IAFE   05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
Trace back of intermittent structures in the solar wind
Autor/es:
NAKWACKI, M.S.; RUIZ, M.E.; NUEVO, F.A.; MANDRINI, C.H.; DASSO, S.
Lugar:
Tandil
Reunión:
Congreso; 56 Reunión Anual de la Asociación Argentina de Astronomía; 2013
Institución organizadora:
AAA
Resumen:
The intermittent structures identified in the solar wind (SW)
are a key observable to study the nature of magnetohydrodynamic (MHD)
turbulence in systems with low dissipation rate, and can be characterized
by computing the degree of phase correlation of the magnetic field. Such
indicator is, commonly, studied near the Earth using in situ observations,
while the solar wind sources remain unknown. In this work, we study in
situ observations of magnetic field intensity from the Advanced Composition
Explorer (ACE) spacecraft, located near 1 AU from the Sun,
and synoptic charts from the Wilcox Obsevatory, together with Potential
Field Source Surface (PFSS) models both from Wilcox and the Michelson
Doppler Imager (MDI) onboard the Solar and Heliospheric Observatory
(SOHO). We identify one intermittent period by computing the phase
coherence index. For these SW observations, we attempt to find the corresponding
solar source identifying a particular pattern of the coronal
magnetic field at the source surface, located at 2.5 R at the time the
SW would have left the Sun considering its speed at 1 AU to be constant.
To ascertain that this magnetic pattern plays a significant role as source
of SW intermittence, more examples should be analyzed.