This page was created by IDL
lasco_mk_html_help.pro on
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NAME:
ALIGN1.PRO
PURPOSE:
Takes two images of EO frange, corrects it from the dark and
sums both, loading the result into X_display
CATEGORY:
??
CALLING SEQUENCE:
ALIGN1, nom_image1,nom_image2,nom_dark,imas,itest
INPUTS:
nom_image1 one of frange images
nom_image2 frange image in oposite side
nom_dark dark image name
itest 'V' or 'H' horizontal or vert alignement
KEYWORD PARAMETERS:
None
OUTPUTS:
imas resulting composite image
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by A.LL v.1.0 LAS 08/25/93
NAME: dvpt_fra.pro
PURPOSE: make a polar development of OE fringe or
of OI blocked fringe
CATEGORY: Processing high level
CALLING SEQUENCE: dvpt_fra,ima_in,Xc,Yc,R,delta_R,ima_out
INPUTS: ima_in reference's image
OPTIONAL INPUT PARAMETERS: Xc,Yc fringe's center
R internal radius
delta_R width of fringe
KEYWORD PARAMETERS: None
OUTPUTS: ima_out result frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: Applications limited to 512*512 frames
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 09/24/93
modified by M.B 02/17/94 : LAS
SCCS variables for IDL use
@(#)dvpt_fra.pro 1.0 09//93 :LAS
NAME: ipolarfra.pro
PURPOSE: make the inverse of polar transformation
for OE developped fringe or for OI blocked
developped fringe
CATEGORY: Processing high level
CALLING SEQUENCE: ipolarfra,ima_in,Xc,Yc,R,delta_R,ima_out
INPUTS: ima_in reference's image
OPTIONAL INPUT PARAMETERS: Xc,Yc fringe's center
R internal radius
delta_R width of fringe
KEYWORD PARAMETERS: None
OUTPUTS: ima_out result frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: Applications limited to 512*512 frames
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 02/17/94 : LAS
SCCS variables for IDL use
@(#)ipolarfra.pro 1.0 02/17/94 : LAS
NAME: gener_mask.pro
PURPOSE: make a circular mask for photometry's studies
CATEGORY: Processing high level
CALLING SEQUENCE: gener_mask,ima_name,npix,Xc,Yc,R,intval,extval
INPUTS: ima_name Name of mask
npix dimension
OPTIONAL INPUT PARAMETERS: Xc,Yc circle's coords
R radius of mask
intval value inside
extval value outside
KEYWORD PARAMETERS: None
OUTPUTS: ima_name mask's frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 09/10/93
modified by M.B 02/17/94 : LAS
SCCS variables for IDL use
@(#)gener_mask.pro 1.0 09/10/93 :LAS
NAME: diafrai.pro
PURPOSE: apply a circular mask for photometry's studies
to a selected frame
(define a circular ROI or apply a diaphragm)
CATEGORY: Processing high level
CALLING SEQUENCE: diafrai,ima_name,Xc,Yc,R,intval,extval
INPUTS: ima_name Name of image
OPTIONAL INPUT PARAMETERS: Xc,Yc circle's coords
R radius of mask
intval value inside to be multiplied
extval value outside to be multiplied
KEYWORD PARAMETERS: None
OUTPUTS: ima_name image with mask
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 02/17/94 : LAS
SCCS variables for IDL use
@(#)diafrai.pro 1.0 02/17/94 :LAS
ro build_fraoe, image1, image2, image3, image4, oefringe
+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
NAME:
BUILD_FRAOE
PURPOSE:
Takes four images of EO fringe, corrects them from the dark and
builds composit frame, loading the result into X_display.
CATEGORY:
calibration, manipulation
CALLING SEQUENCE:
BUILD_FRAOE, image1, image2, image3, image4, oefringe
INPUTS:
image1 first arc of fringe (up)
image2 second & opposite arc of fringe (down)
image3 third arc of fringe (left)
image4 fourth & opposite arc of fringe (right)
KEYWORD PARAMETERS:
None
OUTPUTS:
oefringe resulting composit image
COMMON BLOCKS:
None
SIDE EFFECTS:
None
RESTRICTIONS:
None
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by M.B v.1.0 LAS 03/03/94
NAME: WRITE_IMA
PURPOSE: write image and header to disk file
CATEGORY: BASIC_INTERFACE
CALLING SEQUENCE: WRITE_IMAGE,ima_name,image,hdr
INPUTS: ima_name = string of header filename
image = array containing the image
hdr = header to write to disk
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Writes to disk
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: Creates a new disk file
RESTRICTIONS: Assumes file extensions of .img and .hdr
PROCEDURE:
MODIFICATION HISTORY: RAH 7/2/90
M.BOUT 93/11/16 runs for the new structures
arrays and headers and saves them in two files
NOTE: the procedure VISU_IMA is convenient for the displaying of the saved
files. It's not the case of VISU_CAL.
