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Weitersagen:


Herausgeber: 
  • J. G. Robertson
  • W. J. Tango
  • Very High Angular Resolution Imaging: Proceedings of the 158th Symposium of the International Astronomical Union, held at the Women's College, Univers 
     

    (Buch)
    Dieser Artikel gilt, aufgrund seiner Grösse, beim Versand als 3 Artikel!


    Übersicht

    Auf mobile öffnen
     
    Lieferstatus:   i.d.R. innert 7-14 Tagen versandfertig
    Veröffentlichung:  Dezember 1993  
    Genre:  Naturwissensch., Medizin, Technik 
     
    Algorithms / Astronomische Beobachtung# Observatorien, Ausrüstungen und Methoden / astronomy / Instruments / interferometry / Observatory / optical interferometry / radio astronomy
    ISBN:  9780792326328 
    EAN-Code: 
    9780792326328 
    Verlag:  Springer Netherlands 
    Einband:  Gebunden  
    Sprache:  English  
    Dimensionen:  H 241 mm / B 160 mm / D 33 mm 
    Gewicht:  945 gr 
    Seiten:  524 
    Bewertung: Titel bewerten / Meinung schreiben
    Inhalt:
    The 1990s are proving to be a very exciting p&iod for high angular resolution astronomy. At radio wavelengths a combination of new array instruments and pow? erful imaging algorithms have generated images of unprecedented resolution and quality. In the optical and infrared, the great technical difficulties associated with constructing separated-aperture interferometers have been largely overcome, and many new instruments are now operating or are being developed. As these pro? grams start to produce observational results they will be able to draw extensively on the experience gained by the radio-interferometry community. Thus it seemed that the time was ripe for a meeting which would bring together workers from all wavelength ranges to discuss the details of the science and art of "Very High Angular Resolution Imaging" . While the main emphasis of Symposium No. 158 was on high resolution tech? niques from the radio, mm-wave, infrared and optical bands, it also provided an opportunity for presentation of astronomical results from these techniques. As well as giving our colleagues from the Northern Hemisphere a break from midwinter, the location of the Symposium in Australia recognised the continuing development of astronomical interferometry in this country, especially the recent completion of the Australia Telescope radio array, and the progress toward com? missioning of the Sydney University Stellar Interferometer. A number of the par? ticipants visited these instruments during the post-symposium tour.

      



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