Marsch, E.; Axford, W. I.; Ip, W.-H.; Thomas, N.; Schwenn, R.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T.; Ksanfomality, L. V.; Kogan, A. Y.: InterHelios-Sun and Mercury Observer. Physics and Chemistry of the Earth 22, pp. 469 - 479 (1997)
Marsch, E.; Tu, C.-Y.: The effects of high-frequency Alfvén waves on coronal heating and solar wind acceleration. Astronomy and Astrophysics 319, pp. L17 - L20 (1997)
Marsch, E.; Tu, C.-Y.: Intermittency, non-Gaussian statistics and fractal scaling of MHD fluctuations in the solar wind. Nonlinear Processes in Geophysics 4, pp. 101 - 124 (1997)
Tu, C.-Y.; Marsch, E.: Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfvén waves. Solar Physics 171, pp. 363 - 391 (1997)
Tu, C.-Y.; Marsch, E.; Ivory, K.; Schwenn, R.: Pressure enhancement associated with meridional flow in high-speed solar wind: Possible evidence for an interplanetary magnetic flux rope. Annales Geophysicae 15 (2), pp. 137 - 142 (1997)
Wilhelm, K.; Lemaire, P.; Curdt, W.; Schühle, U.; Marsch, E.; Poland, A. I.; Jordan, S. D.; Thomas, R. J.; Hassler, D. M.; Huber, M. C. E.et al.; Vial, J.-C.; Kühne, M.; Siegmund, O. H. W.; Gabriel, A.; Timothy, J. G.; Grewing, M.; Feldman, U.; Hollandt, J.; Brekke, P.: First results of the SUMER telescope and spectrometer-solar ultraviolet measurements of emitted radiation-on SOHO, I. Spectra and Spectroradiometry. Solar Physics 170, pp. 75 - 104 (1997)
Aellig, M. R.; Grünwaldt, H.; Hefti, S.; Wurz, P.; Bochsler, P.; Axford, W. I.; Balsiger, H.; Bürgi, A.; Coplan, M. A.; Galvin, A. B.et al.; Geiss, J.; Gliem, F.; Gloeckler, G.; Hilchenbach, M.; Hovestadt, D.; Hsieh, K. C.; Ipavich, F. M.; Judge, D. L.; Kallenbach, R.; Klecker, B.; Lee, M. A.; Livi, S.; Managadze, G. G.; Marsch, E.; Möbius, E.; Neugebauer, M.; Ogawa, H. S.; Reiche, K.-U.; Scholer, M.; Verigin, M. I.; Wilken, B.: Solar corona diagnostic with solar wind iron charge spectra. Helv. Phys. Acta 69, pp. 49 - 50 (1996)
Astudillo, H. F.; Livi, S.; Marsch, E.; Rosenbauer, H.: Evidence for nongyrotropic alpha particle and proton distribution functions: TAUS solar wind measurements. Journal Geophysical Research 101, pp. 24423 - 24432 (1996)
Marsch, E.; Tu, C.-Y.: Spatial evolution of the magnetic field spectral exponent in the solar wind: Helios and Ulysses comparison. Journal Geophysical Research 101, pp. 11149 - 11152 (1996)
Marsch, E.; Tu, C.-Y.; Rosenbauer, H.: Multifractal scaling of the kinetic energy flux in solar wind turbulence. Annales Geophysicae 14 (3), pp. 259 - 269 (1996)
Tu, C.-Y.; Marsch, E.; Rosenbauer, H.: An extended structure-function model and its application to the analysis of solar wind intermittency properties. Annales Geophysicae 14 (3), pp. 270 - 285 (1996)
Hovestadt, D.; Hilchenbach, M.; Bürgi, A.; Klecker, B.; Laeverenz, P.; Scholer, M.; Grünwaldt, H.; Axford, W. I.; Livi, S.; Marsch, E.et al.; Wilken, B.; Winterhoff, H. P.; Ipavich, F. M.; Bedini, P.; Coplan, M. A.; Galvin, A. B.; Gloeckler, G.; Bochsler, P.; Balsiger, H.; Fischer, J.; Geiss, J.; Kallenbach, R.; Wurz, P.; Reiche, K.-U.; Gliem, F.; Judge, D. L.; Ogawa, H. S.; Hsieh, K. C.; Möbius, E.; Lee, M. A.; Managadze, G. G.; Verigin, M. I.; Neugebauer, M.: CELIAS-Charge, element and isotope analysis system for SOHO. Solar Physics 162, pp. 441 - 481 (1995)
Liu, S.; Marsch, E.; Livi, S.; Woch, J.; Wilken, B.; von Steiger, R.; Gloeckler, G.: Radial gradients of ion densities and temperatures derived from SWICS/Ulysses observations. Geophysical Research Letters 22, pp. 2445 - 2448 (1995)
Marsch, E.; von Steiger, R.; Bochsler, P.: Element fractionation by diffusion in the solar chromosphere. Astronomy and Astrophysics 301, pp. 261 - 276 (1995)
Schmidt, J. M.; Marsch, E.: Spatial transport and spectral transfer of solar wind turbulence composed of Alfvén waves and convective structures I: The theoretical model. Annales Geophysicae 13 (5), pp. 459 - 474 (1995)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).