@(#)write_ima.pro 1.2 4/10/93 :NRL Solar Physics
common ccd_header,header,nt,tags ; Modif. A.LL. 93/05/28
NAME: write_hdr.pro
PURPOSE: write image header to disk file
CATEGORY: General tools low level routine
CALLING SEQUENCE: write_hdr,ima_name,hdr
INPUTS: ima_name = string of header filename
hdr = header to write to disk
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Writes to disk
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: Creates a new disk file
RESTRICTIONS: Assumes a file extension of .hdr
PROCEDURE:
MODIFICATION HISTORY: RAH 10/1/89
RAH 8/20/91 to use = as keyword delimiter
SCCS variables for IDL use
@(#)write_header.pro 1.2 4/10/93 :NRL Solar Physics
NAME: show_hdr.pro
PURPOSE: visualize keywords in Calibration headers
CATEGORY: General tools high level routine
CALLING SEQUENCE: show_hdr or show_hdr,/FULL
INPUTS: None
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: /FULL
OUTPUTS: A list of ima_header
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY:
All 4/25/93 for VMS files in general
SCCS variables for IDL use
@(#)show_hdr.pro 1.3 4/25/93 :LAS
NAME: show_ima_hdr.pro
PURPOSE: visualize keywords from file headers
CATEGORY: General tools high level routine
CALLING SEQUENCE: show_ima_hdr, hdr_name
show_ima_hdr, hdr_name,/FULL
INPUTS: hdr_name Name of header file
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: /FULL
OUTPUTS: A list of ima_header
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY:
All 4/25/93 for VMS files in general
corrected by M.B according to the new features of headers
11/03/93
SCCS variables for IDL use
@(#)show_ima_hdr.pro 1.3 4/25/93 :LAS
NAME: set_cal_hdr.pro
PURPOSE: set some keywords in Calibration headers
CATEGORY: General tools low level routine
CALLING SEQUENCE: set_ima_hdr,ima_header,refpix_x,refpix_y
INPUTS: ima_header = structure
refpix_x = float, (position of reference 0.,0.)
refpix_y = float, (position of reference 0.,0.)
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima_header
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY:
All 4/25/93 for VMS files in general
SCCS variables for IDL use
@(#)set_ima_header.pro 1.3 4/10/93 :NRL Solar Physics
NAME: copy_ima_hdr.pro
PURPOSE: procedure to copy a heder structure in other
header structure
CATEGORY: CCD
CALLING SEQUENCE: copy_ima_hdr,header_in,header_out
INPUTS: header_in = header input,
header_out = new header structure
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: header_out = filled new header
OPTIONAL OUTPUT PARAMETERS:
SIDE EFFECTS:
RESTRICTIONS: corresponding tags must be of same element type
PROCEDURE:
MODIFICATION HISTORY: All 4/25/93 for VMS files from Fusion
SCCS variables for IDL use
@(#)copy_ima_hdr.pro 1.3 4/10/93 :NRL Solar Physics
NAME: w512.pro PURPOSE: create a 512*512 window CATEGORY: General tools high level routine CALLING SEQUENCE: extract_ima2, iin, hin, x1, x2, y1, y2, iout, hout INPUTS: n Window number OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: A image Window in the screen OPTIONAL OUTPUT PARAMETERS: None COMMON BLOCKS: None SIDE EFFECTS: RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: defined by ALL 6/24/93 SCCS variables for IDL use @(#)extract_ima2.pro 1.0 25/6/93 :LAS
NAME: LOAD_IMA.PRO
PURPOSE: Visualize a image array yet in memory
CATEGORY: General tools high level routine
CALLING SEQUENCE: ima, lcut, hcut, kx, ky
INPUTS: ima image array
lcut,hcut low and hight cut
kx, ky zoom parameters
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: image on screen
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)load_ima.pro 1.0 25/6/93 :LAS
NAME: VISU_IMA.PRO
PURPOSE: Put in virtual memory an image array & visualize it
CATEGORY: Visualization high level routine
CALLING SEQUENCE: VISU_IMA, ima_name, hima, ima, kx, ky, lcut, hcut
INPUTS: ima_name image_name
hima,ima IDL assoc names
kx, ky zoom parameters
lcut, hcut cuts values
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Image on screen
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
modified by M.B 11/04/93
SCCS variables for IDL use
@(#)visu_ima.pro 1.0 25/6/93 :LAS
NAME: LOAD_CAL.PRO
PURPOSE: Visualizes a array image of calibration
(in memory yet)
CATEGORY: Preprocessing high level routine
CALLING SEQUENCE: iout = LOAD_CAL ( ima, lcut, hcut, itest,
nx_out, ny_out )
INPUTS: ima image array
lcut,hcut low an hight cuts
itest operating mode for big images
itest eq 1 not rebin
itest ne 1 rebin by 2 if 1124 pix
images ; OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Image on screen
iout
nx_out
ny_out
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)load_cal.pro 1.0 25/6/93 :LAS
CALIB5.PRO
Upper level routines
Stat
Pro EXTRACT_IMA2, iin, hin, x1, x2, y1, y2, iout, hout
; extracts a subimage
Pro STAT_2D_FRM, ima, kx, ky, imb, imc ;Gives local stats over all
;image
Pro STAT_IMA, ima, x1,y1,x2,y2,z ;gives stas in a ROI
Function MIN_2D_FRM, ima, kx,ky
Function STATIMA, ima, x1,y1,x2,y2 ;
Visu
Pro W512, n ;Creates a 512*512 display
Pro VISU_IMA, ima_name, hima, ima, kx, ky, lcut, hcut ;Visualizes an image
Function LOAD_IMA, ima, lcut, hcut, kx, ky ;Visualizes a loaded ima;
Calib. processing
Pro VISU_CAL,ima_name, iout, hout ;Gets a CAL ima, rectifies
and visu. it
Pro VISU_CAL_CLEAN, ima_name, backg, iout, hout ;Gets a CAL ima, rectifies
subtracts and visu. it
Pro READ_CAL,ima_name, itest, iout, hout ;Gets a CAL ima. rectified
Pro CLEAN_CAL, ima, hima, itest, iout, hout ;rectifies a CAL image
Function LOAD_CAL(ima,hima,lcut,hcut,itest,hout) ;rectifies a CAL image and
visu. it
Pro SET_CAL_HDR, hdr, refpix_x, refpix_y ;Sets cal parameters
Catalogs of images
Pro DARK_CATA ; (CATA)
Pro SHOW_CATALOG ; (CATA)
Pro CHOOSE_DARK, dark_new_name, drk, hdrk ; (CATA)
Pro PRO_CAL, ima_name, drk, hdrk, ima, hima ;process a CAL with
catalogued darks (CATA)
Pro GET_DRK_NAME, ima_name, ass_name ; (CATA)
Pro SET_CATALOG, template, db_ima, nima, ima_name
Pro FIND_IMA, hdr, ima_db, ima_name
Pro IMA_LIST, template, ima_db, nfiles
Function DEFINE_CATALOG( nfiles )
Basic I/O
Pro WRITE_IMA, ima_name, ima, hdr ;Stores an image and a hdr
Pro SHOW_HDR, ima_hdr, FULL = I ;Shows some hdr parameters
Pro COPY_IMA_HDR, hdr_in, hdr_out ;Copies a header
Function READ_IMA( ima_name, hdr, ichoice ) ;opens an image from stor.
