“…γ is the ratio of specific heats, P is the plasma pressure within the flux tube, and V = (1/B)ds is the volume of the flux tube containing 1 Wb of magnetic flux, where s is the length of the flux tube. They reflect the properties of reconnection regions they originate from and thus are of key importance for our understanding of magnetospheric substorm dynamics, and this is the reason why there is a plethora of studies investigating these plasma structures both theoretically/numerically (Sitnov and Swisdak, 2011;Nakamura et al, 2002;Birn et al, 2011;Sitnov et al, 2009;Guzdar et al, 2010) and observationally (Nakamura et al, 2001(Nakamura et al, , 2002Runov et al, 2009;Sergeev et al, 2009;Slavin et al, 2003a, b), just to mention but a few.…”