Wednesday, April 13, 2005

Look out for big lone stars

As I was hinting in a previous entry, the flower constellations of Daniele Mortari could also be used to construct large "objects" in space in order for us to give signals to ETs. If you take a look at some of the constellations that can be built, it does not take much time to realize that these are made by intelligent people, with a sense of art at that. In this article, Luc Arnold proposes to find ET life by looking at large objects, let us hope there is another Daniele Mortari, several parsecs away who has made the same discovery.

There is a good reason as to why these figures would be better detected with interferometry systems. One of the interesting feature of these constellations is that the human brain looks at them and figures they have a shape because they see three of more satellites as if they are always be forming a line. This is mainly an averaging effect but it is striking (Daniele can produce a constellation that reproduces the contour of a star, imagine that, a star looking at a star!) Since interferometric systems do make an average view (they have to collect enough light), we are also likely to see these lines in the interferometric data. And the best way to find them, will be use the curvelet transform. Since interferometric systems are also sparse, in term of light collection, it is likely that we will have incomplete data, Emmanuel Candes who has been working on curvelets, is also now working on incomplete fourier ensembles and he is aware of interferometric systems as witnessed in his recent paper entitled "Stable Signal Recovery from Incomplete and Inaccurate Measurements"

...Fourier ensemble. Suppose now that A is obtained by selecting p rows from the n×n discrete Fourier transform and renormalizing the columns so that they are unitnormed. If the rows are selected at random, the condition for Theorem 1 holds with overwhelming probability for S  C · p/(log n)3 [4]. This case is of special interest as reconstructing a digital signal or image from incomplete Fourier data is an important inverse problem with applications in biomedical imaging (MRI and tomography), Astrophysics (interferometric imaging), and geophysical exploration.


It looks like, it is just a matter of time before we go out on a search for a big lone star, you know the five legged one...

No comments:

Printfriendly