Low level routines
Function GETTOK(st,char)
Function DATE_CAL( date, hour )
Pro DATE_NUM_TEXT,year,month,day,hour
Function DEFINE_IMA_HDR( dummy )
Function DEFINE_CAL_HDR( dummy )
Function DEFINE_BSC_HDR( dummy )
Function DEFINE_C1_HDR( dummy )
Function DEFINE_CCD_HDR( dummy )
Function READ_IMA_HDR( ima_name, hdr, itest )
Function READ_IMA_FRAME( ima_name, bitpix, nx, ny )
Pro WRITE_HDR,ima_name, hdr
Pro CHECK_IMGDIR, dummy
Pro CHECK_FILENAME, filename, path, extension
A.LL.
NAME: visu_cal_clean.pro
PURPOSE: Gets a calib. image from disk, subtracts dark, and visualizes it
CATEGORY: Calibration high level routine
CALLING SEQUENCE: VISU_CAL_CLEAN, ima_name, backg, ima, hdr
INPUTS: ima_name image name of calibration
backg background image array
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Image on screen
ima image array
hdr header of image array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: hdr array is defined as DEFINE_IMA_HDR
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)visu_cal_clean.pro 1.0 25/6/93 :LAS
NAME: read_cal.pro
PURPOSE: Gets a calibration image from disk and visualizes it
CATEGORY: Calibrations high level routine
CALLING SEQUENCE: READ_CAL, ima_name, itest, ima, hdr
INPUTS: ima_name image name of calibration
itest =0 rebin si nx = 1124
=1 no rebin pour nx = 1124
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Image on screen
ima image array
hdr header of image array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: hdr array is defined as DEFINE_IMA_HDR
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)read_cal.pro 1.0 25/6/93 :LAS
NAME: visu_cal.pro
PURPOSE: Gets a calibration image from disk and visualizes it
CATEGORY: Calibrations high level routine
CALLING SEQUENCE: VISU_CAL, ima_name, ima, hdr
INPUTS: ima_name image name of calibration
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: Image on screen
ima image array
hdr header of image array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: hdr array is defined as DEFINE_IMA_HDR
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)visu_cal.pro 1.0 25/6/93 :LAS
NAME: CLEAN_CAL.PRO
PURPOSE: Resizes and rotates a calibration image array
CATEGORY: Calibrations high level routine
CALLING SEQUENCE: CLEAN_CAL, ima, hima, itest, iout, hout
INPUTS: ima image array of calibration
hima header
itest operating mode for big images
itest eq 1 not rebin
itest ne 1 rebin by 2 if 1124 pix
images
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:iout image array
hout header of image array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: hdr array is defined as DEFINE_IMA_HDR
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)clean_cal.pro 1.0 25/6/93 :LAS
NAME: stat_2d_frm.pro
PURPOSE: Build a image of means and a image of sd (standard deviations)
CATEGORY: General tools high level routines, Statistics.
