The Edison infrared space observatory

For five years, theEdison program has had the goal of developing new designs for infrared space observatories which will break the cost curve by permitting more capable missions at lower cost. Most notably, this has produced a series of models for purely radiative and radiative/mechanical (hybrid) cooling which do not use cryogens and optical designs which are not constrained by the coolant tanks. Purely radiatively-cooled models achieve equilibrium temperatures as low as about 20 K at a distance of 1 AU from the sun. More advancedEdison designs include mechanical cooling systems attached to the telescope assembly which lower the optical system temperature to 5 K or less. Via these designs, near-cryogenic temperatures appear achievable without the limitations of cryogenic cooling. OneEdison model has been proposed to the European Space Agency as the next generation infrared space observatory and is presently under consideration as a candidate ESA Cornerstone mission. The basic design is also the starting point for elements of future infrared space interferometers.     

Elliptical Error Statistics for Radiolocation Analysis

A review is made of current techniques used in the statistical analysis of radio direction finding data which predict a region of probable transmitter location based upon a collection of intersecting lines of bearing measurements. This region has been conventionally defined by the elliptical error probability (EEP). Two characterizations for EEP are considered, and a technique is proposed for robust estimation of the elliptical region of probable location.     

Comments on "The GYROLITE: A New Generation Synchronous Satellite"

The effectiveness of the GYROLITE attitude stabilization is discussed on the basis of the basic mathematical equations in [1], and an avenue towards improved performance is indicated.     

Tracing the magnetic topology of coronal mass ejection events by Ulysses/HI-SCALE energetic particle observations in and out of the ecliptic

In January 2000, the Ulysses spacecraft observed an ICME event at 43° S heliographic latitude and ∼ 4.1 AU. We use electron (E _e>38 keV) observations to trace the topology of the IMF embedded within the ICME. The still controversial issue of whether ICMEs have been detached from the solar corona or are still magnetically anchored to it when they arrive at the spacecraft is tackled. An in ecliptic ICME event is also presented. This revised version was published online in August 2006 with corrections to the Cover Date.     

Shell type supernova remnants

The possibility of observing gamma ray emission from supernova remnants is discussed. It is shown that this could be possible in the 100 MeV band accessible to satellite instruments, but that confusion with the Galactic background is a major problem. At TeV energies and with modern imaging atmospheric cherenkov telescopes the situation should be much better and at least some of the nearby remnants may be detectable. Positive detections in both bands would provide a decisive test of current theoretical ideas on particle acceleration in supernova remnants and the origin of the Galactic cosmic rays.     

Application of the Concept of Referenced Radio Navigation

This paper discusses referenced radio navigation, the concept whereby monitoring stations at known locations are used to calibrate out systematic errors in a navigation system. This concept is implemented by broadcasting calibration data to the navigating user for application as real-time corrections to the position fixes made by the user's basic navigation equipment. A method is suggested for the automatic transmission and receiver processing of the correction data. Referenced radio navigation overcomes many of the shortcomings generally associated with long-distance navigation systems, and can increase accuracy and repeatability significantly. The concept is particularly applicable to global navigation systems such as OMEGA, in which propagation or synchronization errors can contribute substantially to the system error budget.     

Automatic target recognition using enhanced resolution SAR data

Using advanced technology, a new automatic target recognition (ATR) system has been developed that provides significantly improved target recognition performance compared with ATR systems that use conventional synthetic aperture radar (SAR) image-processing techniques. This significant improvement in target recognition performance is achieved by using a new superresolution image-processing technique that enhances SAR image resolution (and image quality) prior to performing target recognition. A computationally efficient two-level implementation of a template-based classifier is used to perform target recognition. The improvement in target recognition performance achieved using superresolution image processing in this new ATR system is quantified