IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
Statistics of magnetic autocorrelation lengths in the Solar Wind
Autor/es:
M. E. RUIZ; DASSO, S.; W. H. MATTHAEUS; J.M. WEYGAND; E. MARSCH; J. ISAACS
Reunión:
Simposio; IAUS 300, Nature of prominences and their role in space weather; 2013
Resumen:
There remain unanswered questions regarding the evolution of turbulent
properties in different solar wind regimes, and their role in the dynamics
of the Sun-Earth system. In this work we analyze the evolution
of the spatial structure of interplanetary magnetic field fluctuations,
by examining the heliospheric autocorrelation functions (R) based on
in situ observations and using classical single-spacecraft
techniques. Correlation lengths derived from R can be viewed as a
measured of the integral scale of the turbulence. We focus on the
evolution of these correlation lengths based on an analysis made at
different heliodistances from the Sun, using observations from the
Helios, ACE and Ulysses spacecraft. We distinguish different turbulent
properties for the Parker-type Solar Wind and different transients,
including some geoeffective transients which affect space weather
conditions, as interplanetary coronal mass ejections or magnetic clouds.