SETI - Search for Extra-Terrestrial Intelligence -- AstroPulse
The project listens for broad-band, short-time pulses that might represent
extraterrestial intelligence, or other phenomena such as rapidly rotating
pulsars or exploding primordial black holes.
The port automatically optimizes for the host CPU using the CPUTYPE
variable in /etc/make.conf
SETI - Search for Extra-Terrestrial Intelligence -- Version 7
Use your unused CPU cycles to aid in computations analyzing radio
telescope information for possible signs of extra-terrestrial intelligence.
The port automatically optimizes for the host CPU using the CPUTYPE
variable in /etc/make.conf
A tool to "stamp" photos taken with digital camera with a location, where they
were taken. It uses the GPS coordinates saved in GPX format.
GpsDrive is a car (bike, ship, plane) GPS navigation system.
GpsDrive displays the position provided from a NMEA-capable GPS receiver on
a zoomable map. The map file is autoselected depending on the position and
preferred scale. Speech output is supported if the "festival" software is
running. Waypoint database is supported via MySQL (optional).
Xphoon sets X the root window to a picture of the moon in its current phase.
The GPSTk is an open source C++ library for developing GPS applications.
The GPSTk suite consists of a core library, auxiliary libraries, and a set
of applications. The GPSTk provides a wide array of functions that solve
processing problems associated with GNSS such as processing or using
standard formats such as RINEX. The libraries are the basis for the more
advanced applications distributed as part of the GPSTk suite.
jday and j2d are command line utilities to convert calendar dates
to astronomical julian dates, and julian dates to calendar dates.
There is a corresponding library libjday.a which can be used for
the same functionality within applications.
libnova is a general purpose, double precision, astronomical calculation
library. The intended audience of libnova is C / C++ programmers, astronomers
and anyone else interested in calculating positions of astronomical objects.
This is a trivial program that displays the phase of the moon. It
may help when you play a game that depends on the phase of the moon
(nethack, nlith, etc.).
It can also be used to calculate her...um, you figure this one out. ;)
This program is designed to match up items in two different lists, which may
have two different systems of coordinates. The program allows the two sets of
coordinates to be related by a linear, quadratic, or cubic transformation.
There was a major change in version 0.15: the first stage uses the clever method
of finding the most likely triangles described in Tabur, Publications of the
Astronomical Society of Australia, vol 24 , page 189 (2007). This replaces the
more brute-force-ish method of Valdes et al., Publications of the Astronomical
Society of the Pacific, vol 107, page 1119 (1995), which was employed in version
up to 0.14.
The program was designed and written to work on lists of stars and other
astronomical objects, but it might be applied to other types of data. In order
to match two lists of N points, the main algorithm calls for O(N^6) operations
(yes, that's N-to-the-sixth), so it's not the most efficient choice. I find
myself becoming impatient for N >= 100, but your mileage may vary. On the other
hand, it does allow for arbitrary translation, rotation, and scaling...