; SHOW.PRO
;
; Originally written to show images from Polar Camera initial field test
; at Ryning Farm Observatory
; Modified 1993/1/29 by DPS to handle images from image tree structure
; on /jasper/cnsr3_data1
;
; create byte-valued input parameters
cam=0B & filt=cam & day=cam & month=cam
mask=BYTARR(256,256)
; load various string-valued arrays needed
initialize,filters,months,days,modes,mpaths,firstchars
s=''
!ORDER=1
; set colour table 
PRINT,'Do you want a colour display? ([Y]/N)'
resp=''
READ,resp
IF STRUPCASE(resp) EQ 'N' THEN loadct,0,/silent ELSE loadct,13,/silent

; tell user what imaging modes and filters are available    
PRINT,"Num   Mode          Cam0 Filters            Cam1 Filters" 
FOR i=0,5 DO modes(i)=STRTRIM(modes(i),2)+spc(14-STRLEN(modes(i))) 
col1=modes & maxlen1=MAX(STRLEN(col1))
wavelengths=STRARR(5) 
FOR i=0,4 DO BEGIN    
    wv=STRTRIM(filters(i),2) 
    tmp=STRMID(wv,0,STRPOS(wv,'nm')+2)
    wavelengths(i)=tmp+spc(24-STRLEN(tmp)) 
ENDFOR    
col2=wavelengths & maxlen2=MAX(STRLEN(col2)) 
FOR i=0,4 DO BEGIN 
    wv=STRTRIM(filters(i+5),2) 
    tmp=STRMID(wv,0,STRPOS(wv,'nm')+2)
    wavelengths(i)=tmp+spc(24-STRLEN(tmp)) 
ENDFOR    
col3=wavelengths & maxlen3=MAX(STRLEN(col3)) 
STOP
FOR i=0,4 DO BEGIN 
    line=STRING(i,col1(i),col2(i),col3(i),FORMAT='(I1,5X,A14,2A24)') 
    PRINT,line 
    ENDFOR 
PRINT,STRING(5,col1(5),FORMAT='(I1,5X,A14)') 

; prompt user and get input
PRINT,'Enter the mode, camera, filter, day, month, and year desired'
READ,mode,cam,filt,day,month,year
IF mode EQ 0 THEN BEGIN		; auroral mode. variable exposure time
; prompt user for exposure time desired (0 => all exposure times OK)
    PRINT,'Enter the exposure time (s) for the images you want to view,'
    PRINT,'(or 0 for all available images)'
    READ,texp
ENDIF ELSE texp=0
; create 3-character string giving desired exposure time (or all)
IF texp EQ 0 THEN exp='???' ELSE exp=STRING(texp,FORMAT='(I3.3)')
; ensure a 4-digit year for display; make reasonable assumptions
IF year LT 1900 THEN BEGIN
    IF year LT 50 THEN year=year+2000
    IF year GT 50 THEN year=year+1900
ENDIF

; create title for image plot
wtitle=STRING(modes(mode),filters(cam*5+filt),year,months(month-1), $
	      day,FORMAT='("Polar Camera",2X,A,2X,A,2X,I4,1X,A3,1X,I0.2)')
; define mask for images, with fixed horizon at 150 superpixels 
prad=150
d256=SHIFT(dist(256),128,128) & base=WHERE(d256 GT 150)
wprad=WHERE(d256 LE prad) & mask(wprad)=1
; define path to desired images
IF (mode EQ 1) OR (mode EQ 3) $
    THEN dir=STRING(mpaths(mode),cam,FORMAT='(A,"/c",I1,"/")') $
    ELSE dir=STRING(mpaths(mode),cam,filt,FORMAT='(A,"/c",I1,"/f",I1,"/")')
; make list of available files of desired type
template=firstchars(mode)+STRING(day,cam,filt,FORMAT='(I2.2,I1,I1)') $
         +exp+'.*'
files=FINDFILE(dir+template,COUNT=nfiles)
IF nfiles LE 0 THEN BEGIN
    PRINT,'No files found; quitting.'
    GOTO,DONE
    ENDIF
; sort contents of 'files' in time order
timesort,files,day,month,year,nfiles,jsecs
; define path to corresponding dark frames, if required
IF (mode NE 1) AND (mode NE 3) THEN BEGIN
; only open-shutter images require dark subtraction
    ddir=STRING(mpaths(3),cam,FORMAT='(A,"/c",I1,"/")')
    dtemplate=STRING(day,cam,FORMAT='("d",I2.2,I1,"?")')+exp+'.*'
    dfiles=FINDFILE(ddir+dtemplate,COUNT=ndfiles)
    IF ndfiles GT 0 THEN BEGIN
        timesort,dfiles,day,month,year,ndfiles
        PRINT,STRING(ndfiles,FORMAT='(I3," dark frame files found")')
    ENDIF ELSE PRINT,"No dark frame files found"
ENDIF

