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Table 1

Thermosphere and upper atmosphere models used in the assessment.

Type Drivers (solar | geomagnetic) Hor. & time resolution
NRLMSISE-00 SE F10.7 | ap (array of 7 values) 30°, 3 h
JB2008 SE S10, F10.7, M10, Y10 | Dst, ap 30°, 1 h
DTM2013 SE F30 | Kp 30 × 15°, 3 h
TIE-GCM FP Solomon & Qian bands | Heelis-Kp 5.0 × 5.0°, 1 min
Solomon & Qian bands | Weimer
CTIPe FP F10.7, F81, Solomon & Qian bands Weimer-2005, solar wind density and velocity, interplanetary magnetic field, Hemispheric Power, Kp 2.0 × 18°, 1 min

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