Cranmer and Chandran (2010), SHINE meeting poster

The accompanying tabulated data file presents the information used
in the plots in the section of the poster titled "Are the MHD
fluctuations undergoing turbulent cascade and dissipation?"

Column formats:

(1) heliocentric radius, in solar radii (goes from 5 Rsun to 4 AU)

(2) mass density, in g/cm^3

(3) empirical fit to the heating rate, in erg/s/cm^3

(4) Undamped (WKB) outward (Z_{+}) Elsasser amplitude, in cm/s,
extrapolated both downwards and upwards from a specified value at 0.4 AU.

(5) Damped (non-WKB) outward (Z_{+}) Elsasser amplitude, in cm/s,
extrapolated downwards from a specified value at 0.4 AU.

See poster text for additional details and plots.