| Spherical harmonic coefficients | lon,lat,br,bt,bp,|B| as ASCII on 1 degree grid | |B| as GMT grid (for gridview, for example) | |
|---|---|---|---|
| Sequential model | download | download | |
| Coestimation model | download | download | |
| Correlative model | download | download | download |
The sequential model is based on the internal field (BrI,BtI,BpI) from wake (sun=1) and tail (GSE from 160 to 200) times. It can be downloaded
here.
Note: The lunar magnetic field models here have been evaluated at 30 km altitude to spherical harmonic degree 170. The full-wavelength resolution of the model is about 64 km at low and mid-latitudes.
Note: The lunar magnetic field models here have been evaluated at 30 km altitude to spherical harmonic degree 170. The full-wavelength resolution of the model is about 64 km at low and mid-latitudes.
Correlative lunar magnetic field model at 30 km altitude
