The location of the Earth's magnetopause: A comparison of modeled position and in situ Cluster data

Exploiting 8years of magnetic field data from the Cluster mission, we employ an automated magnetopause crossing detection routine to determine the magnetopause location over varying magnetic latitudes and local times. For a period spanning nearly one solar cycle we build a database of 2709 magnetopause crossings and compare these locations to the magnetopause models of Petrinec and Russell (1996), Shue et al. (1998), Dmitriev and Suvorova (2000), and Lin et al. (2010). We compare our detected locations with the predicted locations for a variety of solar wind conditions and positions on the magnetopause. We find that, on average, the Petrinec and Russell (1996) and Shue et al. (1998) models overestimate the radial distance to the magnetopause by ∼1 R E (9%), while the Dmitriev and Suvorova (2000) and Lin et al. (2010) models underestimate it by 0.5 R E (4.5%) and 0.25 R E (2.3%), respectively. Some varying degree of control on the differences between the predicted and encountered locations, by the solar wind and location parameters, are found.