AMPS: Average Magnetic field and Polar current System

The AMPS model is an empirical model based on magnetic field measurements in low Earth orbit from the CHAMP and Swarm satellites.

Click here to open WebAMPS
 

 

Real-time Data

Below is a presentation of dynamic solar data gathered from various commonly-used sources.

KHO Auroral Forecast: (Left) the size and location of the impact zone of energetic particles from the Sun, (right) local all-sky view of the oval (Courtesy: Kjell Henriksen Observatory, UNIS, Norway)

Kp index: System for measuring auroral strength (Courtesy: SWPC NOAA)

Photosphere: The visible surface of the Sun (Courtesy: SWPC NOAA)

Chromosphere: The second of the three main layers of the Sun (Courtesy: SWPC NOAA)

Corona: The outermost layer of the sun (Courtesy: SWPC NOAA)



GOES X-ray plot: tracks solar activity and flares (Courtesy: SWPC NOAA)


Stackplot

Tromsø magnetometer stackplot: Readings from a network of magnetometer ground stations (Courtesy: Tromsø Geophysical Observatory, Univ. of Tromsø, Norway)