From: Giuseppe Battistoni (Giuseppe.Battistoni@mi.infn.it)
Date: Thu Jan 31 2008 - 10:54:52 CET
we hope that using the last FLUKA respin your problem is definitively
fixed, and we thank you for having pointed out that hidden bug.
In addition to this I wish to recommend 2 other issues for your
a) in addition to yout EMF-CUT cards with blank SDUM to control transport
cutoff of e+,e-,gamma, you should also introduce EMF-CUT cards with
SDUM=PROD-CUT, in order to take full control of production thresholds.
b) it has been tested (Paola Sala) that if you take away the STEPSIZE
cards and set the first 3 WHAT of the magnetic field card
MGFIELD to values that we have used before for atmospheric shower
simulations ( MGFIELD 20. 100. 30. ..... ), then the messages in the logs
concerning problems in precision will disappear. This should speed up a
little your problem.
On Fri, 30 Nov 2007, John Clem wrote:
> While attempting to characterize VHE gamma ray showers in the atmosphere, we
> ran into the below problem that occured for every other primary. For this
> case the primary energies are fixed at 20TeV.
> "Subscript out of range on file line 357, procedure kaskad.f/kaskad.Attempt
> to access the 5501-th element of variable agesec.equests:"
> It became less frequent after maximizing our energy thresholds, however any
> thing above these levels would shroud our analysis goals. Incrementing the
> dimensions would seem like the next obvious step. Lack of access to this
> part of the code prevents such a test. Any suggestions ??
> Thanks, John
> > John Clem
> > Research Associate Professor
> > Bartol Research Institute
> > Department of Physics and Astronomy
> > University of Delaware
> > Newark, DE 19716 USA
> > 302-831-4354
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