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Full Version: How can I remove banding effect from .cub file Magellan Venus
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ncc1701d
I have this .cub file of a section of Venus taken by Magellan that I got from map-a-planet2. Picture included below. You can see the striping effect. Does anyone know of a way to remove this banding effect easily in ISIS3 or another tool?
The best answer I have to far is using "Equalizer" in ISIS3
https://isis.astrogeology.usgs.gov/Applicat.../equalizer.html


Problem though is it looks like you have to fix it using the original striped input images before they are assembled into a .cub.
All I have though is the .cub that was already mosaicked.
Any suggestions on how to remove the striped effect at this point?
I dont believe those orginal individual striped images are avaible to public.
All I know of is the 130 gb .cub file found on mapaplanet2 from which this image was taken from.
thanks
Bjorn Jonsson
dstripe in ISIS3 can remove striping but the problem is that the stripes have to be vertical or horizontal (maybe you could rotate the image before destriping?).

See https://isis.astrogeology.usgs.gov/Applicat...pe/dstripe.html
mcaplinger
QUOTE (ncc1701d @ Feb 1 2016, 11:58 PM) *
I dont believe those orginal individual striped images are avaible to public.

Sure they are. They're called Full Resolution Basic Image Data Records or F-BIDRs. See http://pds-geosciences.wustl.edu/missions/magellan/

Getting rid of shading at the boundaries of the swaths was extremely difficult because of radar artifacts. Maybe in the 20+ years since I've looked at Magellan data someone has improved the processing.
JohnVV
if you want i just gave a copy of my 131072x65536 pixel de striped Venus map to the Mesa Arizona CC planetarium
from the C1 data set

this will save you about 6 months or more of work
the black and white is 8 Gig the color is 24 gig in isis3 cub format and georeferenced
--

--





Dsrtipe is what i used after remapping to Mercator and rotating sections of the C1 data to vertical
( the strips are on a " s "curve )

for the missing "No-data" areas i inpainted using the Resynthesizer plugin for gimp
combined with inpainting using the Greyc laboratories "Greystoration" tool


QUOTE
I dont believe those orginal individual striped images are avaible to public.

yes they are
the C1 is here
http://pds-imaging.jpl.nasa.gov/data/mgn-v...5-midr-c1-v1.0/
the FULLRES "F-BIDR"
http://pds-imaging.jpl.nasa.gov/data/mgn-v...-full-res-v1.0/
JohnVV
an example from the C1
http://pds-imaging.jpl.nasa.gov/data/mgn-v...0n335/c1f12.img
http://pds-imaging.jpl.nasa.gov/data/mgn-v...0n335/c1f12.lbl

CODE
pds2isis from=c1f12.lbl image=c1f12.img to=c1f12.cub


use "qview's" tool measure for the angle
-- 5.6 in this case

CODE
rotate from=c1f12.cub to=work.cub degrees=5.6


CODE
dstripe from=work.cub to=work1.cub vlnl=137 vlns=3 vhnl=3 vhns=137


CODE
rotate from=work1.cub to=c1f12A.cub degrees=-5.6

( you will need to fix the mapping and extra border on the image after the second rotate

Ian R
That's amazing, John. Somewhat on a tangent, could these techniques be utilized to clean-up the USGS Titan radar mosaic, as seen here:

http://astrogeology.usgs.gov/search/detail...n180_128ppd/cub

Furthermore, as someone who doesn't have access to ISIS, would the CUB file preserve the SAR swathes in separate layers?
JohnVV
ian

for that cub ?? no

if you work with each of the radar passes and mosaic then one at a time ?? then maybe ??
but "noseam" would be a better tool

back on target for the thread

The dstripe tool works best on very regular noise and for it's intended use
-- see the images here
https://isis.astrogeology.usgs.gov/Applicat...pe/dstripe.html
mcaplinger
Given how well this worked, I'm surprised no one has gone back and reprocessed the whole C1-MIDR dataset like this. There's this -- http://www.celestiamotherlode.net/catalog/...p?addon_id=1070 -- but I haven't looked at it.
JohnVV
mcaplinger

that IS my map on the Celestia motherload
( libido also ask me not to host any more 12+ gig files )

in 2011 / 2012 over the winter i reworked the C1 data
mcaplinger
QUOTE (JohnVV @ Feb 3 2016, 12:49 PM) *
in 2011 / 2012 over the winter i reworked the C1 data

Is the georeferenced CUB version online anywhere? Maybe USGS should be using that since it's so much better than the original version.
JohnVV
my large map is here:
-- do to age the below links do not work
if someone needs it PM me
https://drive.google.com/file/d/0B6ZYAd08tZ...iew?usp=sharing
and
https://drive.google.com/open?id=0B6ZYAd08t...SXpvS1V1T3R5bDg

this 4.91 gig zip ( would be smaller if i used xz archive) unzips to a 8 gig , 1 band isis3 cub file 131072 x 65536 pixels


this is the header
CODE
Object = IsisCube
  Object = Core
    StartByte   = 65537
    Format      = Tile
    TileSamples = 2048
    TileLines   = 2048

    Group = Dimensions
      Samples = 131072
      Lines   = 65536
      Bands   = 1
    End_Group

    Group = Pixels
      Type       = UnsignedByte
      ByteOrder  = Lsb
      Base       = 0.0
      Multiplier = 1.0
    End_Group
  End_Object

  Group = Mapping
    ProjectionName     = SimpleCylindrical
    CenterLongitude    = 0.0 <degrees>
    TargetName         = Venus
    EquatorialRadius   = 1737400.0 <meters>
    PolarRadius        = 1737400.0 <meters>
    LatitudeType       = Planetocentric
    LongitudeDirection = PositiveEast
    LongitudeDomain    = 180 <degrees>
    MinimumLatitude    = -90.0 <degrees>
    MaximumLatitude    = 90.0 <degrees>
    MinimumLongitude   = -180.0 <degrees>
    MaximumLongitude   = 180.0 <degrees>
    UpperLeftCornerX   = -5458203.0763469 <meters>
    UpperLeftCornerY   = 2729101.5381735 <meters>
    PixelResolution    = 83.285569402241 <meters>

    # PixelResolution    =  <meters/pixel>
    Scale              = 364.088888889 <pixels/degree>
  End_Group
End_Object

Object = Label
  Bytes = 65536
End_Object

Object = History
  Name      = IsisCube
  StartByte = 8590000129
  Bytes     = 1748
End_Object
End
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