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Table 1. Summary of data selection criteria. Here, am and Dst are magnetic indices, IMF-By and IMF-Bz are the vector components of the interplanetary magnetic field in Geocentric Solar Magnetospheric (GSM) coordinates at the bow shock (http://omniweb.gsfc.nasa.gov/hw.html) and Em is the merging electric field (Kan and Lee, 1979). By mid latitudes we mean track segments covering −60° to 60° geomagnetic latitude and high latitudes refers to overlapping tracks at < −50° and >50° geomagnetic latitude.

From: NOAA/NGDC candidate models for the 11th generation International Geomagnetic Reference Field and the concurrent release of the 6th generation Pomme magnetic model

 

Mid latitudes

High latitudes

Max Dst

±30 nT

±30 nT

Max Dst derivative

±2 nT/h

±5 nT/h

Max am

12

27

Max am 3 hours before

15

27

Max IMF-B y

 

±8 nT

Min IMF-B z

 

−2 nT

Max IMF-B z

 

6 nT

Max Em

 

0.8 mV/m

CHAMP only:

Max diamagnetic effect

5 nT

 

Max jump in diam. eff.

2 nT