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Submission addresses

All article submissions, the peer-review process and production (from acceptance to publication) are handled by the Editorial Office in China; all enquiries should be directed to them at the address below.

Plasma Science and Technology
Editorial Office
Institute of Plasma Physics
Chinese Academy of Sciences
PO Box 1126
Hefei 230031
People's Republic of China
Tel: +86 551 5591617, 5591388
Fax: +86 551 5591310
Email: pst@ipp.ac.cn

  1. Reconnaissance of Suspected Old Novae

    Jeff W. Robertson et al. 2000 The Astronomical Journal 119 1365

  2. Bayesian group analysis of plasma-enhanced chemical vapour deposition data

    R Fischer 2004 New J. Phys. 6 25

  3. The Recent Star Formation History of GR 8 from Hubble Space Telescope Photometry of the Resolved Stars

    Robbie C. Dohm-Palmer et al. 1998 The Astronomical Journal 116 1227

  4. A measure of centrality based on network efficiency

    V Latora and M Marchiori 2007 New J. Phys. 9 188

  5. The First MOTESS-GNAT Variable-Star Survey

    Adam L. Kraus et al. 2007 The Astronomical Journal 134 1488

  6. An analytical treatment of single station triaxial seismic direction finding

    S Greenhalgh et al 2005 J. Geophys. Eng. 2 8

  7. Directed network modules

    Gergely Palla et al 2007 New J. Phys. 9 186

  8. Changes in Pluto's Atmosphere: 1988-2006

    J. L. Elliot et al. 2007 The Astronomical Journal 134 1

  9. Using the Galactic Dynamics of M7 Dwarfs to Infer the Evolution of Their Magnetic Activity

    Andrew A. West et al. 2006 The Astronomical Journal 132 2507

  10. Weak nonlinearities: a new route to optical quantum computation

    W J Munro et al 2005 New J. Phys. 7 137

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