Predictive Science Inc.
MHDweb - Modeling of Solar Corona & Heliosphere
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Magnetic field input boundary condition
Phi component of magnetic field
Radial component of magnetic field
Theta component of magnetic field
Sound speed
Wave energy density moving anti-parallel to the field
Wave energy density moving parallel to the field
Local coronal heating rate
Phi component of current density
Radial component of current density
Theta component of current density
Output log
Thermal pressure
Density
Temperature
Alfven speed
Phi component of velocity
Radial component of velocity
Theta component of velocity
ZIP file containing all of the above
Simulation result ID:
hmi__high-cor-thermo2-exp01__high-hel-poly-exp01
hmi__high-cor-thermo1-exp01__high-hel-poly-exp01
hmi__high-cor-poly-exp01__high-hel-poly-exp01
Universal date and time (UT)
Date:
/
/
Time:
:
Carrington rotation and longitude
Rotation:
Longitude:
degrees
Solution
Coronal
Heliospheric
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