Corrected Geomagnetic Coordinates and IGRF/DGRF Model Parameters
This service enables computation of a set of the main geomagnetic
field model parameters and transformation from the GEOcentric spherical
(geographic) coordinates to the Corrected GeoMagnetic (CGM) coordinates
and vice versa. The algorithm is solely based on the DGRF/IGRF
geomagnetic field models for Epochs 1900-2025. The B-min approach is
applied to calculate CGM coordinates through the near-equator area
where the definition of CGM coordinates is invalid. However, GEO <--> CGM
transformations are not performed at certain regions where the CGM equator
cannot be defined at all.
The following output parameters are calculated:
- GEOCENTRIC, CGM, and footprint coordinates of a given point
- DGRF/IGRF magnetic field components H (nT), D (deg.), and
Z (nT) at this pointand its conjugate point
- Geocentric and CGM coordinates of the magnetically conjugate
point and the magnetic field line footprint
- DGRF/IGRF magnetic field components H (nT), D (deg.), and
Z (nT) at footprint point and its conjugate point
- Apex of the magnetic field line: the point at a maximum distance
- UT at time when given point is at midnight (MLT)
- Meridian_angle: the azimuth along a great-circle arc to the North
(South) CGM pole measured from the geographic North (South)
meridian; positive to East (West)
- Oval_angle: the angle between local tangents to the CGM and
geographic (geocentric) latitudes;
Brief Description of CGM and Associated MLT Definition
Select input parameters
Find Tsyganenko N modeling HERE
Geomagnetic Field Models, Maps, and Software
https://www.ngdc.noaa.gov/geomag/models.shtml
If you have any questions/comments contact:
Dr. Vladimir Papitashvili, c/o
Dr. Natalia Papitashvili, E-mail:
Natalia.E.Papitashvili@nasa.gov, Space Physics Data Facility, Mail Code 672, NASA/Goddard Space Flight Center,
Greenbelt, MD 20771
NASA Official: Dr. Robert Candey, Head of the Space Physics Data Facility