{"id":83160,"date":"2023-05-29T11:29:56","date_gmt":"2023-05-29T08:29:56","guid":{"rendered":"https:\/\/myrtalycongress.gr\/?page_id=83160"},"modified":"2023-05-29T13:55:07","modified_gmt":"2023-05-29T10:55:07","slug":"abstracts-flux","status":"publish","type":"page","link":"https:\/\/myrtalycongress.gr\/en\/abstracts-flux\/","title":{"rendered":"Abstracts Flux"},"content":{"rendered":"
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NAME<\/strong><\/span><\/h4>\n<\/td>\n

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TITLE<\/strong><\/span><\/h4>\n<\/td>\n<\/tr>\n

Brun <\/strong>Allan Sacha<\/td>\nON THE INTERPLAY BETWEEN FLUX EMERGENCE AND
\nTURBULENT CONVECTION<\/td>\n<\/tr>\n
Bellot Rubio<\/strong> Luis<\/td>\nUNIPOLAR AND BIPOLAR MAGNETIC FLUX APPEARANCE IN THE QUIET SUN INTERNETWORK<\/td>\n<\/tr>\n
Chintzoglou<\/strong> Georgios<\/td>\nCOLLISIONAL SHEARING: A POSSIBLE MECHANISM PRODUCING RECURRENT EXPLOSIVE (FLARE AND CME) ACTIVITY IN SOLAR ACTIVE REGIONS<\/td>\n<\/tr>\n
Finley<\/strong> Adam<\/td>\nTHE ROLE OF SURFACE DYNAMICS IN THE SOLAR DYNAMO<\/td>\n<\/tr>\n
Guglielmino<\/strong> Salvo<\/td>\nMULTIWAVELENGTH OBSERVATIONS OF SMALL-SCALE ERUPTIVE
\nPHENOMENA DURING FLUX EMERGENCE IN ACTIVE REGIONS<\/td>\n<\/tr>\n
Hansteen<\/strong> Viggo<\/td>\nTHE MG II H&K LINES AND FLUX EMERGENCE: HOW HIGH IS THE
\nCHROMOSPHERE<\/td>\n<\/tr>\n
Hotta<\/strong> Hideyuki<\/td>\nFLUX EMERGENCE SIMULATION FROM THE BASE OF THE
\nCONVECTION ZONE TO THE PHOTOSPHERE<\/td>\n<\/tr>\n
Jouve<\/strong> Laurene<\/td>\nPARAMETRIZING THE FLUX EMERGENCE PROCESS IN SIMPLIFIED
\nDYNAMO MODELS<\/td>\n<\/tr>\n
Leake<\/strong> James<\/td>\nON THE PHOTOSPHERIC IMPRINTS OF SOLAR CORONAL ELECTRIC
\nCURRENTS<\/td>\n<\/tr>\n
MacTaggart<\/strong> David<\/td>\nMAGNETIC WINDING AND THE STRUCTURE OF EMERGING ACTIVE
\nREGIONS<\/td>\n<\/tr>\n
Martinez-Sykora<\/strong> Juan<\/td>\nON THE THERMAL AND FARLEY BULEMAN INSTABILITY IN FLUX
\nEMERGENCE<\/td>\n<\/tr>\n
Mathioudakis<\/strong> Mihalis<\/td>\nFLARE INDUCED PHOTOSPHERIC LINE ASYMMETRIES –
\nAPPLICATIONS TO SOLAR AND STELLAR FLARES<\/td>\n<\/tr>\n
Moraitis<\/strong> Kostas<\/td>\nTHE ROLE OF MAGNETIC HELICITY IN EXPLAINING AN MHD FLUX
\nEMERGENCE SIMULATION<\/td>\n<\/tr>\n
Nindos<\/strong> Alexander<\/td>\nPROPERTIES OF THE MAGNETIC FIELD IN AN MHD SIMULATION
\nOF CORONAL JETS<\/td>\n<\/tr>\n
N\u00f3brega-Siverio<\/strong> Daniel<\/td>\nAN OBSERVATIONAL STUDY OF MAGNETIC FLUX EMERGENCE LEADING TO A DARK BUBBLE, EB, SURGE, AND A UV BURST REACHING 1 MK<\/td>\n<\/tr>\n
Norton<\/strong> Aimee<\/td>\nWHY ARE ACTIVE REGION FLUX EMERGENCE RATES LOWER IN OBSERVATIONS THAN SIMULATIONS?<\/td>\n<\/tr>\n
Pariat<\/strong> Etienne<\/td>\nDYNAMICS OF MAGNETIC ENERGY AND MAGNETIC HELICITY IN ACTIVE REGIONS: RECENT NUMERICAL AND OBSERVATIONAL RESULTS<\/td>\n<\/tr>\n
Schmieder<\/strong> Brigitte<\/td>\nLONG-TERM EMERGING MAGNETIC FLUX AND INTERMITTENT BLOB SOLAR JETS<\/td>\n<\/tr>\n
Strugarek<\/strong> Antoine<\/td>\nMODELLING SOLAR ERUPTIVE EVENTS FROM THEIR ONSET TO THEIR PROPAGATION AT 1 AU<\/td>\n<\/tr>\n
Torok<\/strong> Tibor<\/td>\nSOLAR ERUPTIONS TRIGGERED BY FLUX EMERGENCE<\/td>\n<\/tr>\n
Zhuleku<\/strong> Eugene<\/td>\nMAGNETIC FLUX EMERGENCE SIMULATIONS OF TOROIDAL FLUX TUBES IN THE SUN AND CREATION OF JETS<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

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