Image Details
 
                    Caption: Figure 5.
Maximum density enhancement with respect to the RTV density, 
   n
      p
   /
   n
   RTV as a function of the ratio of loop half-length to heating scale height, 
   L/
   s
      H
   , for a set of eight hydrodynamic numerical simulations performed by Tsiklauri et al. (2004), for 
   s
      H
    = 8.75 Mm and loop half-lengths of 
   L = 9, ..., 55 Mm (diamonds). The scaling law of Serio et al. (1981) yields consistent predictions for 
   L/
   s
      H
    
    3, but overpredicts the density enhancements for higher values of 
   L/
   s
      H
 3, but overpredicts the density enhancements for higher values of 
   L/
   s
      H
    
    3 where no stationary loop solutions exist due to the Rayleigh–Taylor instability. Numerical hydrodynamic simulations yield
   maximum density enhancements of 
   n
      p
   /
   n
   RTV ≲ 2 for stationary solutions (Winebarger et al. 2003a, 2003b). For dynamic simulations of impulsive heating and subsequent
   cooling maximum (Tsiklauri et al. 2004), maximum density enhancements of 
   n
   max/
   n
   RTV ≈ 0.5(1 + 
   L/
   s
      H
   ) are obtained.
 3 where no stationary loop solutions exist due to the Rayleigh–Taylor instability. Numerical hydrodynamic simulations yield
   maximum density enhancements of 
   n
      p
   /
   n
   RTV ≲ 2 for stationary solutions (Winebarger et al. 2003a, 2003b). For dynamic simulations of impulsive heating and subsequent
   cooling maximum (Tsiklauri et al. 2004), maximum density enhancements of 
   n
   max/
   n
   RTV ≈ 0.5(1 + 
   L/
   s
      H
   ) are obtained.
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