The school will serve as a comprehensive introduction to the importance of
multipoint measurements in the understanding of heliospheric space plasma
physics from the Sun to the Earth’s magnetospheric environment. Multipoint
measurements are indeed crucial for investigating phenomena such as
magnetic reconnection, plasma turbulence, shock wave formation, and
particle acceleration, as well as, the three-dimensional structure of the solar
corona, tracking the evolution of solar eruptions, and understanding the
initiation and propagation of solar wind streams, which all play central roles
in the dynamics of the solar and heliospheric plasmas as well as its
interaction with planetary magnetospheres. This course aims at providing an
overview of the importance of multipoint measurements in studying space
plasma processes occurring in the heliosphere to establish a critical
connection between the data from future missions and
complementary data from next-generation ground-based observatories. The
school is addressed to graduate and PhD students, young scientists as well as
undergraduates in heliophysics, space plasma physics, planetary sciences, or
related fields. Early-career stage professionals are invited to apply as well.
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