Post on 12-Jan-2016
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Making friends with IDL
IDL is an interpreted rather than a compiled language. This means that large IDL programs can execute less rapidly than equivalent compiled programs written in FORTRAN or C.
IDL LIMITATIONS:
IDL is a proprietary system (need licence)
interactive environment
excellent for visualizing, analyzing, editing, and displaying numerical data sets
immediate access to all variables
optimized array operations
versatile built-in plotting and graphics routines
data structures
possible interface with C and Fortran routines
on line help (?)
IDL = interactive data language
Making friends with IDL
create variables
> name = ‘Maxwell’ creates a string> z = 1.0e-8 creates a scalar> testdata = fltarr(512,512) creates a 512x512 2-D array with zero entries> a = [1,2,3] creates a vector> a = [a,4] expands a vector
Warning:
If you redefine a variables during your work, you lose the previous values
Avoid operation with different variables types. For example using float and integer these could be different > print, 3.456 * 1
> print, 3.456 * 1.
Variables
Variable names can have letters, numbers and underscores in them. They are NOT case-sensitive: aaa, Aaa and AAA are all the same variable.
IDL> a=[3, 5, 6, 2.5, 100, 27.7]
IDL> a= [[ 2,3,4],[10,20,30]]
IDL> a=float(b)IDL> a=fltarr(n_elements(b),4,2)
Array index START FROM 0!!!!
Array of 2 rows and 3 columns= Array[3,2]
One dimension array of 6 elements= Array[6]
Array manipulations
INVERT - Computes the inverse of a square array. MAX - Returns the value of the largest element of Array. MEDIAN - Returns the median value of Array or applies a median filter. MEAN – Return the mean value (also first element of MOMENT).MIN - Returns the value of the smallest element of an array. MOMENT – compute the first 4 moments (mean, variance…)REFORM - Changes array dimensions without changing the total number of elements. REVERSE- Reverses the order of one dimension of an array. SIZE- Returns array size and type information. TOTAL - Sums of the elements of an array. TRANSPOSE - Transposes an array. WHERE- Returns subscripts of nonzero array elements.
(a b c)## (g h) = (ag+bi+ck ah+bj+cl) (d e f) (i j) (dg+ei+fk dh+ej+fl) (k l)
(a b c)# (g h) = (ag+dh bg+ch cg+fh) (d e f) (i j) (ai+dj bi+ej ci+fj) (k l) (cg+fh ci+fj ck+fl)
> a = [1,2,3] > b = [4,5] > print, a#b > print, b#a > print, a##b> print,a*b
> print,a+1> print,b*2> print,a+b
Warning!!!
Try to avoid loopst=0for i=0,n_elements(a)-1 do t=t+a(i)
t=total(a)
looking for help
? name
help
help,variable : print variable informations.
help,A,/str : print structure info
help,/rou : prints list for all compiled procedures. Lists procedure and
functions separately.
help,/sy : prints current values of all "system variables", which are
special variables known to all routines. Names of these begin with a
"!", e.g. !dir, !path, etc.
help,/rec : prints contents of command recall buffer in reverse order
help,/dev : prints parameter settings for current graphics device
help,/mem : lists current memory usage
print,max(a); print,min(a); print,max(a); print,mean(a); print,variance(a); print,median(a); print,moment(a): print various statistical properties of image array. (moment prints first four moments.)
Open a help on line windows and search for ‘name’
Saving data (and time!)
save
restore
Safety idea: save your data!!!
Be prepared: 99% of time you will have to redo plots.Usual sequence:
1) Make plot2) Save data (and exit from idl)3) Meeting4) Restore data5) Redo plot
It will help also have your code saved in a routines.
> save,variable1,variable2,variable3,filename=‘~elisa/idl/data.sav’
Keyword: ALL => save all common block, system variable and local variable from the current IDL session.
> save,/all,filename=‘datatemp.sav’’
restore, filename=‘~elisa/idl/data.sav’
> restore,filename=‘datatmp.sav’
make a routine!
main routine
procedures or subroutines
functions
As you type, each line is interpreted and immediately executed
for (loop), if, case...
parameters and keywords
IDL routines (.pro)
One of the best ways to learn how to write and use IDL programs is to look the existing IDL programs
...end
pro NAME, VARIABLES...end
function NAME,VARIABLES...return,VALUEend
> .r filename
> name, variables
> a = name (variables)
NAME,input1,input2...output1,output2...keyword1=value1,$ keyword2=value2, /Keyword3.... optional and can be in any order
.pro file requirement How to call it
without .pro
OR
Program execution (and other)
all IDL procedures/functions are assumed to be in files with the explicit extension '.pro'.
compiles the IDL procedure(s) or function(s) in the file [name].pro. If this is a main program, also executes it.
