Power Law of Micro-Scale Turbulence in the Solar Wind Combining Observations of IPS at Different Wavelengths
Ernesto Aguilar-Rodriguez1, Julio Mejia-Ambriz2, E. Romero-Hernandez3, Oyuki Chang4, Carlos Arturo Perez Alanis5, Pedro Corona-Romero2, Mario Mark Bisi6, I. V. Chashei7, Richard Andrew Fallows8, Americo Gonzalez-Esparza2, Periasamy K Manoharan9, Munetoshi Tokumaru10 and S. A. Tyul'bashev7, (1)Universidad Nacional Autonóma de México, Instituto de Geofísica, Unidad Michoacán, Morelia, Mexico, (2)Universidad Nacional Autonóma de México, SCiESMEX, Instituto de Geofísica, Unidad Michoacán, Morelia, Mexico, (3)Universidad Nacional Autonoma de Mexico, SCiESMEX, Instituto de Geofísica, Unidad Michoacán, Mexico City, Mexico, (4)Universidad Nacional Autonoma de Mexico, Posgrado en Ciencias de la Tierra, Mexico City, Mexico, (5)UNAM National Autonomous University of Mexico, Posgrado en Ciencias de la Tierra, Mexico City, Mexico, (6)STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, (7)Lebedev Physical Institute, Pushchino Radio Astronomy Observatory, Moscow, Russia, (8)ASTRON, The Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (9)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (10)Nagoya University, Institute for Space-Earth Environmental, Nagoya, Japan
