Anomalously low solar extreme‐ultraviolet irradiance and thermospheric density during solar minimum

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Causes of low thermospheric density during the 2007–2009 solar minimum (2011, methodology): “[6] Recent work [Solomon et al., 2010] attempted to explain the thermospheric density changes between 1996 and 2008 using EUV measurements [Didkovsky et al., 2010] to estimate synthetic solar spectral input to the NCAR Thermosphere‐Ionosphere‐Electrodynamics General Circulation Model (TIE‐GCM).”
Does the F10.7 index correctly describe solar EUV flux during the deep solar minimum of 2007-2009? (2011, background): “[2010] reported that thermospheric density is significantly lower in the recent Smin than in previous ones, and Solomon et al. [2010] thought this is mainly induced by the lower EUV irradiance in the recent Smin.”
Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “Clear connections can be found between high-speed solar wind streams and modulations of the aurora and geomagnetic indices, radiation belts, ionosphere, and thermosphere (Gibson et al. 2009; Solomon et al. 2010; Lei et al. 2011).”
The DTM-2013 thermosphere model (2015, background): “7 proxy during the last solar minimum, and consequently models overestimate density (Solomon et al. 2010, 2011).”