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Assessing the Quality of Models of the Ambient Solar Wind

author

Mathew Owens

published in: Space Weather

date of publication: 2018-10-01

Cites articles 76

Date

Title

Authors

2018

Low-frequency Alfven waves produced by magnetic reconnection in the Sun's magnetic carpet
2018

An MHD simulation of solar active region 11158 driven with a time-dependent electric field determined from HMI vector magnetic field measurement data
2018-09-18

The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating

William H. Matthaeus
2018-06-11

Toward a Quantitative Comparison of Magnetic Field Extrapolations and Observed Coronal Loops

Ignacio Ugarte-Urra, Xudong Sun, Markus J. Aschwanden
2018-01-09

Simulating the Coronal Evolution of AR 11437 Using SDO/HMI Magnetograms
2018-08-08

Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse

Miloslav Druckmüller, Ioannis Contopoulos, Gordon Petrie, Tahar Amari, Daniel Seaton
2018

On the extrapolation of magnetohydrostatic equilibria on the Sun
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Nonlinear force-free coronal magnetic stereoscopy
2017

A comparison between physics-based and polytropic MHD models for stellar coronae and stellar winds of solar analogs
2017

Data-constrained coronal mass ejections in a global magnetohydrodynamics model
2017

Testing the accuracy of data-driven MHD simulations of active region evolution
2017

The open flux problem
2017

Alfven Wave turbulence as a coronal heating mechanism: simultaneously predicting the heating rate and the wave-induced emission line broadening
2017-04-19

Probabilistic Solar Wind and Geomagnetic Forecasting Using an Analogue Ensemble or "Similar Day" Approach
2017-03-31

Origin of the Wang–Sheeley–Arge solar wind model
2016

Closed-field coronal heating driven by wave turbulence
2016-03-15

FORWARD: A Toolset for Multiwavelength Coronal Magnetometry

Sarah E. Gibson
2016-05-16

Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption
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On the origins and timescales of geoeffective IMF

Sarah Bentley, Mike Lockwood
2016

Coupling of coronal and heliospheric magnetohydrodynamic models: solution comparisons and verification

Tibor Török
2016

A three-dimensional model of active region 7986: comparison of simulations with observations
2016

Achieving consistent Doppler measurements from SDO/HMI vector field inversions

Spiro K. Antiochos
2016

A generalized two-component model of solar wind turbulence and ab initio diffusion mean-free paths and drift lengthscales of cosmic rays

Horst Fichtner
2015-09-28

The influence of spatial resolution on nonlinear force-free modeling

Xudong Sun, Gherardo Valori, Michael S. Wheatland, Tahar Amari
2015-06

The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona

Keiji Hayashi, Xudong Sun, William P. Abbett
2015-05

Validation for solar wind prediction at Earth: Comparison of coronal and heliospheric models installed at the CCMC
2015-05-01

Dissipation and heating in solar wind turbulence: from the macro to the micro and back again

Sandra Chapman
2015

Alfven wave solar model (AWSoM): proton temperature anisotropy and solar wind acceleration
2015

Limitations of force-free magnetic field extrapolations: Revisiting basic assumptions
2015-12

Effect of uncertainties in solar synoptic magnetic flux maps in modeling of solar wind

Luca Bertello
2015-03

On the role played by magnetic expansion factor in the prediction of solar wind speed
2015

Periodic density structures and the origin of the slow solar wind

Article - wd:Q89539069

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