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from the corresponding populations. We will tackle this challenge by extending the JSDM approach to capture intra-annual variation as well as by developing mechanistic state-space models that describe
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structure and their possible extended formation from the low solar corona to inter-planetary space. Most existing global MHD models are largely limited by their lower boundary at 0.1 astronomical unit and
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plasma physics and space weather forecasting. The RIB-Wind project aims to overcome key limitations in current heliospheric models, which typically rely on empirical assumptions to define inner boundary
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(autumn/spring 20xx) If you don’t have a right to study for doctoral degree in DPInvest at the University of Turku: a commitment from the supervisor to supervise the doctoral thesis Information on completed