Yes, entirely feasible if you kind of "fudge and pray" on the practical
realities. Even 10,000Jy is a tiny signal when cast in the context of a
small antenna (2-3dBi). 

But can the technical infrastructure be built with relatively-cheap
SDR-based kit, and Gnu Radio? Absolutely. 

On 2016-04-01 11:14, Dan McKenna wrote: 

> Marcus,
> 
> Thank you for your replies
> 
> Yes, No way with a dipole at a signal flux of 30J
> 
> In discussions with two of our faculty members I was told that
> the bursts can be 10,000 J and attempts to find an afterglow
> have not yielded certain results.
> 
> it is not known if any big antenna was really pointing at the burst such
> that the real gain of the antenna relative to the source position is known.
> 
> This project is looking for the Big Bursts 
> 
> Yes the V/UHF bands are very busy so the big key is the identification of 
> a burst that sweeps through the 10 Mhz bandwidth within certain criteria. 
> 
> The network would then be used to further process events using time of arrival
> as the second filter.
> 
> We would also like to make this work using two orthogonally polarized 
> antennas 
> 
> Does this seem more reasonable?
> 
> D.
> 
> The Lorimer burst was 30Jy peak, lasting only a few milliseconds. You 
> need instruments with *LARGE* effective apertures to "see" such an
> event, and I have doubts about the ability to use a mere ca 20 
> dipoles globally distributed to synthesize such an aperture. Most of the
> FRB events that have been logged are a *LOT* smaller than the Lorimer 
> event. Since those stations would likely not be phase-coherent,
> then any spectra adding would only improve sensitivity by 
> sqrt(N)--you don't get to effectively use the sum of the effective 
> apertures of
> the individual stations.
> 
> The CHIME observatory, currently entering early operations near 
> Penticton, BC, has FRBs as a secondary objective, and their antenna
> can hardly be described as "a dipole or two".
> 
> But, you're the astronomer, so perhaps there's something critical that 
> I've missed...
> 
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