Science Team
The Solar Obiter magnetometer science team has expertise in a broad range of scientific topics directly relevant to the magnetic field on the Sun and in interplanetary space, as well as its effects on the Earth and near-Earth space.
Team
UK science team members
- Prof. David Burgess (Queen Mary, University of London): Simulations of wave-particle interactions
- Prof. Peter Cargill (Imperial College London): Coronal loops and flares
- Dr Jonathan Eastwood (Imperial College London): Reconnection and space weather
- Dr Robert Forsyth (Imperial College London): ICMEs
- Dr Lyndsay Fletcher (Glasgow University): Solar flares
- Prof. Mike Lockwood, FRS (University of Reading): Long term changes in the solar magnetic field, links to climate
- Dr Mathew Owens (University of Reading): Coronal mass ejections and the solar magnetic cycle
- Dr Valery Nakariakov (University of Warwick): Coronal waves
- Prof. Robert Walsh (University of Central Lancashire): Coronal heating and waves
International science team members
- Dr Stuart Bale (University of California at Berkeley): Plasma kinetics and wave-particle interactions; WAVES Co-PI
- Prof. Wolfgang Baumjohann (Space Research Institute, Graz): Space plasmas
- Dr Bruno Bavassano (INAF-IFSI, Rome): Solar wind turbulence
- Dr Vincenzo Carbone (Università della Calabria): Solar wind turbulence
- Dr Nancy Crooker (Boston University): Topology of ICMEs and their connectivity to the Sun
- Dr Geza Erdös (KFKI, Hungary): Solar wind structures, waves and turbulence
- Dr Joe Giacalone (Lunar and Planetary Laboratory, U. Arizona): Particle acceleration and propagation
- Prof. Karl-Heinz Glassmeier (Technical University of Braunschweig): Solar wind waves and turbulence
- Dr Melvyn Goldstein (Goddard Space Flight Center): Waves and turbulence in the solar wind
- Dr Todd Hoeksema (Stanford University): Solar magnetic fields and their links into space
- Dr Werner Magnes (Space Research Institute, Graz): Space instrumentation
- Dr Milan Maksimovic (Observatoire de Paris): Wave-particle interactions;WAVES PI
- Prof. Eckart Marsch (MPI, Lindau): Plasma turbulence and coronal heating
- Prof. William Matthaeus (Bartol, University of Delaware): Solar wind turbulence
- Dr Javier R.-Pacheco (Universidad de Alcala, Madrid): Energetic particles; EPD PI
- Dr Neil Murphy (NASA JPL): Large scale heliospheric magnetic field structure
- Dr Jean-Louis Pincon (CNRS, Orleans): plasma waves and analysis techniques
- Dr Ingo Richter (Space Research Institute, Graz): Space instrumentation
- Dr Peter Riley (SAIC, San Diego): 3D modelling of ICMEs and other solar wind structures from the corona into interplanetary space
- Prof. Christopher Russell (University of California at Los Angeles): ICMEs and other solar wind structures
- Prof. Steve Schwartz (U Colorado Boulder): Plasma kinetics
- Dr Rami Vainio (University of Helsinki): Energetic particle acceleration and propagation
- Prof. Marco Velli (Istituto Nazionale di Astrofisica, Firenze): Theory and modelling of the coronal heating, waves and turbulence
- Dr Susanne Vennerstrom (Danish National Space Center, Copenhagen): Large scale heliospheric magnetic field structure
- Prof. Robert Wimmer-Schweingruber (University of Kiel): Solar wind particles and composition; member, EPD consortium
- Prof. Gary Zank (University of Alabama at Huntsville): Theory and modelling of solar wind acceleration
Useful Links
Solar Orbiter Links: