Search Results for "map it"

PreviSat is a satellite tracking software for observing purposes. Very easy to use, it shows positions of artificial satellites in real-time or manual mode. PreviSat is able to make predictions of their passes, predictions of MetOp and COSMO-SkyMed flares, transits of all satellites, predictions of Starlink satellites passes and several other calculations.

...This software consists from C++/Qt programs such as dotScope (https://dotscope.sourceforge.io) - is a scientific shell for live experiment, dlCAM (https://dlcam.sourceforge.io) - computer aided manufacture for Arduino and others projects, img-map (https://img-map.sourceforge.io) - image digitaizer.

...More exactly -displaying them in ways that hopefully will allow you to explore and better understand your vector data. The basic idea is simple, take a vector defined in one of a few different types of data formats and map it on the screen. Add another vector and you start to form a 'route'. Each route or position vector can be accompanied with a 'force' vector. This can be used to show something acting on a position with direction and magnitude. Finally you can give each position a tag to display on screen. This could be a common math symbol or greek letter, start/end signposts, or a number of the position either from the begining or after a reset. ...

Construct2D is a grid generator designed to create 2D grids for CFD computations on airfoils. The grids are generated in Plot3D format. The only required input file is the set of coordinates defining the airfoil geometry, using the same format as XFoil, the popular vortex-panel code for airfoil analysis. Construct2D can create grids with O topology (recommended for airfoils with a blunt trailing edge) or C topology (recommended for airfoils with a sharp trailing edge). Now available in...

Data evaluation tool for the magnetism reflectometer at the spallation neutron source (BL-4A@SNS). Reads raw nexus files (HDF5) of histogrammed or event mode data to create reflectivity curves and 2D Q-maps.

...The calculations of the interference profile are performed taking into account the experimental conditions: excitation light incidence angle, wavelength range, luminescent centers distribution. An excitation field depth distribution map (*.bmp), normally calculated by the IMD software (D.L. Windt) is required for the calculations. The module is presented both as LabVIEW virtual instrument and executable requiring LabVIEW runtime (http://joule.ni.com/nidu/cds/view/p/id/2534/lang/en). It may be useful for physicists and material scientists working on the luminescence of thin films.