Mateja Dumbovic

Publications

• Radial evolution of the April 2020 stealth coronal mass ejection between 0.8 and 1 AU
• Generic profile of a long-lived corotating interaction region and associated recurrent Forbush decrease
• Drag-Based Ensemble Model (DBEMv4) with variable solar wind speed input
• Predicting the solar cycle amplitude with the new catalogue of hemispheric sunspot numbers
• Galactic cosmic rays as signatures of interplanetary transients
• Evidence of a complex structure within the 2013 August 19 coronal mass ejection
• Validation of the CME Geomagnetic Forecast Alerts Under the COMESEP Alert System
• Evidence of a complex structure within the 2013 August 19 CME. ICME radial and longitudinal evolution in the heliosphere.
• Editorial to the Special Issue “Propagation of Coronal Mass Ejections”
• CME-HSS Interaction and Characteristics Tracked from Sun to Earth
• An Analytical Diffusion-Expansion Model for Forbush Decreases Caused by Flux Ropes
• Validation of the CME Geomagnetic Forecast Alerts Under the COMESEP Alert System
• The unusual widespread solar energetic particle event on 2013 August 19
• Maximal growth rate of the ascending phase of a sunspot cycle for predicting its amplitude
• Modeling the Evolution and Propagation of 10 September 2017 CMEs and SEPs Arriving at Mars Constrained by Remote Sensing and In Situ Measurement
• Utilizing galactic cosmic rays as signatures of coronal mass ejections
• Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs
• Characteristics of a long-lived CIR and analytical modelling of the corresponding depression in the GCR flux
• Detailed Analysis of Solar Data Related to Historical Extreme Geomagnetic Storms: 1868-2010
• Using Forbush Decreases to Derive the Transit Time of ICMEs Propagating from 1 AU to Mars
• Geomagnetic Effects of Corotating Interaction Regions
• Heliospheric Evolution of Magnetic Clouds
• A statistical study of the long-term evolution of coronal hole properties as observed by SDO
• The Drag-based Ensemble Model (DBEM) for Coronal Mass Ejection Propagation
• An Analytical Diffusion–Expansion Model for Forbush Decreases Caused by Flux Ropes
• Forecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard
• Benchmarking CME Arrival Time and Impact: Progress on Metadata, Metrics, and Events
• Tracking and Validating ICMEs Propagating Toward Mars Using STEREO Heliospheric Imagers Combined With Forbush Decreases Detected by MSL/RAD
• Unusual Plasma and Particle Signatures at Mars and STEREO-A Related to CME–CME Interaction
• CME–HSS Interaction and Characteristics Tracked from Sun to Earth
• On the Interaction of Galactic Cosmic Rays with Heliospheric Shocks During Forbush Decreases
• CME–CME Interactions as Sources of CME Geoeffectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in 2017 Early September
• Relating CME density derived from remote sensing data to CME sheath solar wind plasma pile up as measured in-situ
• Using Forbush decreases at Earth and Mars to measure the radial evolution of ICMEs
• Predicting heliospheric propagation of CMEs with probabilistic Drag-Based Ensemble Model (DBEM)
• CME evolution and the corresponding Forbush decrease: modelling vs multi-spacecraft observation
• A new model describing Forbush Decreases at Mars: combining the heliospheric modulation and the atmospheric influence
• Understanding our capabilities in observing and modelling Coronal Mass Ejections
• Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations
• Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations
• Deriving CME Density From Remote Sensing Data and Comparison to In‐Situ Measurements
• Propagating Conditions and the Time of ICME Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models
• On the Rigidity Spectrum of Cosmic-Ray Variations within Propagating Interplanetary Disturbances: Neutron Monitor and SOHO/EPHIN Observations at ∼1–10 GV
• The Unusual Widespread Solar Energetic Particle Event on 2013 August 19: Solar origin, CME-driven shock evolution and particle longitudinal distribution
• Influence of the CME orientation on the ICME propagation
• Deriving CME volume and density from remote sensing data
• Statistical study of CMEs, lateral overexpansion and SEP events
• Comparative study of halo CME arrival predictions
• Quo vadis, European Space Weather community?
• Probabilistic Drag-Based Ensemble Model (DBEM) Evaluation for Heliospheric Propagation of CMEs
• Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars
• Strong coronal deflection of a CME and its interplanetary evolution to Earth and Mars
• A simple model of Forbush decreases caused by sheathless magnetic clouds
• Geoeffectiveness of Coronal Mass Ejections in the SOHO Era
• Heliospheric Propagation of Coronal Mass Ejections: Comparison of Numerical WSA-ENLIL+Cone Model and Analytical Drag-based Model
• Predicting CME transit time with neural networks
• Kinematics of Interacting ICMEs and Related Forbush Decrease: Case Study
• Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model
• The Successive CME on 13th; 14th and 15th February 2011 and Forbush decrease on 18 February 2011
• Cosmic ray modulation by different types of solar wind disturbances
• Solar Hα and white light telescope at Hvar Observatory
• Solar influences on the short-term cosmic ray modulation
• Cosmic ray modulation by solar wind disturbances
• Forecasting the Arrival of Coronal Mass Ejections: The Drag-Based Model
• Forbush Decrease Prediction Based on Remote Solar Observations
• Predicting coronal mass ejections transit times to Earth with neural network
• Extreme Geomagnetic Storms-1868-2010
• Three-dimensional relation between coronal dimming, filament eruption, and CME
• Refined Modeling of Geoeffective Fast Halo CMEs During Solar Cycle 24
• Deriving the interaction point of an Interplanetary Coronal Mass Ejection and High-Speed stream : A case study
• Probing CME’s inclination effects with EUHFORIA
• CME-CME-CIR interaction - comparison of "homologous" events from two different solar rotations
• A new method of measuring Forbush decreases
• Unveiling the journey of a highly inclined CME
• The Catalog of Hvar Observatory Solar Observations
• Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes
• Deriving the Interaction Point between a Coronal Mass Ejection and High-speed Stream: A Case Study
• Probing Coronal Mass Ejection Inclination Effects with EUHFORIA
• Three-part structure of a solar coronal mass ejection observed in low coronal signatures of Solar Orbiter
• Estimating the early propagation direction of the coronal mass ejection with DIRECD during the severe event on May 8 and for the follow-up event on June 8, 2024
• Constraints to the drag-based reverse modeling
• Comparative analysis of two episodes of strongly geoeffective coronal mass ejection events in November and December 2023
• Analyzing the Geomagnetic Impact of Interacting CMEs and Sector Boundary Crossings During Autumn 2023 Eruptive Events
• Why doesn’t model improvement result in better forecast: the 3D drag-based model for CME propagation example