; identify image sequences and prompt user for sequence(s) to display
djs=ABS(jsecs-SHIFT(jsecs,1))	; rectify big negative number in front
seqstart=WHERE(djs GT 600)	; semi-arbitrary large number (10 min)
ext_list=extension(files)

PRINT,'There are '+STRTRIM(nfiles,2)+' images, with extensions '+ $
      ext_list(0)+' to '+ext_list(nfiles-1)+'.'
IF seqstart(0) GE 0 THEN BEGIN
    PRINT,'Sequences begin with the following image file numbers(s):'
    PRINT,extension(files(seqstart))
ENDIF
PRINT,'Enter the range of image file numbers to display (* for all images)'
instring='' & READ,instring

f=isnumber(instring,inf)
IF f NE 0 THEN BEGIN		; user entered at least one number
    inf=FIX(inf)
    IF f GT 0 $			; user entered only one number
	THEN inl=nfiles-1 $
        ELSE BEGIN
	    f=isnumber(getwrd(instring,1),inl)
	    IF f NE 0 THEN inl=FIX(inl) ELSE inl=nfiles-1
        ENDELSE
ENDIF ELSE BEGIN
    inf=0
    inl=nfiles-1
ENDELSE

;IF STRPOS(instring,'*') EQ -1 THEN BEGIN	; user entered numbers
;    instring=STRTRIM(instring,2)	; remove leading/trailing blanks
;    blank=STRPOS(instring,' ')	; space between two numbers
;    inf=FIX(STRMID(instring,0,blank))
;    inl=FIX(STRMID(instring,blank,STRLEN(instring)-blank))
;    inf=WHERE(inf EQ FIX(ext_list))
;    inl=WHERE(inl EQ FIX(ext_list))
;ENDIF ELSE BEGIN
;    inf=0 & inl=nfiles-1
;ENDELSE

; Prompt user for fixed saturation brightness
PRINT,'If you want to assign the top of the color bar to a fixed number of counts,'
PRINT,'enter that number now, otherwise enter anything else for auto-scaling.'
tops=''
READ,tops
flag=isnumber(tops,topnum)	; topnum=0 if tops doesn't represent a number

; If camera 0 images from RFO selected, load the image to try removing
; the in-camera contamination
; IF cam EQ 0 THEN BEGIN
;     minname=STRING(day,cam,filt,FORMAT='("a",I2,I1,I1,"060.min")')
;     rdkimg,dir+minname,h,minim
; ENDIF

