Unifying the Validation of Ambient Solar Wind Models

  title={Unifying the Validation of Ambient Solar Wind Models},
  author={Martin A. Reiss and Karin Muglach and R. E. Mullinix and Maria M. Kuznetsova and Chiu P. Wiegand and Manuela Temmer and Charles N. Arge and Sergio Dasso and Shing F. Fung and Jos{\'e} Juan Gonz{\'a}lez Avil{\'e}s and Siegfried Gonzi and Lan K. Jian and Peter J. MacNeice and Christian Mostl and Mathew J. Owens and Barbara Perri and Rui F. Pinto and Lutz Rastatter and Pete Riley and Evangelia Samara and Iswat H1-01 Team Members},
  journal={Advances in Space Research},
1 Citations

Figures and Tables from this paper

CME Evolution in the Structured Heliosphere and Effects at Earth and Mars During Solar Minimum

The activity of the Sun alternates between a solar minimum and a solar maximum, the former corresponding to a period of “quieter” status of the heliosphere. During solar minimum, it is in principle



Comprehensive Assessment of Models and Events Using Library Tools (CAMEL) Framework: Time Series Comparisons

The Comprehensive Assessment of Models and Events using Library Tools (CAMEL) framework leverages existing Community Coordinated Modeling Center services: Run‐on‐Request postprocessing tools that

Air Force Data Assimilative Photospheric Flux Transport (ADAPT) Model

As the primary input to coronal and solar wind models, global estimates of the solar photospheric magnetic field distribution are critical to space weather forecasting. These global magnetic maps are

Coronal Magnetic Field

Validation of community models: 2. Development of a baseline using the Wang‐Sheeley‐Arge model

This paper is the second in a series providing independent validation of community models of the outer corona and inner heliosphere. Here I present a comprehensive validation of the Wang‐Sheeley‐Arge

Verification of high‐speed solar wind stream forecasts using operational solar wind models

High‐speed solar wind streams emanating from coronal holes are frequently impinging on the Earth's magnetosphere causing recurrent, medium‐level geomagnetic storm activity. Modeling high‐speed solar

Assessing the Influence of Input Magnetic Maps on Global Modeling of the Solar Wind and CME‐Driven Shock in the 2013 April 11 Event

In the past decade, significant efforts have been made in developing physics‐based solar wind and coronal mass ejection (CME) models, which have been or are being transferred to national centers

Theoretical Refinements to the Heliospheric Upwind eXtrapolation Technique and Application to in-situ Measurements

The large-scale structure and evolution of the solar wind are typically reproduced with reasonable fidelity using three-dimensional magnetohydrodynamic (MHD) models. However, such models are

On the Sources and Sizes of Uncertainty in Predicting the Arrival Time of Interplanetary Coronal Mass Ejections Using Global MHD Models

Accurate predictions of the properties of interplanetary coronal mass ejection (ICME)‐driven disturbances are a key objective for space weather forecasts. The ICME's time of arrival (ToA) at Earth is

The role of Alfvén wave dynamics on the large scale properties of the solar wind: comparing a MHD simulation with PSP E1 data

During Parker Solar Probe’s first orbit, the solar wind plasma has been observed in situ closer than ever before, the perihelion on November 6th 2018 revealing a flow that is constantly permeated by