[R-sig-Geo] spacetime : adding a fourth (spectral) dimension
scizmeli
sa.cizmeli at usherbrooke.ca
Wed May 4 00:30:52 CEST 2011
I am reflecting on a data structure that will allow us to perform all kinds
of spectral operations we normally do in remote sensing. Due to lack of an
appropriate data structure supporting spatially based spectral data, right
now we have to keep our data in non-georeferenced N-dimensional arrays. As
for extending spacetime, for now, I can think of an ability to:
* store in the same spacetime object both the spectral and the non-spectral
products (a spectral radiance image cube+computed image layers);
* easily subset ranges of wavelengths (hopefully both by wavelength and band
indexes) and be able to easily perform all kinds of space-time operations on
the subsets;
* select pixels and extract full (or partial) spectra
* easily plot different spectral images in lattice panels (with stplot?) for
a given time
* some channels are usually too noisy so we would need ability to flag some
unwanted channels at some pixels
* store spectral data for point and trajectory measurements
* incrementally import high volumes of data without having to load at once
all the data in memory. Size of spectral image times series can be very
large. On-disk storage can be sought with the use of netcdf technology for
extremely large databases.
and ability to easily implements methods like :
* band-ratio (or all kinds of other arithmetic) operations to compute new
image layers.
* computation of things like spectral derivatives, spectral unmixing as well
as classification algorithms that use spatial/spectral information together
etc.
* overlay ground truth data (ship trajectory/ground truth points/polygons)
onto image time series to match image pixels with ground truth data based on
spatial coordinates and time information (ship trajectories will coincide
with satellite images only at some given days)
* easily plot different spectra (graph of measurement wrt wavelenth) for a
given pixel in panels (or in the same graph) for different times (with
stplot?)
* spectrally interpolate images with a high spectral resolution to estimate
non-existing channels
There will certainly be dimensions other than "spectral" that people from
other disciplines will want to add in a spacetime object. So, to my mind, it
all boils down to the ability of adding custom dimensions into a spacetime
object (with numeric/string attributes addressable as in
st[pixel,time,wavelength,otherdimension]
If the upcoming versions of the spacetime package can be designed in such a
way, we could start implementing methods on spacetime objects for our tasks
in hand and the package would very fast become popular.
Are any these ideas feasible?
Servet
PS: I am definitely ready to help if you think this is a good direction to
go. I never created new object/methods myself but I am committed to learn
pretty fast if some initial directions are given.
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