; create and label image display window
X_charheight=10		; try to keep scalings that apply in X windows
X_charwidth=8
barwidth=16
ninrow=4
nincol=3
ninwin=ninrow*nincol
wwidth=ninrow*256+barwidth
wheight=nincol*256+4*X_charheight
IF !D.NAME EQ 'X' THEN $
    WINDOW,0,XSIZE=wwidth,YSIZE=wheight $
    ELSE DEVICE,/COLOR,BITS_PER_PIXEL=8	; PostScript
csz=((1.*X_charheight)/wheight)/((1.*!D.Y_CH_SIZE)/!D.Y_VSIZE)	; keep 'X' char size
XYOUTS,scl(res=120.,(wwidth-barwidth)/2) $
      ,scl(res=120.,wheight-3*X_charheight),wtitle $
      ,/DEVICE,ALIGNMENT=0.5,CHARSIZE=2.0*csz,WIDTH=twidthn
twidthd=CONVERT_COORD([twidthn,0.],/NORMAL,/TO_DEVICE)
twidthd=twidthd(0)			; we only need the x-component
; get user's name and display it
SPAWN,'whoami',username
XYOUTS,scl(res=120.,wwidth-X_charwidth),scl(res=120.,wheight-3.9*X_charheight) $
      ,'User '+STRUPCASE(username),ALIGNMENT=1.0,/DEVICE,CHARSIZE=csz
; get date/time and display them
SPAWN,'date -u',datetime
XYOUTS,scl(res=120.,wwidth-X_charwidth),scl(res=120.,wheight-2.5*X_charheight) $
      ,STRMID(datetime,11,9)+' UT',ALIGNMENT=1.0,/DEVICE,CHARSIZE=csz
XYOUTS,scl(res=120.,wwidth-X_charwidth),scl(res=120.,wheight-1.1*X_charheight) $
      ,STRMID(datetime,4,7)+STRMID(datetime,24,4),ALIGNMENT=1.0,/DEVICE,CHARSIZE=csz
; create and display color bar
bar=REBIN(BINDGEN(256,barwidth),nincol*256,barwidth)
bar=ROTATE(bar,3)
mtv,bar,ninrow*256,0,res=120.

; read in each image, decode the header, subtract dark frame, rebin to 
; 256x256 if necessary, scale to 8 bits and display
ip=-1
mid=-1
FOR i=inf(0),inl(0) DO BEGIN
    rdkimg,files(i),h,im
    KIh=gethd(h)
; if image isn't 256x256, rebin it
    im=REBIN(im,256,256)
; ensure counts are actually summed if a 512x512 image is compressed
    cfac=512/(256*KIh.exp.sbin)
    rfac=512/(256*KIh.exp.pbin)
    im=im*cfac*rfac
; extract start time of image from header
    itime=BYTARR(4)
    FOR itptr=0,3 DO itime(itptr)=KIh.misc.tm.(itptr)
    utsecs=TOTAL(itime*[3600,60,1,.01])

    IF NOT ((mode EQ 1) OR (mode EQ 3)) THEN BEGIN
        IF (ndfiles GT 0) AND $	; dark frames exist, for this exposure time
           (TOTAL(exposure(dfiles) EQ exposure(files(i))) GT 0) THEN BEGIN
; find closest dark frame
; (NB: this isn't going to work over day boundaries!)
            id=MAX([mid-1,-1])
            mid=-1
            mindif=90000.
            thisdif=86400.
            REPEAT BEGIN
                id=id+1
                IF (exposure(dfiles(id)) EQ exposure(files(i))) THEN BEGIN
                    rdkihd,dfiles(id),dh	; read id'th file header
                    dKIh=gethd(dh)
                    dtime=BYTARR(4)
                    FOR itptr=0,3 DO dtime(itptr)=dKIh.misc.tm.(itptr)
                    dutsecs=TOTAL(dtime*[3600,60,1,.01])
                    thisdif=ABS(dutsecs-utsecs)
                    IF thisdif LT mindif THEN BEGIN
                        mindif=thisdif	; update minimum time difference
                        mid=id		; and id no. of closest frame
                    ENDIF
                ENDIF
            ENDREP UNTIL (mindif LT thisdif) OR (id EQ ndfiles-1)

