Large scale 1/f magnetic field spectrum in the solar wind close to the Sun: comparison between 0.15 and 0.3AU

Lorenzo Matteini1,2, Christopher H K Chen3, David Stansby4, Timothy Simon Horbury4, Denise Perrone5, Anna Tenerani6, Marco Velli7, Stuart Bale8, Marc Pulupa9, David Malaspina10, John W Bonnell9, Peter Harvey9, Keith Goetz11, Thierry Dudok de Wit12 and Robert J MacDowall13, (1)Imperial College London, Physics Department, London, United Kingdom, (2)Observatoire de Paris, LESIA, Paris, France, (3)Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom, (4)Imperial College London, London, SW7, United Kingdom, (5)ASI – Italian Space Agency, Rome, Italy, (6)California Institute of Technology, Pasadena, CA, United States, (7)University of California Los Angeles, Los Angeles, CA, United States, (8)University of California, Berkeley, Berkeley, CA, United States, (9)University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (10)University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (11)University of Minnesota, Minneapolis, MN, United States, (12)LPC2E, CNRS and University of Orléans, Orléans, France, (13)NASA/Goddard Space Flight Center, Greenbelt, United States