IDL will locate the first file with this name in the IDL path or current directoryWARNING!!!!
stop > .c or .con
@file_name
; comment
Values of keywords are usually determined by assignment statements:
PROCEDURE_NAME,parm1,parm2.....KEYWORD1=100.,KEYWORD2='dumbo',...
in the case of switches, keywords can be set to a value of 1 by using the following syntax:
NAME,parm1,parm2...../KEYWORD1,.....
> retall
Run from IDL prompt
Inside a file.proCompile the file_name.pro Useful if the file mane is different from the procedure name
>.r or .run [name]
Don’t forget the comments!!! Comments begin with ‘;’
for debugging!! ... print... plot... to continue
if you wont to come back to the first level
Structures
A structure can be thought of as a user-defined data type or groups of different data IDL allows you to put lots of variables into a single ‘structure’
dsat={aod550:aot,$ ; mean AODstdaod550:sigma,$ ; standard deviationn:num,$ ; number of points latc:latitude,$ ; central lat of the boxeslonc:longitude} ; central longitude of the boxes
For example satellite data can be load as a structure containing:Instrument name, data and time, pixels radiances, coordinates and observing angles of the pixels
Define a structure:A structure (e.g. dsat) is an ensamble of other, previously defined, variables (and structures)
> help, dsat,/str AOD550 DOUBLE Array[720, 360] STDAOD550 DOUBLE Array[720, 360] N LONG Array[720, 360] LATC DOUBLE Array[360] LONC DOUBLE Array[720]
> print,dsat.aod550(good)
To access the variables of a structureUse: mone_str.nome_var
Routine that read satellite data usually load a structure for any image/orbit
keep related variables togetherpass/return a lot of variables with only one name
Basic plots
window,0,xsize=300,ysize=200x=findgen(10)
IDL> print,x 0.000 1.000 2.000 3.000 4.000 5.000 6.000 7.000 8.000 9.000
IDL> plot,sin(x2)
x2=2*!PI/100*findgen(100)
seed=1ln=32x=randomu(seed,n)y=randomu(seed,n)y2=randomu(seed,n)plot,x,y,psym=1,title='Random XY Points'oplot,x,y2,psym=2,colour=2
Others useful things
cut of data where
good = where (time eq 1000.,count) if (count eq 1 ) then begin...
If (count gt 1) then begin plot, x(good), y(good)
endif
and ; and ...or ; orgt ; greater than (similarly lt)ge ; gt or equal to (similarly le)eq ; equal tone ; not equal to
Logical operator
a = tvrd(true=3) write_jpeg, 'namefile.jpg',a,true=3
save a window like .jpg
print on postscript .ps file set_plot, 'ps' device, filename='filename.ps‘…close, /deviceset_plot, 'x'
Smaller file, good to make presentations and movies,NOT good for reports and papers !!!
‘comp_map_'+sat1+'_vsall.jpg’
plotting commands
png?
routines at AOPP
mappoints,data,lat,lon,centre=[0,0],/nogrey,nlevels=100
loadxy loadxyz
colour_ps
/home/crun/eodg/idl/
tvdata
ncol=4 nrow=4 !P.MULTI= [0,ncol,nrow,0,0]
mappoints,dayav.AOD550,lat,lon,centre=[0,0],/nogrey,$Nlevels=100,range=range,symsize=0.6,$title='AOD all daset average '+strcompress(i+1)+' March 2006'
avgrid,lat,lon,aod
imagepoints,data,lat,lon
fitexy,px,py,A,B,X_SIG=X_SIG,Y_SIG=Y_SIG
Linear fit when both x and y have errors (y = A + B x)
Plots data points, with defined latitudes and longitudes
Interpolate data (with the associated lat,lon) onto a regular lat lon grid, and plot the image
Using the same some fast regridding code (RAL)
Load txt file in columns
Set colour bar
+ several routine to load different type of data
ASK!!!