Date: Thu, 14 Sep 2023 15:41:53 +0000
Dear Alfredo,
I'm having the below problem when plotting the data after upgrading to the new Flair and Fluka. This wasn't an issue on the previous version. I'm using Ubuntu and Debian WSL systems. Thanks for any solution on how to fix this.
[cid:image001.png_at_01D9E72A.533364A0]
Best regards,
Sanjeev Faruk
Health Physicist
Laser Safety Officer (LSO)
T: +44 (0)1235 778875
M: +44 (0) 7824 519 159
E: sanjeev.faruk_at_diamond.ac.uk
-----Original Message-----
From: owner-fluka-discuss_at_mi.infn.it <owner-fluka-discuss_at_mi.infn.it> On Behalf Of alfredo.ferrari_at_mi.infn.it
Sent: Wednesday, September 13, 2023 8:02 PM
To: Petr Martynenko <martynenkopetr91_at_gmail.com>
Cc: fluka-discuss_at_fluka.org
Subject: RE: [fluka-discuss]: New Fluka major eelease, fluka2023.3.0
Fixed! Try now...
> Dear alfredo.ferrari_at_mi.infn.it<mailto:alfredo.ferrari_at_mi.infn.it> ;
> I haven't accesses to
> fluka2023.3-linux-gfor64bit-13.2-glibc2.37-AA.tar.gz gfortran 13.2,
> glibc2.37
> on the official FLUKA web site (https://eur03.safelinks.protection.outlook.com/?url=http%3A%2F%2Fwww.fluka.org%2F&data=05%7C01%7Csanjeev.faruk%40diamond.ac.uk%7C472a7c98d04d46a5467f08dbb490d0ca%7C9d27ba7401004d0d81ff1d728dae8df6%7C0%7C0%7C638302306331389678%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=mqnwaxgXACDxNNkdIsrcrQCytvkhahG5TkTWrZxPUuE%3D&reserved=0<http://www.fluka.org/>).
> What's about this?
>
> Thanks all Fluka team for the new release fluka-2023.3-0.
> Отправлено из приложения "Почта" для Windows
>
> От: alfredo.ferrari_at_mi.infn.it<mailto:alfredo.ferrari_at_mi.infn.it>
> Отправлено: 13 сентября 2023 г. в 18:31
> Кому: fluka-discuss_at_fluka.org<mailto:fluka-discuss_at_fluka.org>
> Тема: [fluka-discuss]: New Fluka major eelease, fluka2023.3.0
>
>
> Dear FLUKA users,
>
> Fluka2023.3.0, a major iteration of the 4th generation of the FLUKA
> code, is now available on the official FLUKA web site
> (https://eur03.safelinks.protection.outlook.com/?url=http%3A%2F%2Fwww.fluka.org%2F&data=05%7C01%7Csanjeev.faruk%40diamond.ac.uk%7C472a7c98d04d46a5467f08dbb490d0ca%7C9d27ba7401004d0d81ff1d728dae8df6%7C0%7C0%7C638302306331389678%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=mqnwaxgXACDxNNkdIsrcrQCytvkhahG5TkTWrZxPUuE%3D&reserved=0<http://www.fluka.org/>).
>
> This release represents a big step forward for FLUKA, it contains
> several important new features and changes.
>
> In the following a short list of the main new features:
>
> - Photonuclear interactions: both cross sections and models are
> completely new above ~100 MeV: this is a major improvement which
> gets
> rid of many limitations and inaccuracies of the the previous
> implementation (see the release notes for more details);
> - Photon cross section: upgraded from EPDL97 to EPICS2017;
> - Photon cross sections and bremsstrahlung cross sections are now
> extended up
> to 1.E21 eV;
> - GDR photonuclear cross sections have been updated for a few
> isotopes,
> in particular Lead ones;
> - Ortho-Positronium three-gamma annihilation is now included,
> including
> the 3-body matrix-element for the decay;
> - The hadronisation model of the high energy generator has been fully
> reworked
> in order to better account for experimental data which somewhat
> contradict
> widely accepted assumptions about string fragmentation;
> - All hadron-nucleus cross sections are new and extended up to 10^20
> eV,
> and all of them are now consistently calculated with Peanut: they
> have
> been validated up to the highest cosmic ray data;
> - Coherent elastic scattering of neutrons between 20 and 40 MeV is now
> treated using ad-hoc Legendre expansions;
> - Updated galactic cosmic ray spectra, now based on AMS02 data (thanks
> to Nicola Mazziotta and Pedro de la Torre Luque) are now available:
> they can be activated by new option in SPECSOUR : sdum = GCR-AMS;
> - Built-in source routines for neutron spectra from Am-Be, Am-B,
> 252-Cf
> sources are now available (see the BEAM card);
> - Internal conversion decays (IC) are now modeled as such and no
> longer
> as (wrongly) gamma emission, including the explicit transport of the
> excited nuclei to the decay point;
> - The charged particle stopping power in water is now defined in
> agreement
> with the ICRU90 recommendations. In particular, but not only, the
> water
> average ionization potential is now set to I=78 eV;
> - The sampling of the example solar flare spectra has been
> definitively
> corrected;
> - The default DPMJET is now the newest one, 3.19.3.x, the previous
> version
> is no longer distributed;
> - By default intranuclear cascade reinteractions in Dpmjet are now
> treated
> by the FLUKA hadronic models;
> - The sets of fluence-to-dose conversion coefficients from ICRP116 are
> now
> available, in particular ambient dose has been added;
> - A new interface to Ultra High Energy Cosmic Ray generators is now
> available: at present it supports interfacing to EPOS and Sibyll.
