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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>Three-dimensional Positive Ion Analyser (JPA)</h1><p><strong>NSSDC ID:</strong> 1985-056A-05<br/><strong>Mission Name:</strong> Giotto<br/><strong>Principal Investigator:</strong> Dr. Alan D. Johnstone<br/></p><div class="twocol"><div class="urone"><h2>Description</h2><p>
          The objective of this investigation is to measure the plasma flow around Comet Halley in order to study (1) the mass loading of the solar wind by ions of cometary origin, (2) the existence, location, and strength of the upstream shock transition in the solar wind flow, (3) the position of and forces controlling the pressure balance surface between the cometary and the solar plasma, (4) the processes that form tail rays and other discrete visible features in the coma, and (5) the detection of wave motion induced by the cometary interaction that leads to the thermalization of solar wind and implanted ions. The instrument employs two sensors. One is a 270-deg spherical electrostatic energy analyzer (EEA) with a microchannel plate detector that measures the three-dimensional energy/charge distribution of positive ions from 10 eV to 20 keV over the polar angle range 20 - 180 deg with respect to the spin axis of the spacecraft. A complete set of measurements is obtained every spin period (4 s). The second sensor consists of a quadrispherical EEA with six time-of-flight analyzers set at different polar angles in the range 20 - 160 deg. The three-dimensional energy distribution of five major mass groups of ions up to 44 u over the energy range 0.1 - 70 keV is measured in 32 spin periods (128 s).
          </p></div><div class="urtwo"><h2>Alternate Names</h2><ul><li>JPA</li></ul><h2>Facts in Brief</h2><p><strong>Mass:</strong> 4.7 kg<br/><strong>Power (avg):</strong> 4.4 W<br/><strong>Bit rate (avg):</strong> 1.355 bps<br/></p><h2>Funding Agencies</h2><ul><li>Consiglio Nazionale delle Richerche, Italy (Italy)</li><li>Max-Planck-Institut (Federal Republic of Germany)</li></ul><h2>Discipline</h2><ul><li>Planetary Science: Small Bodies</li></ul><h2>Additional Information</h2><ul><li><a href="spacecraftDisplay.do?id=1985-056A">Giotto</a></li><li><a href="datasetSearch.do?spacecraft=Giotto&amp;experiment=Three-dimensional Positive Ion Analyser (JPA)">Data collections from this experiment</a></li></ul><h2/><p>
          Questions or comments about this experiment can be directed to:
          <a href="mailto:David.R.Williams@nasa.gov?Subject=NMC Comment/Question: Three-dimensional Positive Ion Analyser (JPA) (1985-056A-05)">Dr. David R. Williams</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>Dr. Helmut R. Rosenbauer</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Aeronomie</td><td>rosenbauer@linmpi.mpg.de</td></tr><tr class="odd"><td>Prof. Reimar Luest</td><td>Co-Investigator</td><td>European Space Agency</td><td> </td></tr><tr><td>Prof. Henri Reme</td><td>Co-Investigator</td><td>CNRS Centre d'Etudes Spatiale des Rayonments</td><td>henry.reme@cesr.fr</td></tr><tr class="odd"><td>Dr. Gerhard Haerendel</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Extraterrestrische Physik</td><td>hae@mpe.mpg.de</td></tr><tr><td>Dr. J. David Winningham</td><td>Co-Investigator</td><td>Southwest Research Institute</td><td>david@cluster.space.swri.edu</td></tr><tr class="odd"><td>Prof. Marino Dobrowolny</td><td>Co-Investigator</td><td>CNR, Space Plasma Laboratory</td><td>marino.dobrowolny@ifsi.rm.cnr.it</td></tr><tr><td>Prof. Ludwig F. B. Biermann</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Extraterrestrische Physik</td><td> </td></tr><tr class="odd"><td>Dr. Max K. Wallis</td><td>Co-Investigator</td><td>University College, Cardiff</td><td>mkw@nss.cs.ucl.ac.uk</td></tr><tr><td>Dr. William C. Feldman</td><td>Co-Investigator</td><td>Los Alamos National Laboratory</td><td>wfeldman@lanl.gov</td></tr><tr class="odd"><td>Mr. Denison R. Lepine</td><td>Co-Investigator</td><td>Rutherford Appleton Laboratory</td><td>c.lepine@rl.ac.uk</td></tr><tr><td>Dr. Wolfgang Studemann</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Aeronomie</td><td> </td></tr><tr class="odd"><td>Dr. Berend Wilken</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Aeronomie</td><td> </td></tr><tr><td>Dr. Vittorio Formisano</td><td>Co-Investigator</td><td>CNR, Space Plasma Laboratory</td><td>formisan@nike.ifsi.rm.cnr.it</td></tr><tr class="odd"><td>Dr. Alan D. Johnstone</td><td>General Contact</td><td>Mullard Space Science Laboratory</td><td> </td></tr><tr><td>Prof. Alberto Egidi</td><td>Co-Investigator</td><td>CNR, Space Plasma Laboratory</td><td>egidi@roma2.infn.it</td></tr><tr class="odd"><td>Dr. Goetz Paschmann</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Extraterrestrische Physik</td><td>gep@mpe.mpg.de</td></tr><tr><td>Dr. Klaus Jockers</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Aeronomie</td><td>jockers@linmpi.mpg.de</td></tr><tr class="odd"><td>Dr. Hermann Ulrich Schmidt</td><td>Co-Investigator</td><td>Max-Planck-Institut fur Physik und Astrophysik</td><td>schmidt@mpa-garching.mpg.de</td></tr><tr><td>Dr. Roberto Terenzi</td><td>Co-Investigator</td><td>CNR, Space Plasma Laboratory</td><td>roberto.terenzi@ifsi.rm.cnr.it</td></tr><tr class="odd"><td>Dr. P. Ricardo Cerulli</td><td>Co-Investigator</td><td>CNR, Space Plasma Laboratory</td><td>ricardo.cerulli@ifst.rm.cnr.it</td></tr><tr><td>Dr. Duncan A. Bryant</td><td>Co-Investigator</td><td>Rutherford Appleton Laboratory</td><td>dab@ac.rl.uk</td></tr></tbody></table><h2>Selected References</h2><p>Glassmeier, K.-H., <em>et al.</em>,
      Spectral characteristics of low-frequency plasma turbulence upstream of comet P/Halley,
      <em>J. Geophys. Res.</em>, 94, No. A1, 37-48, Jan. 1989.
      </p><p>Coates, A. J., <em>et al.</em>,
      Plasma parameters near the comet Halley bow shock,
      <em>J. Geophys. Res.</em>, 95, No. A12, 20701-20716, Dec. 1990.
      </p><p>Johnstone, A. D., <em>et al.</em>,
      The Giotto three-dimensional positive ion analyser,
      In--The Giotto Mission--Its Scientific Investigations, ESA SP-1077, edited by R. Reinhard and B. Battrick, pp. 15-32, Mar. 1986.
      </p><p>Huddleston, D. E., and A. D. Johnstone,
      Relationship between wave energy and free energy from pickup ions in the comet Halley environment,
      <em>J. Geophys. Res.</em>, 97, No. A8, 12217-12230, Aug. 1992.
      </p><p>Johnstone, A., <em>et al.</em>,
      Ion flow at comet Halley,
      <em>Nature</em>, 321, No. 6067, 344-346, May 1986.
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