Cossorscope 2000

Cossor, A.C.; London

  • Année
  • 1962 ?
  • Catégorie
  • Appareils de mesure et de dépannage (matériel de labo)
  • Radiomuseum.org ID
  • 330140

 Spécifications techniques

  • No. de tubes
  • 34
  • Lampes / Tubes
  • Gammes d'ondes
  • Bandes en notes
  • Tension / type courant
  • Alimentation Courant Alternatif (CA) / 90-240 Volt
  • Haut-parleur
  • - - Pas de sortie basse fréquence
  • Matière
  • Boitier métallique
  • De Radiomuseum.org
  • Modèle: Cossorscope 2000 - Cossor, A.C.; London
  • Forme
  • Modèle de table générique
  • Dimensions (LHP)
  • 11 x 15 x 17 inch / 279 x 381 x 432 mm
  • Remarques
  • COSSORSCOPE, Model 2000

    Models 2000 and 2100 are compact versatile oscilloscopes for general-purpose measurements.
    Physically, the two instruments are almost identical and the circuitry for each Model is very similar.
    Both Models employ a modern double-gun CRT which provides a brilliant display with excellent definition. The CRT for Model 2100, however, is fitted with a spiral post-deflexion anode and is operated at a higher voltage so that faster writing speeds can be attained than with Mode! 2000.

    Specifications:

    Cathode-Ray Tube 4 in. (10 cm) double-gun tube with green fluorescence, operating at 1·5 kV.
    Y1/Y2 Amplifier Frequency response DC to 5 MHz
      Rise-time 70 mµsec
      Sensitivity calibrated 100 mV/cm to 100 V/cm, in steps of 1, 3 and 10
      Input Attenuator impedance 1 MΩ, 30 pF
    Y Pre Amp (2) Sensitivity. 1 mV/cm, bandwidth 10 Hz to 200 kHz, & 10 mV/cm
      Input impedance l MQ.
    Time-Base 21 calibrated ranges from 3 sec/cm to 1µsec/cm.
      Sweep expansion X 10.
    Trigger Four modes of operation, Auto, Slow, Fast and TV Frame. Positive or negative from 50 Hz, internai or external.

     

  • Poids net
  • 34.5 lb (34 lb 8 oz) / 15.663 kg
  • Littérature
  • - - Manufacturers Literature (Manual For Cossorscopes Model 2000 & Model 2100)
  • Auteur
  • Modèle crée par Gary Cowans. Voir les propositions de modification pour les contributeurs supplémentaires.

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