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INSTITUTET FÖR RYMDFYSIK |
UPPSALA |
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Swedish Institute of Space Physics |
(59°50.272′N, 17°38.786′E) |
Student project at IRF Uppsala
Internship/Praktik
Magnetic-cloud geoeffectiveness from different solar wind-magnetosphere coupling functions
Student: Alexandre Muller,
Institut Supérieur de l'Aéronautique et de l'Espace, Toulouse
Supervisor:
Vanina Lanabere
Period: spring-summer 2024
Abstract
Magnetic Clouds (MC) are large-scale plasma structures expelled from the Sun into the
interplanetary medium. When they reach Earth, these can lead to intense geomagnetic
storms. Using the MC database compiled by Lepping et al. and the corresponding
data from both the Wind spacecraft and the geomagnetic index Disturbance Storm Time
(DST), we provide a coupled theoretical and experimental analysis of the geoeffectiveness
of MC depending mainly on the orientation of the axis. We propose a method which
uses rotation matrices to change the orientation of the MC and compute the coupling
function (a physical quantity which aggregates solar wind parameters to explain ground
disturbances) to predict the minimum value of the DST reached. In the end, we demonstrated the validity of the method by performing it on 161 clouds registered between 1995
and 2012. We obtained an empirical relation to link the perturbation in the DST index
with the maximum of a MC’s electric field as proposed by Kan and Lee in 1979. We
also highlight that the most geoeffective orientation for a given cloud is not always the
southern pointing axis but depends on the CA parameter (the minimum distance between
the spacecraft and the MC’s axis). Finally we validate our method by showing that on
average, results are consistent with the theory. Since the validity of our analysis for a
given cloud depends on the goodness of the fit with the Lundquist model, this raises the
question whether this model is always the correct one.
Results
Final report
Process pipeline implemented and used in the project.
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