Characterizing Dissipation Scale Solar Wind Turbulence at 1 AU Using Correlation Functions.
Characterizing Dissipation Scale Solar Wind Turbulence at 1 AU Using Correlation Functions.
Alvin Angeles1, Harlan E. Spence2, Charles William Smith3, Bernard John Vasquez4, Ian Cohen5, Kevin James Genestreti6, Ruth M. Skoug7, Savvas Raptis8,9, Christine Gabrielse10, Daniel J Gershman11, David Fischer12, Christopher T Russell13, James L Burch14, Roy B Torbert3 and Werner Magnes12, (1)University of New Hampshire Main Campus, Physics and Astronomy Space Science Center, Durham, United States, (2)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (3)University of New Hampshire, Durham, United States, (4)University of New Hampshire, Durham, NH, United States, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (6)Southwest Research Institute, Durham, United States, (7)Los Alamos National Laboratory, Los Alamos, NM, United States, (8)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (9)KTH Royal Institute of Technology, Division of Space and Plasma Physics, Stockholm, Sweden, (10)The Aerospace Corporation, El Segundo, United States, (11)NASA Goddard Space Flight Center, Greenbelt, United States, (12)Austrian Academy of Sciences, Space Research Institute, Graz, Austria, (13)University of California Los Angeles, Los Angeles, United States, (14)Southwest Research Institute San Antonio, San Antonio, United States