caa a22 4500 445815876 CHVBK 20180317145228.0 cr unu---uuuuu 170323e20111201xx s 000 0 eng 10.1007/s11214-011-9826-4 doi (NATIONALLICENCE)springer-10.1007/s11214-011-9826-4 Recent Results from Titan's Ionosphere [Elektronische Daten] [A. Coates, J.-E. Wahlund, K. Ågren, N. Edberg, J. Cui, A. Wellbrock, K. Szego] Titan has the most significant atmosphere of any moon in the solar system, with a pressure at the surface larger than the Earth's. It also has a significant ionosphere, which is usually immersed in Saturn's magnetosphere. Occasionally it exits into Saturn's magnetosheath. In this paper we review several recent advances in our understanding of Titan's ionosphere, and present some comparisons with the other unmagnetized objects Mars and Venus. We present aspects of the ionospheric structure, chemistry, electrodynamic coupling and transport processes. We also review observations of ionospheric photoelectrons at Titan, Mars and Venus. Where appropriate, we mention the effects on ionospheric escape. Springer Science+Business Media B.V., 2011 Ionosphere nationallicence Titan nationallicence Mars nationallicence Venus nationallicence Coates A. Department of Space and Climate Physics, Mullard Space Science Laboratory, University College London, RH5 6NT, Holmbury St. Mary, Dorking, UK aut Wahlund J.-E Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut Ågren K. Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut Edberg N. Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut Cui J. Department of Astronomy & Key Laboratory of Modern Astronomy and Astrophysics in Ministry of Education, Nanjing University, 210093, Nanjing, China aut Wellbrock A. Department of Space and Climate Physics, Mullard Space Science Laboratory, University College London, RH5 6NT, Holmbury St. Mary, Dorking, UK aut Szego K. Research Institute for Particle and Nuclear Physics, Hungarian Academy of Sciences, KFKI-RMKI, Budapest, Hungary aut Space Science Reviews Springer Netherlands 162/1-4(2011-12-01), 85-111 0038-6308 162:1-4<85 2011 162 11214 https://doi.org/10.1007/s11214-011-9826-4 text/html Onlinezugriff via DOI 1 review-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/s11214-011-9826-4 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Coates A. Department of Space and Climate Physics, Mullard Space Science Laboratory, University College London, RH5 6NT, Holmbury St. Mary, Dorking, UK aut NATIONALLICENCE 700 1- Wahlund J.-E Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut NATIONALLICENCE 700 1- Ågren K. Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut NATIONALLICENCE 700 1- Edberg N. Swedish Institute of Space Physics, Box 537, 751 21, Uppsala, Sweden aut NATIONALLICENCE 700 1- Cui J. Department of Astronomy & Key Laboratory of Modern Astronomy and Astrophysics in Ministry of Education, Nanjing University, 210093, Nanjing, China aut NATIONALLICENCE 700 1- Wellbrock A. Department of Space and Climate Physics, Mullard Space Science Laboratory, University College London, RH5 6NT, Holmbury St. Mary, Dorking, UK aut NATIONALLICENCE 700 1- Szego K. Research Institute for Particle and Nuclear Physics, Hungarian Academy of Sciences, KFKI-RMKI, Budapest, Hungary aut NATIONALLICENCE 773 0- Space Science Reviews Springer Netherlands 162/1-4(2011-12-01), 85-111 0038-6308 162:1-4<85 2011 162 11214 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer