Changes between Version 47 and Version 48 of CollidingFlows

Timestamp:

10/15/12 09:30:44 (12 years ago)

Author:

Jonathan

Comment:

—

CollidingFlows

@@ -101 +101 @@
 
 === Spectra ===
+
+First looked at 1D models of colliding flows.  The initial velocity field is essentially a heaviside function - and the window used is a cosine window.  While these results are for 1D models - the initial flow is 3D although there could be subtleties associated with the windowing in the y and z direction - though probably not at small wave numbers.
+
+[[Image(PowerSpectraSamples.png, width=400)]]
+
+----
+
 Kinetic Energy Spectra [attachment:Kinetic.gif gif] and [attachment:Kinetic.AVI avi]
 || 0 Myr ||  [[Image(Kinetic0000.bmp, width=400)]]  ||
@@ -107 +114 @@
 || 27 Myr || [[Image(Kinetic0245.bmp, width=400)]]  ||
 
-
-
+Mass and Grav Energy Spectra [attachment:MassGrav.gif gif] and [attachment:MassGrav.AVI avi]
+|| 0 Myr ||  [[Image(MassGrav0000.bmp, width=400)]]  ||
+|| 10 Myr || [[Image(MassGrav0083.bmp, width=400)]]  ||
+|| 20 Myr || [[Image(MassGrav0166.bmp, width=400)]]  ||
+|| 27 Myr || [[Image(MassGrav0245.bmp, width=400)]]  ||
+
+Velocity Spectra [attachment:Spectra.gif gif] and [attachment:Spectra.AVI avi]
+|| 0 Myr ||  [[Image(Spectra0000.bmp, width=400)]]  ||
+|| 10 Myr || [[Image(Spectra0083.bmp, width=400)]]  ||
+|| 20 Myr || [[Image(Spectra0166.bmp, width=400)]]  ||
+|| 27 Myr || [[Image(Spectra0245.bmp, width=400)]]  ||
 
 [[CollapsibleStart(Previous runs)]]