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<div id="contentwrapper"><div id="rightcontent"><div id="headimage"><img height="100" width="530" alt="National Space Science Data Center Header" src="/logo/nssdc_header.jpg"/></div><h1>Position Sensitive Proportional Counter (PSPC)</h1><p><strong>NSSDC ID:</strong> 1990-049A-02<br/><strong>Mission Name:</strong> ROSAT<br/><strong>Principal Investigator:</strong> Prof. Joachim Truemper<br/></p><div class="twocol"><div class="urone"><h2>Description</h2><p>
          The position sensitive proportional counter (PSPC) was a thin-window gas counter. Incoming photons were absorbed, producing an electron cloud proportional to the photon energy. The electron cloud drifted to the anode wire grid where a high voltage was applied. In the high electric field, close to the wires, gas amplification of about 50,000 took place producing a charge signal at the anode wires which was proportional to the energy of the incoming photons. Simultaneous charge signals were induced in two cathode wire grids close to the anode. These signals were used to obtain the position of the photons with an accuracy of about 120 micrometers. A rotating filter wheel, in front of each PSPC, allowed the selection of reduced photon energy bands. In one position, the filter wheel was utilized as a vacuum door containing three radioactive sources for calibration.
          </p></div><div class="urtwo"><h2>Alternate Names</h2><ul><li>PSPC</li></ul><h2>Funding Agency</h2><ul><li>Max-Planck-Institut (Federal Republic of Germany)</li></ul><h2>Discipline</h2><ul><li>Astronomy: X-Ray</li></ul><h2>Additional Information</h2><ul><li><a href="spacecraftDisplay.do?id=1990-049A">ROSAT</a></li><li><a href="datasetSearch.do?spacecraft=ROSAT&amp;experiment=Position Sensitive Proportional Counter (PSPC)">Data collections from this experiment</a></li></ul><h2/><p>
          Questions or comments about this experiment can be directed to:
          <a href="mailto:nssdc-request@lists.nasa.gov?Subject=NMC Comment/Question: Position Sensitive Proportional Counter (PSPC) (1990-049A-02)">Coordinated Request and User Support Office</a>.
          </p></div></div><div class="clear"> </div><h2>Personnel</h2><table cellspacing="0" class="datatab"><thead><tr><th>Name</th><th>Role</th><th>Original Affiliation</th><th>E-mail</th></tr></thead><tbody><tr><td>Prof. Joachim Truemper</td><td>Principal Investigator</td><td>Max-Planck-Institut fur Extraterrestrische Physik</td><td>jtrumper@mpe.mpg.de</td></tr><tr class="odd"><td>Dr. Horst Hippmann</td><td>Other Investigator</td><td>Max-Planck-Institut fur Extraterrestrische Physik</td><td>hippmann@mpg.mpe.de</td></tr></tbody></table><h2>Selected References</h2><p>Snowden, S. L., <em>et al.</em>,
      ROSAT detection of an X-ray shadow in the 1/4-keV diffuse background in the Draco nebula,
      <em>Science</em>, 252, No. 5012, 1529-1532, June 1991.
      </p><p>Burrows, D. N., and J. A. Mendenhall,
      Soft X-ray shadowing by the Draco cloud,
      <em>Nature</em>, 351, No. 6328, 629-631, June 1991.
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        <li>NASA Official: <a href="mailto:Edwin.J.Grayzeck@nasa.gov">Dr. Ed Grayzeck</a></li>
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