Images were customized with respect to the luminosity of each observer.
Figure 3 shows a typical shock luminosity signal recorded using a polyethylene target, along with the fiducial signal.
We call this property the luminosity of the flow.
The shock luminosity signals recorded in the two targets clearly show the relative shock transit time delay.
Solar luminosity is given in column 4 relative to the present output.
The differences in luminosity are taken to be the result of different accretion rates within the disks.
The model is based on the global carbon cycle mediated by life and driven by increasing stellar luminosity and plate tectonics.
The luminosity evolution of the main-sequence central star is deduced by polynomial fitting of stellar evolution models.
