Pregled bibliografske jedinice broj: 1072312
PREDICTING CME ARRIVAL TIME AND SPEED WITH DBEM
PREDICTING CME ARRIVAL TIME AND SPEED WITH DBEM // 2nd China-Europe Solar Physics Meeting
Hvar, Hrvatska, 2019. str. 1-1 (predavanje, međunarodna recenzija, sažetak, znanstveni)
CROSBI ID: 1072312 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
PREDICTING CME ARRIVAL TIME AND SPEED WITH DBEM
Autori
Jaša Čalogović, Mateja Dumbović, Bojan Vršnak, Davor Sudar, Manuela Temmer, Leila M. Mays, Astrid Veronig, Isabell Piantschitsch
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni
Skup
2nd China-Europe Solar Physics Meeting
Mjesto i datum
Hvar, Hrvatska, 06.05.2019. - 10.05.2019
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
coronal mass ejections ; interplanetary shocks ; space weather ; forecasts ; models ; Physics - Space Physics
Sažetak
The Drag-based Model (DBM) is an analytical model that predicts the CME arrival time and speed at Earth or any other target in the solar system. It is based on the equation of motion and depends on certain initial parameters such as CME launch speed, background solar wind speed and empirically derived drag parameter. DBM uses a CME cone geometry that includes CME’s angular half-width and longitude of CME source region as additional input parameters. The main advantage of DBM is a very short computational time (<1 ms) which allowed 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 distribution and significance of DBM results. Using such approach, DBEM can determine the most likely CME arrival times and speeds, quantify the prediction uncertainties and calculate the forecast confidence intervals. Recently, a fully operational DBEM web application was integrated as one of the ESA Space Situational Awareness portal services providing an important tool for space weather forecast. Using a simple web interface, the user can enter all input parameters and their uncertainties in order to get the CME arrival time and speed distributions at the target (e.g. Earth) based on several thousand DBM calculations within just few seconds. Recent developments of DBEM will be shown together with validation tests where DBEM is compared with observations and more complex numerical models (e.g. ENLIL).
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Geodetski fakultet, Zagreb