CALLING SEQUENCE: stat_2d_frm, ima,kx,ky,imb,imc
INPUTS: ima image array
kx step_size in x
ky step_size in y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:imb image array of means
imc image array of sd. deviations
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)stat_2d_frm.pro 1.0 25/6/93 :LAS
NAME: stat_ima.pro
PURPOSE: local statistics in a image array (in memory)
CATEGORY: General tools high level routine
CALLING SEQUENCE: stat_ima, ima, x1, x2, y1, y2, z
INPUTS: ima image array
x1,x2 x interval of rectangle
y1,y2 y interval of rectangle
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:z array of values
z(0) = ntot
z(1) = sum
z(2) = moy
z(3) = std
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)stat_ima.pro 1.0 25/6/93 :LAS
NAME: MIN_2D_FRM.PRO
PURPOSE: make an image of local minima
CATEGORY: General tools high level routine
CALLING SEQUENCE: ima_out = min_2d_frm( ima_in, kx, ky)
INPUTS: ima_in image array
kx step_size in x
ky step_size in y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:ima_out mapping of local minima
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B and A.LL 26/10/93
SCCS variables for IDL use
@(#)min_2d_frm.pro 1.0 26/10/93 :LAS
NAME: statima.pro
PURPOSE: extract a image from another
CATEGORY: General tools high level routine
CALLING SEQUENCE: extract_ima2, iin, hin, x1, x2, y1, y2, iout, hout
INPUTS: iin image array
hin header of image array
x1,x2 x interval of rectangle
y1,y2 y interval of rectangle
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:iout extracted image array
hout header for extracted image
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: opens a catalog of darks
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)extract_ima2.pro 1.0 25/6/93 :LAS
NAME: extract_ima2.pro
PURPOSE: extract a image from another
CATEGORY: General tools high level routine
CALLING SEQUENCE: extract_ima2, iin, hin, x1, x2, y1, y2, iout, hout
INPUTS: iin image array
hin header of image array
x1,x2 x interval of rectangle
y1,y2 y interval of rectangle
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:iout extracted image array
hout header for extracted image
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: opens a catalog of darks
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
corrected by M.B 11/03/93 for header's filling
SCCS variables for IDL use
@(#)extract_ima2.pro 1.0 25/6/93 :LAS
NAME:DEFINE_CATALOG.pro PURPOSE Sets a array of structures for a image catalog CATEGORY: Preprocessing low level CALLING SEQUENCE: db = DEFINE_CATALOG(nfiles) INPUTS: nfiles Nombre max of files in catalog OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: a array structure for catalog OPTIONAL OUTPUT PARAMETERS: None COMMON BLOCKS: None SIDE EFFECTS: None RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: defined by ALL 6/24/93 SCCS variables for IDL use @(#)DEFINE_CATALOG.pro 1.0 25/6/93 :LAS
NAME: define_ima_hdr
PURPOSE: defines a image header structure
CATEGORY: BASIC_INTERFACES
CALLING SEQUENCE: hdr = define_ima_hdr(0)
INPUTS: None
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: structure array containing initialized an header
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: RAH 10/1/89
RAH 8/20/91 Added AES BSBD camera keywords
ALL 04/27/93 takes only standard KEYWORDS
SCCS variables for IDL use
@(#)define_ima_hdr.pro 1.1 7/6/92 :NRL Solar Physics
;;common ccd_header,header,nt,tags
NAME: DATE_NUM_TEXT.PRO PURPOSE: Gives a set of date strings, ex: 12, 09, 1994 (for the 12 Sep 1994) A.LL.
NAME: IMA_LIST.pro
PURPOSE: list the catalog of images (corresp to a template)
CATEGORY: Preprocessing low level routine
CALLING SEQUENCE: DARK_LIST, template, ima_db, nfiles
INPUTS: template Template to define the list of images
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:ima_db image catalog
nfiles Number of images in catalog
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: opens a catalog of darks
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)ima_list.pro 1.0 25/6/93 :LAS
NAME: find_ima.pro
PURPOSE: From the image header finds the asociate dark in dark catalog
CATEGORY: Preprocessing low level
CALLING SEQUENCE: find_ima, hdr, ima_db, ima_name
INPUTS: hdr image header
ima_db image catalog
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:ima_name name of associated image in catalog
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
corrected by M.B 11/03/93 for darks without shutter
SCCS variables for IDL use
@(#)find_ima.pro 1.0 25/6/93 :LAS
NAME: SET_CATALOG.PRO
PURPOSE: Set a catalog of images in memory
CATEGORY: Preprocessing high level routine
CALLING SEQUENCE: SET_CATALOG
INPUTS: template Template For image names
db_dark Liste of images
ndarks Number of images in catalog
drk_name Associate dark name
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: catalog list in the screen
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: opens a catalog of darks if it don't exists
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)set_catalog.pro 1.0 25/6/93 :LAS
NAME: show_catalog.pro PURPOSE: list the catalog in memory CATEGORY: Preprocessing CALLING SEQUENCE: SHOW_CATALOG INPUTS: None OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: catalog list in the screen OPTIONAL OUTPUT PARAMETERS: None COMMON BLOCKS: CATA, db_dark, ndarks, drk_name SIDE EFFECTS: opens a catalog of darks if this dont exists RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: defined by ALL 6/24/93 SCCS variables for IDL use @(#)show_catalog.pro 1.0 25/6/93 :LAS
NAME: list_ima_param.pro PURPOSE: list the catalog in memory CATEGORY: Preprocessing CALLING SEQUENCE: CHOOSE_DARK, drk_new_name, drk, hdrk INPUTS: template Template of files names to list OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: catalog lis in the screen OPTIONAL OUTPUT PARAMETERS: None COMMON BLOCKS: None SIDE EFFECTS: None RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: defined by ALL 6/24/93 SCCS variables for IDL use @(#)list_ima_param.pro 1.0 25/6/93 :LAS
NAME: choose_dark.pro
PURPOSE: defines a dark frame as the active dark
CATEGORY: Preprocessing
CALLING SEQUENCE: CHOOSE_DARK, drk_new_name, drk, hdrk
INPUTS drk_new_name Name of dark array
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: drk array of data
hdrh header of data array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: CATA, db_dark, ndarks, drk_name
SIDE EFFECTS: fullfills the dark catalog common
if it don't exists
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)choose_dark.pro 1.0 25/6/93 :LAS
NAME: get_drk_name.pro
PURPOSE: founds de associate dark frame for
a image and gets their name
CATEGORY: Preprocessing high level
CALLING SEQUENCE: get_drk_name, ima_name, drk_name
INPUTS: ima_name Name of image
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ass_name Name of associate dark frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: CATA, db_dark, ndarks, drk_name
SIDE EFFECTS: 1) defines de found dark as the active dark
