Modeling the Magnetic Field of Eruptive Structures from the Corona to the Heliosphere via Self-consistent Data-driven Time-dependent Simulations
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W[2022AGUFMSH22E2051P]
LA["Linked Authors (3)"]
LI["Linked Institutions (1)"]
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W== affil ==>LI
click LA "#linked-authors"
click LI "#linked-institutions"
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