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Multi-source connectivity as the driver of solar wind variability in the heliosphere.

Autor: Yardley SL; Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, UK.; Department of Meteorology, University of Reading, Reading, UK.; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK.; Donostia International Physics Center (DIPC), San Sebastián, Spain., Brooks DH; Department of Physics & Astronomy, George Mason University, Fairfax, VA USA., D'Amicis R; INAF-Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy., Owen CJ; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Long DM; School of Physical Sciences, Dublin City University, Dublin, Ireland., Baker D; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Démoulin P; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, Meudon, France.; Laboratoire Cogitamus, Paris, France., Owens MJ; Department of Meteorology, University of Reading, Reading, UK., Lockwood M; Department of Meteorology, University of Reading, Reading, UK., Mihailescu T; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Coburn JT; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Dewey RM; Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA., Müller D; European Space Agency, ESTEC, Noordwijk, The Netherlands., Suen GHH; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Ngampoopun N; Department of Space and Climate Physics, UCL Mullard Space Science Laboratory, Holmbury St Mary, UK., Louarn P; Institut de Recherche en Astrophysique et Planétologie, Toulouse, France., Livi S; Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA.; Present Address: Southwest Research Institute, San Antonio, TX USA., Lepri S; Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA., Fludra A; RAL Space, UKRI STFC Rutherford Appleton Laboratory, Chilton, UK., Haberreiter M; Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, Davos Dorf, Switzerland., Schühle U; Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany.

Publikováno v: Nature astronomy [Nat Astron] 2024; Vol. 8 (8), pp. 953-963. Date of Electronic Publication: 2024 May 28.

A transient enhancement of Mercury's exosphere at extremely high altitudes inferred from pickup ions.

Autor: Jasinski JM; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA. jasinski@jpl.nasa.gov., Regoli LH; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA.; Applied Physics Laboratory, The John Hopkins University, Laurel, MD, USA., Cassidy TA; Laboratory of Atmospheric and Space Sciences, University of Colorado Boulder, Boulder, CO, USA., Dewey RM; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA., Raines JM; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA., Slavin JA; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA., Coates AJ; Mullard Space Science Laboratory, UCL, Dorking, UK.; Center for Planetary Sciences, UCL/Birkbeck, London, UK., Gershman DJ; NASA Goddard Space Flight Center, Greenbelt, MD, USA., Nordheim TA; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA., Murphy N; NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.

Publikováno v: Nature communications [Nat Commun] 2020 Sep 29; Vol. 11 (1), pp. 4350. Date of Electronic Publication: 2020 Sep 29.

Intense energetic electron flux enhancements in Mercury's magnetosphere: An integrated view with high-resolution observations from MESSENGER.

Autor: Baker DN; Laboratory for Atmospheric and Space Physics University of Colorado Boulder Colorado USA., Dewey RM; Laboratory for Atmospheric and Space Physics University of Colorado Boulder Colorado USA., Lawrence DJ; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Goldsten JO; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Peplowski PN; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Korth H; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Slavin JA; Department of Atmospheric, Oceanic and Space Sciences University of Michigan Ann Arbor Michigan USA., Krimigis SM; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA; Office of Space Research and Technology Academy of Athens Athens Greece., Anderson BJ; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Ho GC; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., McNutt RL Jr; The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA., Raines JM; Department of Atmospheric, Oceanic and Space Sciences University of Michigan Ann Arbor Michigan USA., Schriver D; Department of Physics and Astronomy University of California Los Angeles California USA., Solomon SC; Department of Terrestrial Magnetism Carnegie Institution of Washington Washington District of Columbia USA; Lamont-Doherty Earth Observatory Columbia University Palisades New York USA.

Publikováno v: Journal of geophysical research. Space physics [J Geophys Res Space Phys] 2016 Mar; Vol. 121 (3), pp. 2171-2184. Date of Electronic Publication: 2016 Mar 18.