wsjtx 2.7.0~rc3+repack-1build2 source package in Ubuntu

Changelog

wsjtx (2.7.0~rc3+repack-1build2) noble; urgency=medium

  * No-change rebuild for CVE-2024-3094

 -- William Grant <email address hidden>  Mon, 01 Apr 2024 19:36:20 +1100

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Uploaded by:
William Grant
Uploaded to:
Noble
Original maintainer:
Ubuntu Developers
Architectures:
linux-any all
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Noble release universe misc

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File Size SHA-256 Checksum
wsjtx_2.7.0~rc3+repack.orig.tar.xz 13.6 MiB 107ff97544cfcdadde7759e061a65db130421bf71217ba4ea9d53801e3fa4901
wsjtx_2.7.0~rc3+repack-1build2.debian.tar.xz 18.7 KiB 70efe07ed1a9676bd5c82145d78b084f30a15bc2dc2334a4554b93640cda3482
wsjtx_2.7.0~rc3+repack-1build2.dsc 2.5 KiB 4e2780e6343b8ad296b90269935d8922c5fd2f874b6767b04e2cda6ef9299110

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Binary packages built by this source

wsjtx: Weak-signal amateur radio communications

 WSJT-X implements amateur radio communication protocols or "modes" called
 FST4, FST4W, FT4, FT8, JT4, JT9, JT65, Q65, MSK144, and WSPR, as well as one
 called Echo for detecting and measuring your own radio signals reflected from
 the Moon. These modes were all designed for making reliable, confirmed QSOs
 under extreme weak-signal conditions.
 .
 JT4, JT9, and JT65 use nearly identical message structure and source encoding
 (the efficient compression of standard messages used for minimal QSOs). They
 use timed 60-second T/R sequences synchronized with UTC. JT4 and JT65 were
 designed for EME ("moonbounce") on the VHF/UHF/microwave bands. JT9 is
 optimized for the MF, and HF bands. It is about 2 dB more sensitive than
 JT65 while using less than 10% of the bandwidth. Q65 offers submodes with a
 wide range of T/R sequence lengths and tone spacings.
 .
 FT4 and FT8 are operationally similar but use T/R cycles only 7.5 and 15 s
 long, respectively. MSK144 is designed for Meteor Scatter on the VHF bands.
 These modes offer enhanced message formats with support for nonstandard
 callsigns and some popular contests.
 .
 FST4 and FST4W are designed particularly for the LF and MF bands. On these
 bands their fundamental sensitivities are better than other WSJT-X modes with
 the same sequence lengths, approaching the theoretical limits for their rates
 of information throughput. FST4 is optimized for two-way QSOs, while FST4W is
 for quasi-beacon transmissions of WSPR-style messages. FST4 and FST4W do not
 require the strict, independent time synchronization and phase locking of
 modes like EbNaut.
 .
 WSPR mode implements a protocol designed for probing potential propagation
 paths with low-power transmissions. WSPR is fully implemented within WSJT-X,
 including programmable "band-hopping".

wsjtx-data: Weak-signal amateur radio communications (data files)

 WSJT-X implements amateur radio communication protocols or "modes" called FT4,
 FT8, JT4, JT9, JT65, QRA64, ISCAT, MSK144, and WSPR, as well as one called
 Echo for detecting and measuring your own radio signals reflected from the
 Moon. These modes were all designed for making reliable, confirmed QSOs under
 extreme weak-signal conditions.
 .
 This package contains architecture-independent data files.

wsjtx-dbgsym: debug symbols for wsjtx
wsjtx-doc: Documentation and examples for the WSJT-X package

 WSJT-X implements amateur radio communication protocols or "modes" called FT4,
 FT8, JT4, JT9, JT65, QRA64, ISCAT, MSK144, and WSPR, as well as one called
 Echo for detecting and measuring your own radio signals reflected from the
 Moon. These modes were all designed for making reliable, confirmed QSOs under
 extreme weak-signal conditions.
 .
 This package provides the software documentation.