2) fullfills the dark catalog common if it
don't exists
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)get_drk_name.pro 1.0 25/6/93 :LAS
NAME: DARK_CATA.pro
PURPOSE: Set a catalog of darks in memory
CATEGORY: Preprocessing high level routine
CALLING SEQUENCE: SET_CATALOG
INPUTS: None
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: catalog list in the screen
Modifies CATA common
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: CATA, db_dark, ndarks, drk_name
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
SCCS variables for IDL use
@(#)set_catalog.pro 1.0 25/6/93 :LAS
NAME: pro_cal.pro
PURPOSE: get in memory an image and
substracts the right dark
CATEGORY: Preprocessing high level routine
CALLING SEQUENCE: PRO_CAL, ima_name, drk, hdrk, iout, hout
INPUTS: ima_name Name of image to process
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: drk Associate dark array
hdrk Associate header of dark
iout Corrected image array
hout Header for corrected image array
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: CATA, db_dark, ndarks, drk_name
SIDE EFFECTS: opens a catalog of darks if this doesn't exist
and associates a dark to frame
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: defined by ALL 6/24/93
rewritted and corrected by M.B 11/04/93
SCCS variables for IDL use
@(#)pro_cal.pro 1.0 25/6/93 :LAS
NAME: define_C1_Hdr PURPOSE: defines the C1 (PF) header structure CATEGORY: General tools Low level routine CALLING SEQUENCE: h=define_C1_hdr (0) INPUTS: None OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: h struct. array containing initialized an header OPTIONAL OUTPUT PARAMETERS: COMMON BLOCKS: none SIDE EFFECTS: RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: define_ccd_hdr RAH 10/1/89 RAH 8/20/91 define_ccd_hdr Added AES BSBD camera keywords ALL 6/24/93 Remove common, changes to define_C1_hdr SCCS variables for IDL use @(#)define_c1_hdr.pro 1.1 7/6/92 :NRL Solar Physics
NAME: define_cal_hdr PURPOSE: defines header structure for cal. images of C2 and C3 CATEGORY: General tools low level routines CALLING SEQUENCE: h=define_cal_hdr (0) INPUTS: None OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: h struct. array containing initialized an header OPTIONAL OUTPUT PARAMETERS: COMMON BLOCKS: none SIDE EFFECTS: RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: define_ccd_hdr RAH 10/1/89 RAH 8/20/91 define_ccd_hdr Added AES BSBD camera keywords ALL 6/24/93 Remove common, changes to define_cal_hdr SCCS variables for IDL use @(#)define_ccd_hdr.pro 1.1 7/6/92 :NRL Solar Physics
NAME: define_BSC_Hdr PURPOSE: defines the basic header structure for lasco images CATEGORY: General tools low level routine CALLING SEQUENCE: h=define_bsc_hdr (0) INPUTS: None OPTIONAL INPUT PARAMETERS: None KEYWORD PARAMETERS: None OUTPUTS: struct. array containing initialized an header OPTIONAL OUTPUT PARAMETERS: COMMON BLOCKS: none SIDE EFFECTS: RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: RAH 10/1/89 RAH 8/20/91 Added AES BSBD camera keywords ALL 6/24/93 Remove common, adapts for a basic set of KEYWORDS SCCS variables for IDL use @(#)define_bsc_hdr.pro 1.1 7/6/92 :NRL Solar Physics
NAME: define_CCD_Hdr
PURPOSE: defines the CCD header structure
CATEGORY: CCD low level routine
CALLING SEQUENCE: h=define_CCD_hdr (0)
INPUTS: None
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: struct. array containing initialized an header
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: ccd_header,header,nt,tags
header = the header structure
nt = number of elements in the header
tags = string array of names of header items
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: RAH 10/1/89
RAH 8/20/91 Added AES BSBD camera keywords
SCCS variables for IDL use
@(#)define_ccd_hdr.pro 1.1 7/6/92 :NRL Solar Physics
NAME: read_ima_hdr
PURPOSE: function procedure to read header from disk file, f
and store in a standard header structure type
CATEGORY: BASIC_INTERFACES
CALLING SEQUENCE: read_ima_hdr,ima_name,ima_header
INPUTS: ima_name = string containing the header filename
ima_header = structure
verbose = 1, print all absent variables
verbose = 0, print only a resumee
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima_header = header structure from disk
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: RAH 10/1/89, ACG 11/21/89, rah 1/9/91
rah 3/15/91 to account for unrecognized keyword
rah 8/20/91 to trim leading and trailing blanks
DW 8/27/91 change delimiter to '='
DW 2/26/93 put TEMP_FNG in TEMP as well
All 4/25/93 for VMS image files in general
Common supression
SCCS variables for IDL use
@(#)read_ima_header.pro 1.3 4/10/93 :NRL Solar Physics
NAME: READ_IMA_FRAME
PURPOSE: reads a image frame from disk
CATEGORY: BASIC_INTERFACE
CALLING SEQUENCE: a = read_ima_frame(name,bitpix,nx,ny)
INPUTS: name = string of the name of the file to read
bitpix = nb of bits/pixel
nx = nb de pixels en x
ny = nb de pixels en y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: a = array containing the image
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: RAH 7/2/90
rah 3/21/90 to account for non-integer input fil
es
rah 3/33/90 to check for datamax & datamin
ALL 5/12/93
SCCS variables for IDL use
@(#)read_ima_frame.pro 1.3 4/10/93 :NRL Solar Physics
NAME: read_ima
PURPOSE: reads a image and their header
CATEGORY: BASIC_INTERFACES
CALLING SEQUENCE: ima = read_ima(ima_name, hdrima, ichoice)
INPUTS: ima_name Name of image
hdrima Header structure
ichoice Type of header
0 = IMA, 1 = BSC, 2=CAL, 3=C1
4 = CCD. else external header
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima Image frame
hdrima Filled header structure
OPTIONAL OUTPUT PARAMETERS:
COMMON BLOCKS: None
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY: RAH 10/1/89
RAH 8/20/91 Added AES BSBD camera keywords
ALL 04/27/93 takes only standard KEYWORDS
SCCS variables for IDL use
@(#)read_ima.pro 1.1 7/6/92 :NRL Solar Physics
NAME:
check_filename
PURPOSE:
Removes the extension and path from the filename
if present
CALLING SEQUENCE:
check_filename,filename
check_filename,filename,path,extension
INPUTS:
filename = string to be checked (may be a string array)
OUTPUTS:
filename will be returned without extension and path
OPTIONAL OUTPUTS:
path = path name
extension = extension not including decimal point
MODIFICATION HISTORY:
RAH 10/1/89
rah 3/28/91 added array input for filename
ALL 5/15/93 adapted to VMS
SCCS variables for IDL use
@(#)check_filename.pro 1.1 7/6/92 :NRL Solar Physics
NAME:
check_imgdir
PURPOSE:
checks !imgdir for a / on the end
CALLING SEQUENCE:
check_imgdir
INPUTS: None
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
PROCEDURE:
if !imgdir does not end with / then puts one on
MODIFICATION HISTORY: RAH 3/26/91
ALL 5/15/93 adapted to VAX VMS
SCCS variables for IDL use
@(#)check_imgdir.pro 1.1 7/6/92 :NRL Solar Physics
NAME: crosscorr.pro
PURPOSE: determination of the function of crossing-
correlation between two frames and the off-
centering between these two frames.