; Dark frames not taken at some exposure times; warn user and go on

            IF mid NE -1 THEN BEGIN
                rdkimg,dfiles(mid),dh,dkimg	; read dark frame closest in time
                im=(im-dkimg)>0		; subtract dark frame
            ENDIF ELSE BEGIN
	        IF NOT KEYWORD_SET(meandk) THEN BEGIN
                    fexp=FIX(STRMID(files(i),STRLEN(files(i))-7,3))
                    rdmeandk,cam,fexp,meandk
                ENDIF
                im=(im-meandk)>0
            ENDELSE
        ENDIF ELSE BEGIN
	    IF NOT KEYWORD_SET(meandk) THEN BEGIN
                fexp=FIX(STRMID(files(i),STRLEN(files(i))-7,3))
                rdmeandk,cam,fexp,meandk
            ENDIF
            im=(im-meandk)>0
        ENDELSE
    ENDIF
; If camera 0, subtract contamination image
;    IF cam EQ 0 THEN im=(im-minim)>0

; If autoscaling is desired, find lmaxi, otherwise use topnum
    IF topnum EQ 0 THEN BEGIN
; Is there any useful information left in the image?
; identify useful min and max values for byte-scaling
        ih=HISTOGRAM(im(wprad),MIN=0,BIN=1)	; histogram of exposed image
        cih=ih	; next line computes cumulative pixel value pdf
        FOR jj=1,N_ELEMENTS(cih)-1 DO cih(jj)=cih(jj)+cih(jj-1)
        cih=cih/FLOAT(MAX(cih))		; normalize to unity
        lmaxi=MAX(WHERE(cih LE .999))	; top 0.1% of pixels saturate
    ENDIF ELSE lmaxi=topnum
; if viewing filter images, take dark 'skirt' as min value
    IF filt LE 4 THEN BEGIN
	IF MAX(im(base) GT 0) THEN BEGIN
            bh=HISTOGRAM(im(base),MIN=0,BIN=1)
            maxbh=MAX(bh,lmaxbh)	; bottom = most prob. skirt value
	ENDIF ELSE lmaxbh=0
    ENDIF ELSE BEGIN
; otherwise take lowest level in dark frame
        lmini=MIN(WHERE(cih GE .001))
        lmaxbh=lmini	; rename this parameter for compatibility below
    ENDELSE

