IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
Two Point Measurements of statistical properties of solar wind turbulence
Autor/es:
MATTHAEUS W.H.; DASSO S.; WEYGAND J.M.; SMITH C.W.; KIVELSON M.G.
Lugar:
San Francisco, USA
Reunión:
Conferencia; American Geophysical Union, Fall Meeting 2006; 2006
Institución organizadora:
AGU
Resumen:
Multipoint measurements are of central importance in establishing the
three dimensional statistical and correlation properties of low
frequency interplanetary turbulence, while also serving to corroborate
the wealth of information gleaned from single point measurements based
on the "frozen-in flow" approximation. Multipoint measurements with
widely ranging spatial separations and well controlled time calibration
are required to unravel the space-time structure of MHD scale
turbulence, which presents complexity in both domains. To address these
problems we have been developing methods for statistical and correlation
analyses of multiple streams of spacecraft data, and have developed a
well documented object oriented (Python based) software framework that
is designed for ease of adaptation, flexibility and effective
collaboration between groups. Progress on our three target problems will
be reviewed here: (1) Determination of the two-point spatial correlation
properties of solar wind turbulence. Our main results here are based on
simultaneous solar wind magnetic field data from the ACE, Cluster,
Geotail, IMP 8, and Wind spacecraft. We have determined [1] the
direction averaged spatial correlation function, the correlation (outer)
scale, and the inner (Taylor) microscale near 1 AU. The correlation
scale is determined to be 1.2 × 106 km, the Taylor scale is 2500
km, and the effective magnetic Reynolds number is calculated to be
230,000. Similar analyses have been carried out plasma sheet data [2].
Taylor scale computations require careful treatment of the Cluster data
[3]. (2) Evaluation of accuracy of the frozen in approximation. This
ongoing work will focus on comparison of correlation scale, Taylor scale
and correlation function data from single and multiple spacecraft. (3)
Evaluation of the Eulerian (plasma frame single point multiple time)
correlation function. Progress in developing a methodology for this
problem will be reviewed. This research supported by the RSSW1AU and
Cluster programs.