Next generation GPS-aided space navigation systems

The next generation of low cost Global Positioning System (GPS) receivers for space navigation and attitude determination are positioned to take full advantage of the improvements made in the commercial GPS receivers used for terrestrial applications. There have been recent improvements made to the GPS receivers that include the addition of extra GPS satellite channels that can be tracked simultaneously. The older style GPS receivers were only able to handle five channels at a time. In order for proper determination of three-dimensional position, a minimum of four channels was required and the fifth channel of the receiver was reserved to perform search functions for finding the next satellite. This included searching for satellites that could be used to replace exiting satellites moving out of the Field of View (FOV). The search function also enables the GPS receiver to search for the best constellation for maximum performance accuracy. The fifth roaming channel also provided a best next-satellite selection capability in case the field of view to one of the satellites was blocked or shaded.     

Measurement of cosmic ray elemental composition from the CAKE balloon experiment

CAKE (Cosmic Abundances below Knee Energies) was a prototype balloon experiment for the determination of the charge spectra and abundances of the primary cosmic rays (CR) with Z > 10. It was a passive instrument made of layers of CR39® and Lexan®/Makrofol® nuclear track detectors; it had a geometric acceptance of ∼0.7 m² sr for Fe nuclei. Here, the scanning and analysis strategies, the algorithms used for the off-line filtering and for the tracking in automated mode of the primary cosmic rays are presented, together with the resulting CR charge distribution and their abundances.