A new class of discontinuous solar wind solutions (original) (raw)

The formation of a standing shock in a polytropic solar wind model within 1–10 R s

Shadia Habbal

Journal of Geophysical Research, 1985

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A Review on Solar Wind Modeling: Kinetic and Fluid Aspects

Joseph Lemaire

Surveys in Geophysics, 2011

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Self-consistent and Time-dependent Solar Wind Models

Robert Rosner

The Astrophysical Journal, 1997

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Transient response of the solar wind to changes in flow geometry

Siraj Hasan

Solar Physics, 1982

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Stability Analysis of the Polytropic Solar Wind

Utpal Deka

Canadian Journal of Physics, 2014

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Fitting of hydrodynamic and kinetic solar wind models

Joseph Lemaire

Planetary and Space Science, 1977

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A polytropic model for the solar wind

Stefaan Poedts

Advances in Space Research, 2011

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Model for vortex turbulence with discontinuities in the solar wind

Brahmananda Dasgupta

Nonlinear Processes in Geophysics, 2003

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A three-dimensional model of corotating streams in the solar wind, 1. Theoretical foundations

Razia Parveen

Journal of Geophysical Research, 1978

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On Solutions in the Hydrodynamic Approximation of Solar and Stellar Winds with Viscosity

Xenophon Moussas

Physics International, 2014

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A Generalized Equatorial Model for the Accelerating Solar Wind

Iver Cairns

Journal of Geophysical Research: Space Physics, 2018

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Three-Fluid, Three-Dimensional Magnetohydrodynamic Solar Wind Model with Eddy Viscosity and Turbulent Resistivity

Melvyn Goldstein

The Astrophysical Journal, 2014

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Half a Century of Kinetic Solar Wind Models

Joseph Lemaire

2010

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Numerical simulations to study solar wind turbulence

himanshu singh

Physics of Plasmas, 2011

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Flow properties of the solar wind derived from a two-fluid model with constraints from white light and in situ interplanetary observations

madhulika guhathakurta

Geophysical Research Letters, 1995

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Flow shear across solar wind discontinuities: WIND observations

Johan De Keyser

Geophysical Research Letters, 1998

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Solar Wind Modeling with Turbulence Transport and Heating

Melvyn Goldstein

The Astrophysical Journal, 2011

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How does the solar wind blow? A simple kinetic model

N. Meyer-vernet

European journal of physics, 1999

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APPLICATION OF A SOLAR WIND MODEL DRIVEN BY TURBULENCE DISSIPATION TO A 2D MAGNETIC FIELD CONFIGURATION

Roberto Lionello

The Astrophysical Journal, 2014

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Further Criteria for the Existence of Steady Line‐driven Winds

Nicolas Pereyra

The Astrophysical Journal, 2005

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A Semiempirical Magnetohydrodynamical Model of the Solar Wind

Igor Sokolov

The Astrophysical Journal, 2007

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Dissipation-scale turbulence in the solar wind

Steven Cowley

AIP Conference Proceedings, 2007

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Propagation of LongitudinalWaves in Super-Radially Expanding Solar Plumes

Jordan A Guerra A

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An application of the turbulent magnetohydrodynamic residual-energy equation model to the solar wind

Nobumitsu Yokoi

Physics of Plasmas, 2007

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Blob formation and acceleration in the solar wind: role of converging flows and viscosity

Giovanni Lapenta

Annales Geophysicae, 2008

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Heating the Solar Wind by a Magnetohydrodynamic Turbulent Energy Cascade

Luca Sorriso-Valvo

Astrophysical Journal, 2008

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A global 2.5‐dimensional three fluid solar wind model with alpha particles

Xing Li

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