@InProceedings{LeeSSHSCSRGTRWB:2017:CoCaSt,
               author = "Lee, Sun Hee and Silveira, Marcos D. and Sibeck, David G. and 
                         Hwang, Kyoung-Joo and Samsonov, Andrey and Carr, Chris and 
                         Schwartz, Steven J. and Ruohoniemi, J. Michael and Giles, Barbara 
                         L. and Torbert, Roy B. and Russell, Christopher T. and Wei, 
                         Hanying and Burch, James L.",
          affiliation = "{NASA Goddard Space Flight Center} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {NASA Goddard Space Flight Center} 
                         and {Goddard Planetary Heliophysics Institute - GPHI} and {St. 
                         Petersburg State University} and {Imperial College London} and 
                         {Imperial College London} and {Virginia Polytechnic Institute and 
                         State University} and {NASA Goddard Space Flight Center} and 
                         {Southwest Research Institute} and {University of California Los 
                         Angeles} and {University of California Los Angeles} and {Southwest 
                         Research Institute}",
                title = "Comprehensive case study of magnetosheath pressure pulses and 
                         rapid magnetopause/bow shock motion",
            booktitle = "Proceedings...",
                 year = "2017",
         organization = "AGU Fall Meeting",
             abstract = "We present multi-point observations of dayside transient events 
                         and their impact on the Earths magnetosphere. The Magnetospheric 
                         Multiscale (MMS) spacecraft observed a series of pulsed density 
                         enhancements and a rapid transition from the magnetosphere to the 
                         region upstream from the bow shock within just 2 min on 10 
                         December 2016. Strong antisunward, and sometimes sunward, flows 
                         are observed in conjunction with the pulses, which are bathed in 
                         energetic particles that appear to have escaped from the outer 
                         magnetosphere rather than energization of solar wind particles 
                         within the foreshock. The selectively escaping ion species provide 
                         information concerning distance from the magnetopause to the bow 
                         shock. The transient magnetosheath density and (corresponding 
                         dynamic pressure) enhancements may result from solar wind 
                         discontinuities interacting with the bow shock and/or ripples 
                         generated on the bow shock surface. Observed magnetospheric 
                         responses to these transient phenomena include patchy, sporadic 
                         magnetopause reconnection, magnetopause surface waves, transient 
                         magnetic field variations in ground magnetograms and ionospheric 
                         flow enhancements. We inspect the strikingly different 
                         observations seen by multipoint solar wind monitors at different 
                         locations and the transient response seen by high-latitude ground 
                         magnetometers and radars.",
  conference-location = "New Orleans",
      conference-year = "11-15 Dec.",
             language = "en",
           targetfile = "lee_comprehensive.pdf",
        urlaccessdate = "27 abr. 2024"
}