> For
> a rationale of this interface, and on how to use it, please refer to
> the release notes;
> - Dose averaged LET maps are now implemented on-line (generalized
> particle
> DOSAVLET);
> - Corresponding neutron group-wise cross sections no longer needed if
> point-wise one are requested for a given material;
> - The source code has been deeply reorganised. Among others, the old
> high
> energy interaction model (eventv/eventvmvax) has been removed, since
> it
> is no longer used by any of the interaction routines.
>
> At the same time a new bug fixing version of flair, python3 version
> only#, is also available on the web site. Those new python3
> compatible files are called flair...2.3-0dpy3..., see
> https://eur03.safelinks.protection.outlook.com/?url=http%3A%2F%2Fwww.f<http://www.f/>
> luka.org%2Fflair%2Fdownload.html&data=05%7C01%7Csanjeev.faruk%40diamon
> d.ac.uk%7C472a7c98d04d46a5467f08dbb490d0ca%7C9d27ba7401004d0d81ff1d728
> dae8df6%7C0%7C0%7C638302306331389678%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiM
> C4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C
> %7C&sdata=2ON0zKvI8E%2FeT9mrEZdo9Z1e4HHb%2BGdJLzJqWd%2BUdTw%3D&reserve
> d=0,
> let us know if there are problems.
>
> Due to the amount of changes/additions, and despite the extensive
> testing carried out by the FLUKA collaboration members, rare bugs
> cannot be excluded. If you experience a crash, or you feel something
> is incorrect when running fluka2023.3, please report the issue at
> fluka-discuss_at_fluka.org<mailto:fluka-discuss_at_fluka.org>.
>
> All users are urged to update to this release. As usual, assistance
> will be provided only for the latest release/respin.
>
> The FLUKA developers
>
> # The python2 version of Flair is frozen and no effort will be made to
> fix still existing problems. If possible, migrate to the python3
> version
>
>
> Available FLUKA files:
>
> fluka2023.3-data.tar.gz data files required by all
> versions
> (changed wrt previous
> releases!!)
>
> Linux:
>
> fluka-2023.3-0.i686.rpm rpm 32/64bit g77
> fluka-2023.3-0.x86_64.rpm rpm gfortran 13.2,
> glibc2.37
> fluka2023.3-linuxAA.tar.gz 32/64bit g77
> fluka2023.3-linux-gfor64bit-9.4-glibc2.17-AA.tar.gz gfortran 9.4,
> glibc2.17
> fluka2023.3-linux-gfor64bit-10.3-glibc2.32-AA.tar.gz gfortran 10.3,
> glibc2.32
> fluka2023.3-linux-gfor64bit-11.4-glibc2.35-AA.tar.gz gfortran 11.4,
> glibc2.35
> fluka2023.3-linux-gfor64bit-12.3-glibc2.36-AA.tar.gz gfortran 12.3,
> glibc2.36
> fluka2023.3-linux-gfor64bit-13.2-glibc2.37-AA.tar.gz gfortran 13.2,
> glibc2.37
>
> MAC arm64
>
> fluka2023.3-macarm-gfor64bit-12.3-AA.tar.gz gfortran 12.3
>
> MAC intel
>
> fluka2023.3-mac-gfor64bit-11.3-AA.tar.gz gfortran 11.3
> fluka2023.3-mac-gfor64bit-12.2-AA.tar.gz gfortran 12.2
>
>
>
>
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