Structural and dynamical features of the ionised and neutral upper atmosphere are strongly organised by the
geomagnetic field, and several magnetic coordinate systems have been developed to describe this organisation.
Here we provide a quasi-dipole geomagnetic coordinate calculator (Emmert et al, J. Geophys. Res., 2010) using
coefficients for all spherical harmonic degrees (up to 13) of the 14th Generation
International Geomagnetic Reference Field, and for comparison, a simple tilted dipole coordinate calculator using
only the degree 1 coefficients of IGRF-14. Locations which have similar geomagnetic latitudes are likely to experience
similar levels of magnetic disturbance. Local time and conductivity structures also influence magnetic disturbance
levels.
These data are delivered under the Open Government Licence, subject to the following acknowledgement accompanying the reproduced BGS materials:
"Geomagnetic coordinates are determined using model calculations provided by British Geological Survey - Geomagnetism"
If you require further information, wish to report a problem, or have suggestions as to how we can improve our service, please contact BGS Enquiries.
Coordinate Filters
Geodetic Coordinates:
Input as latitude/longitude/altitude, where altitude is km above WGS84 reference ellipsoid. Altitude must be greater than 0km.
If requesting a gridded output, the latitude/longitude step cannot be less than 0.01, and the latitude/longitude ranges must
greater than the input step sizes.
Specify latitude and longitude as one of:
Examples
Description
40°44'55"N
40:44:55S
73 59 11W
Degrees, minutes and seconds suffixed with 'N'/'S' (for latitude) or 'E'/'W' (for longitude)
to indicate the hemisphere:
Degree, minute, and second values can be separated either by the
standard symbols for angles (°, ' and ") or by colon characters (:) or by spaces.
Negative numbers may not be used.
Degree, minute and second values must all be integers - no decimal values are allowed
40.7486
-40.7486
-73.9864
Signed decimal degrees without compass direction ('N'/'S' or 'E'/'W'). Negative
values indicate south latitude or west longitude.
Temporal Filter
Date: must be between 1900-01-01 and 2029-12-31
Decimal year: can be greater or equal to 1900 and less than or equal to 2030.
As this is based on a web service you can also obtain results in JSON format using an HTTP GET request. Fetch data
here modifying the query string parameters as appropriate.
As this is based on a web service you can also obtain results in JSON format using an HTTP GET request. Fetch data
here modifying the query string parameters as appropriate.
Warning: One or more input values are invalid!
Caution:Dates beyond 2030 are not recommended! Inputs of 2035 onwards do not work.
Warning: Saved results cannot exceed 50. Please clear your saved outputs and try again.
Warning: Too many grid points requested. Try increasing latitude or longitude step size.
Learn More
The Earth's magnetic field is a vector quantity; at each point in space it has a strength and a direction. To completely describe it we need three quantities. These may be:
X, Y, and Z - three orthogonal strength components
F, D, and I - the total field strength and two angles
H, Z, and D - two strength components and an angle
The relationship between these 7 elements can be viewed at: INTERMAGNET
Secular variation (SV) is typically defined as the slow annual to decadal change of the Eath's magnetic field and is caused by the flow of liquid in the outer core,
deep inside the Earth. The change of the field is not easily predictable due to the nature of the flow regime in the core and the mechanism by which the magnetic field is generated.
However, an estimate of the instantaneous flow itself can be computed, if we make some assumptions about its nature and how it affects the magnetic field we observe at the surface.
If we have a longer series of data we can compute the accelerated flow too.