    ip=ip+1		; index number for screen position of image
; show image orientation, one time only
    IF ip EQ 0 THEN BEGIN
        nflag=isnumber(KIh.misc.az,azimuth)
        IF nflag NE 0 THEN BEGIN 	; if the camera azimuth is known,
            azrad=!DTOR*azimuth		; plot arrows showing the azimuth
            leftend=scl(res=120.,wwidth/2.)-twidthd/2.
            maxlen=(leftend-scl(res=120.,1.5*X_charwidth)) $
                   /scl(res=120.,(COS(azrad)+SIN(azrad))*X_charheight)
            arlen=MIN([FIX(maxlen),4])*X_charheight
            tailx=REPLICATE(scl(res=120.,0.5*X_charwidth+SIN(azrad)*arlen),2)
            taily=REPLICATE(scl(res=120.,nincol*256),2)
            headx=[tailx(0)-scl(res=120.,arlen*SIN(azrad)), $
                   tailx(1)+scl(res=120.,arlen*COS(azrad))]
            heady=[scl(res=120.,nincol*256+arlen*COS(azrad)), $
                   scl(res=120.,nincol*256+arlen*SIN(azrad))]
            arrow,tailx,taily,headx,heady,/device,hsize=-0.2
            XYOUTS,headx(0)+scl(res=120.,X_charwidth) $
                  ,MIN([heady(0),scl(res=120.,wheight-X_charheight)]) $
                  ,'N',ALIGNMENT=0,/DEVICE,CHARSIZE=csz
            XYOUTS,headx(1)+scl(res=120.,X_charwidth),heady(1),'E' $
                  ,ALIGNMENT=0.5,/DEVICE,CHARSIZE=csz
        ENDIF ELSE BEGIN		; otherwise show cardinal directions
            XYOUTS,scl(3*X_charwidth,res=120.) $
                  ,scl(nincol*256+3*X_charheight,res=120.) $
                  ,'N',/DEVICE,ALIGNMENT=0.5,CHARSIZE=csz
            XYOUTS,scl(res=120.,X_charwidth) $
                  ,scl(res=120.,nincol*256+1.5*X_charheight),'W' $
                  ,/DEVICE,ALIGNMENT=0.5,CHARSIZE=csz
            XYOUTS,scl(res=120.,5*X_charwidth) $
                  ,scl(res=120.,nincol*256+1.5*X_charheight),'E' $
                  ,/DEVICE,ALIGNMENT=0.5,CHARSIZE=csz
            XYOUTS,scl(res=120.,3*X_charwidth) $
                  ,scl(res=120.,nincol*256),'S',/DEVICE $
                  ,ALIGNMENT=0.5,CHARSIZE=csz
        ENDELSE
    ENDIF
; display the image
    mtv,ROTATE(im*mask,5),low=lmaxbh,high=lmaxi,res=120. $
       ,(ip MOD ninrow)*256,(nincol-1-(ip MOD ninwin)/ninrow)*256
;   mtv,im*mask,low=lmaxbh,high=lmaxi,res=120. $
;      ,(ip MOD ninrow)*256,(nincol-1-(ip MOD ninwin)/ninrow)*256
; display image sequence number
    XYOUTS,scl(res=120.,(ip MOD ninrow)*256+1) $
          ,scl(res=120.,(nincol-(ip MOD ninwin)/ninrow)*256-1-X_charheight) $
          ,ext_list(i),/DEVICE,ALIGNMENT=0.0,CHARSIZE=csz,COLOR=0.8*!D.N_COLORS
; and image time
    XYOUTS,scl(res=120.,(ip MOD ninrow)*256+1) $
          ,scl(res=120.,(nincol-1-(ip MOD ninwin)/ninrow)*256+3+X_charheight) $
          ,/DEVICE,ALIGNMENT=0.0,CHARSIZE=csz,COLOR=0.8*!D.N_COLORS $
          ,STRING(itime(0:2),FORMAT='(I2.2,":",I2.2,":",I2.2)')
; and exposure time
    XYOUTS,scl(res=120.,(ip MOD ninrow)*256+1) $
          ,scl(res=120.,(nincol-1-(ip MOD ninwin)/ninrow)*256+1) $
          ,STRING(KIh.misc.exp_scale*KIh.exp.exposure/1000. $
          ,FORMAT='(F5.1,1X,"s")'),/DEVICE,ALIGNMENT=0.0,CHARSIZE=csz $
          ,COLOR=0.8*!D.N_COLORS
; and maximum displayed DN
    XYOUTS,scl(res=120.,((ip MOD ninrow)+1)*256-1) $
          ,scl(res=120.,(nincol-(ip MOD ninwin)/ninrow)*256-1-X_charheight) $
          ,STRING(FIX(lmaxi),FORMAT='("< ",I0.0," DN")') $
          ,/DEVICE,ALIGNMENT=1.0,CHARSIZE=csz,COLOR=0.8*!D.N_COLORS
; and minimum displayed DN
    XYOUTS,scl(res=120.,((ip MOD ninrow)+1)*256-1) $
          ,scl(res=120.,(nincol-1-(ip MOD ninwin)/ninrow)*256+1) $
          ,STRING(FIX(lmaxbh),FORMAT='("> ",I0.0," DN")'),/DEVICE $
          ,ALIGNMENT=1.0,CHARSIZE=csz,COLOR=0.8*!D.N_COLORS
    PRINT,'.',FORMAT='(A,$)'
    IF (ip+1) MOD ninwin EQ 0 THEN PRINT,'|',FORMAT='(A,$)'
    IF GET_KBRD(1) EQ 'q' THEN GOTO,DONE
ENDFOR
DONE:
PRINT,''
END