CATEGORY: Processing high level
CALLING SEQUENCE: crosscorr,ima1_in,ima2_in,x1,x2,y1,y2,ima_out,res
INPUTS: ima1_in name of 1st frame
ima2_in name of 2nd frame
x1,x2,y1,y2 selected area
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima_out cross-correlation frame
res maxima's area reinterpolated
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: The cubic interpolation is maded by Rinter.pro
who has to be compiled before applications.
This program runs well with even frames
(dimensions paires en X et en Y)
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 01/14/94
SCCS variables for IDL use
@(#)crosscorr.pro 1.0 01/17/94 :LAS
NAME: crosscorrbis.pro
PURPOSE: determination of the function of crossing-
correlation between two frames and the off-
centering between these two frames.
CATEGORY: Processing high level
CALLING SEQUENCE: crosscorrbis,ima1_in,ima2_in,x1,x2,y1,y2,ima_out,res
INPUTS: ima1_in name of 1st frame
ima2_in name of 2nd frame
x1,x2,y1,y2 selected area
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima_out cross-correlation frame
res maxima's area reinterpolated
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: The sinc interpolation is maded by resample.pro
included in utilities.pro who has to be compiled
before applications.
This program runs well for even frames
(dimensions paires en X et en Y)
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 01/20/94
SCCS variables for IDL use
@(#)crosscorrbis.pro 1.0 01/20/94 :LAS
NAME:
DATE_CAL
PURPOSE:
Procedure to perform conversion of dates to decimal form
format: string (ascii text) encoded as
DD MON YEAR for date
HH:MM:SS.SS for hour
(eg. 14 JUL 1987 15:25:44.23)
CALLING SEQUENCE
jt = DATE_CAL( DATE, HOUR )
INPUTS:
DATE - input date in one of the three possible formats
OUTPUTS:
The converted date is returned as the function value.
HISTORY:
version 1 D. Lindler July, 1987
adapted for IDL version 2 J. Isensee May, 1990
adapted from DATE_CONV to lasco use A.LL.
990126 Ed Esfandiari Fixed for Y2K problem.
NAME:
DCURSOR.PRO
PURPOSE:
put the pixels coordinates & the pixels values selected with the
cursor in a table that can be readed.
CATEGORY:
array manipulation
CALLING SEQUENCE:
DCURSOR, ima, tab_name, n_points
INPUTS:
ima image array (in memory)
tab_name name of table that receives the values
n_points number of points in the table
KEYWORD PARAMETERS:
None
OUTPUTS:
values writted in the table
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by M.B v.1.0 : LAS 01/27/94
ro drawcircle, ima_in, x_cntr, y_cntr, radius, ptyp, psiz, color ; Draw a circle of given radius and given center on a frame ; Created by M.B on 31/01/94 : LAS v1.0 ; Modified by M.B on 17/02/94 : LAS ; inputs : ; ima_in image that receives the picture ; x_cntr, y_cntr center coordinates of the drawn circle ; radius radius of the drawn circle ; ptyp selected drawn points (0 --> 9) ; psiz heigth of the drawn points (scale*1.) ; color color of the drawn points (0(black) --> 255(white)) ; outputs : ; on the selected window, the picture appears
NAME: filtgauss.pro
PURPOSE: gaussian filtering applications
CATEGORY: Processing high level
CALLING SEQUENCE: filtgauss,ima_in,width,ima_out
INPUTS: ima_in name of frame
width width '1/e' of gaussian
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: ima_out resulting frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: Applications limited to 512*512 frames
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 01/07/94
SCCS variables for IDL use
@(#)filtgauss.pro 1.0 01/07/94 :LAS
RO GCURSOR,TABLE_NAME,N_POINTS
created by M.BOUT, LAS, 931118
the graphic cursor becomes enable and a group of points taken on the
plot are printed & writed into a given table.
