URI: 	http://hdl.handle.net/10201/123584
Title:	The Low-Altitude Ionosphere of the Ice Giant Planets
Author:	G. J. Molina-Cuberos,  O. Witasse, D. Toledo} and  S.N. Tripathi
Journal: Journal Geophysical Research-Planets, submitted 2022


The repository include the data presented in the above paper (see folders) and the matlab file to 
produce the figure (CalculosPaper.m). 

Folders "aerosoles" and "results" 
Include charge and conductivity profiles for several conditions such us planet 
(Uranus or Neptune), aerosol profile (standard, minimum, maximum), geomagnetic latitude, 
solar heliocentric potential (300, medium, 800) and mean mass of the most abundant 
ion (33, 100). 
For example: 
	Neptune_mIon_33_MV300vc0_Stan.dat=> Planet Neptune, mass of the ion 33, 
	solar modulation 300, vcutoff parameter (to model magnetic field) 0 and Standard model 
	for aerosols
	Uranus_mIon_33_MV800vc46_Stan.dat=> Planet Uranus, mass of the ion 33, solar modulation 800, 
	vcutoff parameter (to model magnetic field) 46 and Standard model for aerosols

Folder "gcr"  
Includes the ionization rate profiles (crpr*.dat) and proton spectra at 
minimum atmospheric depth available by the model.
For examaple:
	crpr_ur_MV500vc46.dat=> planet Uranus, solar modulation parameter 500, vcutoff parameter
	(to model magnetic field) 46
	ProtonFux_SeveralMV => proton fux  at .450 G/CM^2 very low to simulate interplanetary medium
	for severa solar conditions

CalculosPaper.m 
matlab R2020a file to plot the figures of the paper. It is divided in 
sections by using %% Fig (or similar) to make each plot. The sections run independently and
read the input data from the above folders. 


Any commet to: gregomc@um.es