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mSWiM - Home

Welcome to the Michigan Solar Wind Model (mSWiM) site! MSWiM was developed in order to provide solar wind conditions at a range of solar system objects beyond Earth’s orbit. The model calculates solar wind conditions using measurements from near Earth orbit spacecraft as input and propagates these conditions radially outward to various solar system objects using a 1-D MHD model. The output of the model is freely available. However, we do ask that you register. 2015 Regents of the University of Michigan.

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mSWiM - Home | mswim.engin.umich.edu Reviews

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Welcome to the Michigan Solar Wind Model (mSWiM) site! MSWiM was developed in order to provide solar wind conditions at a range of solar system objects beyond Earth’s orbit. The model calculates solar wind conditions using measurements from near Earth orbit spacecraft as input and propagates these conditions radially outward to various solar system objects using a 1-D MHD model. The output of the model is freely available. However, we do ask that you register. 2015 Regents of the University of Michigan.

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mSWiM - Home | mswim.engin.umich.edu Reviews

https://mswim.engin.umich.edu

Welcome to the Michigan Solar Wind Model (mSWiM) site! MSWiM was developed in order to provide solar wind conditions at a range of solar system objects beyond Earth’s orbit. The model calculates solar wind conditions using measurements from near Earth orbit spacecraft as input and propagates these conditions radially outward to various solar system objects using a 1-D MHD model. The output of the model is freely available. However, we do ask that you register. 2015 Regents of the University of Michigan.

INTERNAL PAGES

mswim.engin.umich.edu

1

mSWiM - Data Use Policy

http://mswim.engin.umich.edu/data_use.php

MSWiM Data Use Policy. Model results are freely available after registration. We ask that you register because it helps us to know how many people use the model results and for what purpose. In addition, registration allows us to notify users about any errors that we find or of new releases of results. Zieger, B. and K.C. Hansen (2008). Statistical validation of a solar wind propagation model from 1 to 10 AU", J. Geophys. Res.,. Http:/ mswim.engin.umich.edu/. We have worked hard to ensure that the mSWiM ...

2

mSWiM - Home

http://mswim.engin.umich.edu/index.php

Welcome to the Michigan Solar Wind Model (mSWiM) site! MSWiM was developed in order to provide solar wind conditions at a range of solar system objects beyond Earth’s orbit. The model calculates solar wind conditions using measurements from near Earth orbit spacecraft as input and propagates these conditions radially outward to various solar system objects using a 1-D MHD model. The output of the model is freely available. However, we do ask that you register. 2016 Regents of the University of Michigan.

3

mSWiM - Validation

http://mswim.engin.umich.edu/validation.php

MSWiM has been extensively validated on a statistical basis using 12 years of Pioneer, Voyager, Ulysses and Cassini data from 3.5 to 10 AU [Zieger and Hansen, 2008]. Main statistical results to keep in mind:. The most accurately predicted solar wind variable is the solar wind velocity. The IMF magnitude, density and the tangential component of IMF (B. Poor as shown by the hardly significant correlations between predicted and observed B. Finally the user must remember that B. Thus the highest prediction e...

4

mSWiM - Model

http://mswim.engin.umich.edu/model.php

Solar Wind Propagation Model. MSWiM is a 1.5-D ideal MHD model implemented with the Versatile Advection Code (VAC), a general software package designed to solve a conservative system of hyperbolic partial differential equations with additional non-hyperbolic source terms [Tóth, 1996]. The model propagates the solar wind plasma radially outward from the Earth´s orbit at a selected helioecliptic longitude in the inertial frame of reference assuming spherical symmetry. In RTN coordinate system as a function...

5

mSWiM - FAQ

http://mswim.engin.umich.edu/mswim_faq.php

Frequently Asked Questions (FAQ). PLEASE, PLEASE, PLEASE READ THE VALIDATION PAPER. It answers the vast majority of the most common questions users have. Why is Br a constant in the files? The short answer is that Div B = 0. Remember we are doing a 1-D propagation and are therefore assuming that there are no gradients in the direction perpendicular to the direction of propagation. Think about this in Cartesian coordinates, taking the direction of propagation to be the z direction,. We specifically use th...

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csem.engin.umich.edu

CSEM - SWMF Home

http://csem.engin.umich.edu/tools/swmf

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. SWMF - Space Weather Modeling Framework. SWMF development is funded by grants from the following organizations:. Astronauts are vulnerable to energetic radiation. Disruption in GPS navigation systems. Massive disruptions in electric power distribution systems. CSEM is developing the capability with SWMF which will enable the implementa...

csem.engin.umich.edu

CSEM - Tomography

http://csem.engin.umich.edu/tools/tomography

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - MMS

http://csem.engin.umich.edu/tools/MMS

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - GITM

http://csem.engin.umich.edu/tools/GITM

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - People

http://csem.engin.umich.edu/people/index.php

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. CSEM has an assemblage of faculty from around the world who are experts in their fields, staff that keep our operations moving. CSEM's partners span the globe and contribute their own expertise to our organization. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - Geospace/ITM

http://csem.engin.umich.edu/projects/geospace.php

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - Missions

http://csem.engin.umich.edu/missions/index.php

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. To become the first spacecraft to orbit Mercury, MESSENGER followed a path through the inner solar system, including one flyby of Earth, two flybys of Venus, and three flybys of Mercury. This impressive journey is returning the first new spacecraft data from Mercury since the Mariner 10 mission over 30 years ago.

csem.engin.umich.edu

CSEM - HEIDI

http://csem.engin.umich.edu/tools/HEIDI

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. 2016 Regents of the University of Michigan.

csem.engin.umich.edu

CSEM - Center for Space Environment Modeling

http://csem.engin.umich.edu/tools/FDIPS

Models and Tools Index. ICES - Inner Coma Environment Simulator. MSWiM - Michigan Solar Wind Model. MAPSview - MAPS Key Parameter Database. VMR - Virtual Model Repository. FDIPS - Finite Difference Iterative Potential-field Solver. FDIPS is a Finite Difference Iterative Potential-field Solver that can generate the 3D potential magnetic field solution based on a magnetogram. FDIPS is written in Fortran 90 and it uses the MPI library for parallel execution. FDIPS v1.2.tgz.

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mSWiM - Home

Welcome to the Michigan Solar Wind Model (mSWiM) site! MSWiM was developed in order to provide solar wind conditions at a range of solar system objects beyond Earth’s orbit. The model calculates solar wind conditions using measurements from near Earth orbit spacecraft as input and propagates these conditions radially outward to various solar system objects using a 1-D MHD model. The output of the model is freely available. However, we do ask that you register. 2015 Regents of the University of Michigan.

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