NAME: GETTOK PURPOSE: Function to retrieve the first part of the string until the character char is encountered. CALLING SEQUENCE: token = gettok( st, char ) INPUT: char - character separating tokens, scalar string INPUT-OUTPUT: st - (scalar) string to get token from (on output token is removed) OUTPUT: token - scalar string value is returned EXAMPLE: If ST is 'abc=999' then gettok(ST,'=') would return 'abc' and ST would be left as '999' HISTORY version 1 by D. Lindler APR,86 Remove leading blanks W. Landsman (from JKF) Aug. 1991
NAME: lux_diff.pro
PURPOSE: make an image of the scattering function
CATEGORY: Processing high level
CALLING SEQUENCE: lux_diff,ima_name,Xc,Yc,OPTION,A,B
INPUTS: ima_name Name of result
OPTIONAL INPUT PARAMETERS: Xc,Yc center's coords
OPTION function's chars
KEYWORD PARAMETERS: None
OUTPUTS: ima_name scattering funct
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: Applications limited to 512*512 frames
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 10/11/93
SCCS variables for IDL use
@(#)lux_diff.pro 1.0 10/11/93 :LAS
NAME: FILTMEDIAN.PRO
PURPOSE: apply a median filter and rebin in the same time.
CATEGORY: General tools high level routine
CALLING SEQUENCE: filtmedian,ima_in,kx,ky,ima_out
INPUTS: ima_in image array
kx step_size in x
ky step_size in y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:ima_out resulting frame
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 20/01/94
SCCS variables for IDL use
@(#)filtmedian.pro 1.0 20/01/94 :LAS
ro pattern1,ima1,ima2,ima3,ima4,difres ;; by M.B :LAS 21/01/94 extract & display the pattern of ccd
ro pattern2,difres1,difres2,difres_out ;; by M.B :LAS 21/01/94 magnify the pattern (shunt aleatory peaks) & give ;; the signal/noise ratio
NAME:
PCURSOR.PRO
PURPOSE:
Plot cursor position on display and
put the pixels coordinates selected with the
cursor in a table that can be readed.
CATEGORY:
array manipulation
CALLING SEQUENCE:
PCURSOR,IMA,TAB_NAME
INPUTS:
IMA : IMAGE INPUT
KEYWORD PARAMETERS:
None
OUTPUTS:
TAB_NAME : table des coordonnees des points selectionnes
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by JP.L & M.B v.1.0 : LAS 01/27/94
NAME: MEAN_2D_FRM.PRO
PURPOSE: make an image of local means and of standard deviation
CATEGORY: General tools high level routine
CALLING SEQUENCE: mean_2d_frm,ima_in,kx,ky,ima_moy,ima_std
INPUTS: ima_in image array
kx step_size in x
ky step_size in y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:ima_moy mapping of local means
ima_std mapping of local sigmas
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 07/12/93
SCCS variables for IDL use
@(#)mean_2d_frm.pro 1.0 07/12/93 :LAS
NAME: POLM1M2.PRO
PURPOSE: make images of local means and of standard deviation for
the Stokes parameters, the fractionnal polarization & direction of
polarization for the light of calib lamps after passing thru mirrors
CATEGORY: General tools high level routine
CALLING SEQUENCE: polm1m2,I1p,I2p,I3p,kx,ky,P_moy,P_std,alpha_moy,alpha_std
INPUTS: I1p image array of intensity with pol-60
I2p image array of intensity with pol00
I3p image array of intensity with pol+60
kx step_size in x
ky step_size in y
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS:P_moy mapping of local means for polarization
P_std mapping of local sigmas for polarization
alpha_moy mapping of local means for direction
alpha_std mapping of local sigmas for direction
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: None
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 07/12/93
SCCS variables for IDL use
@(#)polm1m2.pro 1.0 07/12/93 :LAS
NAME:
REPLACIMA.PRO
PURPOSE:
Select an interval of pixels values and replace these one by another
CATEGORY:
??
CALLING SEQUENCE:
REPLACIMA, IMA, minval, maxval, selectval
INPUTS:
ima image array (in memory)
minval lower cuts value selected
maxval higher cuts value selected
selectval new value of pixels between lcuts & hcuts
KEYWORD PARAMETERS:
None
OUTPUTS:
ima with the selected intervals replaced
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by M.B v.1.0 LAS 12/13/93
UNCTION RINTER, P, X, Y, DFDX, DFDY + NAME: RINTER PURPOSE: Cubic interpolation of an image at a set of reference points points. Optionally obtain the X and Y derivatives at these points. Used by the DAOPHOT PSF sequence but can also be for general cubic interpolation. CALLING SEQUENCE: Z = RINTER( P, X, Y, [ DFDX, DFDY ] ) INPUTS: P - Two dimensional data array, X - Either an N element vector or an N x M element array, containing X subscripts where cubic interpolation is desired. Y - Either an N element vector or an N x M element arra, containing Y subscripts where cubic interpolation is desired. OUTPUT: Z - Result = interpolated vector or array. If X and Y are vectors, then so is Z, but if X and Y are arrays then Z will be also. If P is DOUBLE precision, then so is Z, otherwise Z is REAL. OPTIONAL OUTPUT: DFDX - Vector or Array, (same size and type as Z), containing the derivatives with respect to X DFDY - Array containing derivatives with respect to Y EXAMPLE: suppose P is a 256 x 256 element array and X = FINDGEN(50)/2. + 100. and Y = X. Then Z will be a 50 element array, containing the cubic interpolated points. SIDE EFFECTS: can be time consuming. RESTRICTION: Interpolation is not possible at positions outside the range of the array (including all negative subscripts), or within 2 pixel units of the edge. No error message is given but values of the output array are meaningless at these positions. PROCEDURE: invokes CUBIC interpolation algorithm to evaluate each element in Z at virtual coordinates contained in X and Y with the data in P. COMMON BLOCKS: If repeated interpolation of the same array is to occur, then one can save time by initializing the common block RINTER REVISION HISTORY: March 1988 written W. Landsman STX Co. Checked for IDL Version 2, J. Isensee, September, 1990 Corrected call to HISTOGRAM, W. Landsman November 1990
unction round1,var ;; by JP.L & M.B at LAS : 02/11/94 ;;Arrondit la variable a la valeur la plus proche
NAME:
STAT_CURSOR.PRO
PURPOSE:
Draws a box in a image and does a statistic (mean and standard
deviation inside
CATEGORY:
??
