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Multi-Scale Physics in Coronal Heating and Solar Wind Acceleration

118.00 EUR 104.34 EUR 12% Off

Ergründet die komplexen Prozesse der Sonnenkorona bis zur inneren Heliosphäre, verbindet theoretische Magnetohydrodynamik mit modernen Beobachtungsdaten und liefert neue Erkenntnisse über Plasmaströmungen, Wärmeleitung und Energieverteilung.

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