;called from ~\lightning\idl\iss\scattered_light\main_scattered_light.pro



r_saturn_thous_km=60.
rho_albedo_phase_index_ring_versus_r_sat= $
 [[75. ,92.,93.,94.,98.,100,103,105,116,117.,122.,122.5,125,133,133.1,133.7,137,137.1], $;,200], $
  [0.05,0.2,1.6,0.8,0.9,1.5,1.0,1.7,1.3,0.15,0.3 ,1.   ,0.5,0.4,0.1  ,0.5  ,0.5,0.001], $;,0.001], $
  [0.4 ,0.4,0.4,0.4,0.4,0.4,0.4,0.4,0.4,0.4 ,0.4 ,0.5  ,.48,.46,0.46 ,0.46 ,0.5,0.5  ], $;,0.46], $
  [3.1 ,3.1,3.1,3.1,3.1,3.1,3.1,3.1,3.1,3.1 ,3.1 ,3.1  ,3.1,2.7,2.7  ,2.7  ,2.6,2.6  ]] ;,2.6]]


;; 4 lines below for test purposes only
;[[75.,140], $
; [0.5,0.5], $
; [0.01,0.01], $
; ;[1.,1], $
; [3.092,3.092]]

;High-res data from Henry (Luke Dones' results) will be composed by running the following batch file

@~\lightning\idl\iss\scattered_light\ins\compose_hi_res_rho_albedo_phase_index_ring_versus_r_sat.pro
get_ring_phase_lookup_table_spline,ring_phase_lookup_table $
		,label_lookup,tau_lookup,albedo_lookup,solar_elev_lookup,obs_elev_lookup,obs_azim_lookup

rho_albedo_phase_index_ring_versus_r_sat(*,0)=rho_albedo_phase_index_ring_versus_r_sat(*,0)/r_saturn_thous_km

;last row-phase index ~3.3  ;formula P(s) = 0.13 s**power_ph_fun from Luce Dones
					;where s = pi - the phase angle in radians