellar Medium by Voyager 1
Published in The Astrophysical journal (20-12-2019)“…Voyager 1 observed Kolmogorov-like (k−5/3) compressible turbulence just upwind of the heliopause. Subsequent measurements by Voyager 1 further from the…”
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7
A Solar Coronal Hole and Fast Solar Wind Turbulence Model and First-orbit Parker Solar Probe (PSP) Observations
Published in The Astrophysical journal (01-10-2020)“…Abstract We propose a turbulence-driven solar wind model for a fast solar wind flow in an open coronal hole where the solar wind flow and the magnetic field…”
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8
On the Parallel and Oblique Firehose Instability in Fluid Models
Published in The Astrophysical journal (10-04-2017)“…A brief analysis of the proton parallel and oblique firehose instability is presented from a fluid perspective, and the results are compared with kinetic…”
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9
Spectral Anisotropy in 2D plus Slab Magnetohydrodynamic Turbulence in the Solar Wind and Upper Corona
Published in The Astrophysical journal (01-09-2020)“…The 2D + slab superposition model of solar wind turbulence has its theoretical foundations in nearly incompressible magnetohydrodynamics (NI MHD) in the plasma…”
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10
Self-consistent Energetic Particle Acceleration by Contracting and Reconnecting Small-scale Flux Ropes: The Governing Equations
Published in The Astrophysical journal (10-09-2018)“…Previous application of our focused transport equation for energetic ion test particle acceleration by numerous active small-scale flux ropes to solar wind…”
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11
The Role of Magnetic Reconnection-associated Processes in Local Particle Acceleration in the Solar Wind
Published in The Astrophysical journal (01-03-2019)“…Recent studies of unusual or atypical energetic particle flux events (AEPEs) observed at 1 au show that another mechanism, different from diffusive shock…”
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12
Turbulence-dominated Shock Waves: 2D Hybrid Kinetic Simulations
Published in The Astrophysical journal (01-02-2022)“…Abstract We investigate the interaction of turbulence with shock waves by performing 2D hybrid kinetic simulations. We inject force-free magnetic fields…”
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13
The Transport of Low-frequency Turbulence in Astrophysical Flows. I. Governing Equations
Published in The Astrophysical journal (20-01-2012)“…Numerous problems in space physics and astrophysics require a detailed understanding of the transport and dissipation of low-frequency turbulence in an…”
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14
A KINETIC TRANSPORT THEORY FOR PARTICLE ACCELERATION AND TRANSPORT IN REGIONS OF MULTIPLE CONTRACTING AND RECONNECTING INERTIAL-SCALE FLUX ROPES
Published in The Astrophysical journal (10-03-2015)“…Simulations of particle acceleration in turbulent plasma regions with multiple contracting and merging (reconnecting) magnetic islands emphasize the key role…”
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15
Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence. IV. Solar Coronal Turbulence
Published in The Astrophysical journal (10-02-2018)“…A new model describing the transport and evolution of turbulence in the quiet solar corona is presented. In the low plasma beta environment, transverse…”
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16
II. Transport of Nearly Incompressible Magnetohydrodynamic Turbulence from 1 to 75 au
Published in The Astrophysical journal (01-06-2017)“…The thermal plasma beta in the solar wind and the solar corona is of the order of and . Zank et al. developed 2D and slab turbulence transport model equations…”
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17
The Pickup Ion-mediated Solar Wind
Published in The Astrophysical journal (10-12-2018)“…The New Horizons Solar Wind Around Pluto (NH SWAP) instrument has provided the first direct observations of interstellar and He pickup ions (PUIs) at distances…”
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18
Particle-in-cell simulations – ion beam instabilities and the generation of Alfvén and whistler waves in low β plasma
Published in Monthly notices of the Royal Astronomical Society (29-09-2023)“…ABSTRACT Ion beam-driven instabilities in a collisionless space plasma with low β, i.e. low plasma and magnetic pressure ratio, are investigated using…”
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A Focused Transport-based Kinetic Fractional Diffusion-advection Equation for Energetic Particle Trapping and Reconnection-related Acceleration by Small-scale Magnetic Flux Ropes in the Solar Wind
Published in The Astrophysical journal (01-06-2021)“…Abstract Analysis of energetic particle inner heliospheric spacecraft data increasingly suggests the existence of anomalous diffusion phenomena that should be…”
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20
The Origin of Compressible Magnetic Turbulence in the Very Local Interstellar Medium
Published in The Astrophysical journal (20-06-2017)“…Voyager 1 observed compressible magnetic turbulence in the very local interstellar medium (VLISM). We show that inner heliosheath (IHS) fast- and slow-mode…”
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