CALLING SEQUENCE:
STAT_CURSOR, ima
INPUTS:
ima image array (in memory)
KEYWORD PARAMETERS:
None
OUTPUTS:
Values
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by A.LL v.1.0 LAS 08/25/93
PROJECT:
SOHO - LASCO
NAME:
t_param.pro
PURPOSE:
Gets main telescope parameters
CALLING SEQUENCE:
value = t_param( detector, key )
EXAMPLE
pixsze = t_param('C2','PIXEL')
INPUTS:
detector 'C1','C2','C3' STRING
key parameter name STRING
'PIXEL' pixelsize (in mm)
'SCALE' angular scale for pixel (in deg)
'FOCAL' equivalent focal (in mm)
'FIELD' field (in deg)
'DFIELD' diagonal field (in deg)
'BIAS' electric bias of each amplifier (in ADU)
get byas from offset_bias.pro (needs the header)
'OCCULTER' radius of occlusion due to internal oculter
in 'CCD pixel units'
'DISTORTION' set of coefs of distortion (to be used in mm)
NOTE: drho = a0*rho+a1*rho^3+a2*rho^5
'DISCNTR' distortion center (in mm)
'CENTER' Sun center (in pixels)
'OCCENTER' occulter center (in pixels)
KEYWORD INPUT
none
OUTPUTS:
value searched value
OUTPUTS INPUTS:
none
PROCEDURE:
Gets parameters from a set of internal data
CALLED PROCEDURES:
none
HISTORY:
Def. and code: A.Llebaria (LAS-CNRS) Aug 1996
Corrected and modified by Dr. M.-V. Bout on March, 4th, 1998
NOTA :
Distortion parameters: ; rho*(a0+a1*rho^2+a2*rho^4)
history
pm.distortion = [0.0060519645, -0.00014672423, 2.0899603e-07]
list9604_1ora_00_g_ldist.dat
pm.distortion = [0.0051344125, -0.00012233862, 1.0978595e-07]
list9603_1ora_00_a_ldist.dat
pm.distortion = [0.0044836143, -0.00011276272, 5.9968042e-08]
list9602_2ora_00_a_ldist.dat
pm.distortion = [0.0051344125, -0.00012233862, 1.0978595e-07]
list9603_1ora_00_a_ldist.dat
pm.distortion = [0.0056511656, -0.00013827504, 1.6940201e-07]
list9604_1ora_00_h_ldist.dat
.NAME:
utilities.pro
.PURPOSE:
Define a bunch of handy IDL utilities.
.COMMENT:
Compile with ".run utilities" from IDL V2.
.AUTHOR:
Hans-Martin Adorf
Space Telescope - European Coordinating Facility
European Southern Observatory
D-8046 Garching bei Muenchen
Karl-Schwarzschild-Str. 2
F.R. Germany
Internet: adorf@eso.org SPAN: ESO::ADORF or adorf@eso.span
.MODIFICATION HISTORY:
Jul 1990 HMA Initial implementation
Aug 1990 HMA Further improvements
Sep 1991 HMA Some comments provided
Oct 1991 HMA Added new features
Feb 1992 HMA Added new utilities
jan 1994 M.B Truncated version for IDL v 3.1.1 <==> LASCO
.TO DO
Introduce global variables to control, e.g. the verbosity of
graphics and image display of intermediate results.
unction vignettage,xc,yc ; created by M.B on 02/02/94 at LAS ; modified by M.B on 04/03/94 at LAS ; construction of a normalized model of vignetting function for LASCO ; This model can be used for vignetting of solar corona frames ; inputs : ; ; xc,yc center coordinates of internal occultor ; ; outputs : ; model name of the resultant image ; ; restrictions : ; the generated model is 512*512 pixels
NAME: crevig.pro
PURPOSE: construction of the vignetting function for
LASCO/C2 coronagraph using the bidimensionnal
convolution filtering method
CATEGORY: Processing high level
CALLING SEQUENCE: crevig,ima_name,off_x,off_y
INPUTS: ima_name name of the simulation result
off_x,off_y off-centering of the occultor
OPTIONAL INPUT PARAMETERS: None
KEYWORD PARAMETERS: None
OUTPUTS: image of given name
OPTIONAL OUTPUT PARAMETERS: None
COMMON BLOCKS: None
SIDE EFFECTS: None
RESTRICTIONS: This procedure is adapted to 512*512 frames
PROCEDURE:
MODIFICATION HISTORY: defined by M.B 02/07/94
SCCS variables for IDL use
@(#)crevig.pro v 1.0 02/07/94 :LAS
unction lunule,R1,R2,d
ro crevig,ima_name,off_x,off_y
NAME:
WRITIMA.PRO
PURPOSE:
Draws a box in an image and replaces all pixels values inside
the box by the given value
CATEGORY:
??
CALLING SEQUENCE:
WRITIMA, ima, val
INPUTS:
ima image array (in memory)
val value to be written
KEYWORD PARAMETERS:
None
OUTPUTS:
ima with the selected intervals replaced
COMMON BLOCKS:
None.
SIDE EFFECTS:
None
RESTRICTIONS:
PROCEDURE:
Straightforward.
MODIFICATION HISTORY:
Written by M.B v.1.0 LAS 12/13/93
lasco_mk_html_help.pro on
Wed Aug 17 12:21:56 2005.