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Pregled bibliografske jedinice broj: 1141301

Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs


Calogovic, Jasa; Dumbović, Mateja; Sudar, Davor; Vršnak, Bojan; Martinić, Karmen; Temmer, Manuela; Veronig, Astrid
Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs // vEGU21, the 23rd EGU General Assembly
online, 2021. str. 1-1 (ostalo, međunarodna recenzija, sažetak)


CROSBI ID: 1141301 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs

Autori
Calogovic, Jasa ; Dumbović, Mateja ; Sudar, Davor ; Vršnak, Bojan ; Martinić, Karmen ; Temmer, Manuela ; Veronig, Astrid

Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, ostalo

Skup
VEGU21, the 23rd EGU General Assembly

Mjesto i datum
Online, 19-30.4.2021

Vrsta sudjelovanja
Ostalo

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
coronal mass ejection, space weather, drag based model

Sažetak
The Drag-based Model (DBM) is an analytical model for heliospheric propagation of Coronal Mass Ejections (CMEs) that predicts the CME arrival time and speed at Earth or any other given target in the solar system. It is based on the equation of motion and depends on initial CME parameters, background solar wind speed, w and the drag parameter γ. A very short computational time of DBM (< 0.01s) allowed us to develop the Drag-Based Ensemble Model (DBEM) that considers the variability of model input parameters by making an ensemble of n different input parameters to calculate the distribution and significance of the DBM results. Using such an approach, we apply DBEM to determine the most likely CME arrival times and speeds, quantify the prediction uncertainties and calculate the confidence intervals. Recently, a new DBEMv3 version was developed including the various improvements and Graduated Cylindrical Shell (GCS) option for the CME geometry input as well as the CME propagation visualizations. Thus, we compare the DBEMv3 with previous DBEM versions (e.g. DBEMv2), evaluate it and determine the DBEMv3 performance and errors by using various CME-ICME lists. Compared to the previous versions, the DBEMv3 provides very similar results for all calculated output parameters with slight improvement in the performance. Based on the evaluation performed for 146 CME- ICME pairs, the DBEMv3 performance with mean error (ME) of -11.3 h, mean absolute error (MAE) of 17.3 h was obtained, similar to previous DBM and DBEM evaluations. Fully operational DBEMv3 web application was integrated as one of the ESA Space Situational Awareness portal services (https://swe.ssa.esa.int/current-space- weather) providing an important tool for space weather forecasters.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove:
Geodetski fakultet, Zagreb

Citiraj ovu publikaciju

Calogovic, Jasa; Dumbović, Mateja; Sudar, Davor; Vršnak, Bojan; Martinić, Karmen; Temmer, Manuela; Veronig, Astrid
Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs // vEGU21, the 23rd EGU General Assembly
online, 2021. str. 1-1 (ostalo, međunarodna recenzija, sažetak)
Calogovic, J., Dumbović, M., Sudar, D., Vršnak, B., Martinić, K., Temmer, M. & Veronig, A. (2021) Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs. U: vEGU21, the 23rd EGU General Assembly.
@article{article, year = {2021}, pages = {1-1}, keywords = {coronal mass ejection, space weather, drag based model}, title = {Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs}, keyword = {coronal mass ejection, space weather, drag based model}, publisherplace = {online} }
@article{article, year = {2021}, pages = {1-1}, keywords = {coronal mass ejection, space weather, drag based model}, title = {Drag-Based Ensemble Model (DBEM) to predict the heliospheric propagation of CMEs}, keyword = {coronal mass ejection, space weather, drag based model}, publisherplace = {online} }




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