There is also an FTP server , with contents: Various AIPS tasks and support routines for the processing of Australia Telescope data; Observing proposals and documentation related to the use and operation of the Australia Telescope, including vistors guides to all the ATNF sites; The Karma package (library and applications for Signal and Image Processing; A spectral line reduction package which can read a number of formats including those used by the Parkes 64m telescope; Another spectral line reduction package specifically for the reduction of spectral line data from the Parkes 64m telescope; - README
A CFHT page at CADC has information about the CFHT archive, CCDs, proposal template and manuals.
Rein H. Warmels, Karl-Schwarzschild-Strasse 2, D 85748 Garching bei Muenchen Email: firstname.lastname@example.orgIn particular, authors of ESO-MIDAS application software that would be of general interest for the ESO-MIDAS community, are invited to make this software available.
If you want to receive future issues of the Courier, please contact the editor. More updated information about ES0-MIDAS can be obtained from the ESO-MIDAS Bulletin Board , which is also accessible via the USEnet News facility.
The list is posted on regular basis to the USENET newsgroup sci.physics.computational.fluid-dynamics.
The topics covered include linear and non-linear plasma physics, waves and radiation phenomena in plasma, waves in random media and turbulence, planetary, solar and stellar coronal plasma, plasma under extreme conditions in space, space plasma radio emission, radio methods for investigating space plasma environments, and the use of the Earth's ionosphere and magnetosphere as a space plasma laboratory for model experiments simulating phenomena in other plasma environments
The presentation will be in the form of lectures, tutorial talks, student oral papers, and poster papers.
The Haverah Park group studies high energy cosmic rays by various techniques.
The Whipple group is attempting to detect gamma rays with energies > 1TeV using air-Cherenkov detectors.