European Solar Physics Online Seminar Archiv

Auf Initiative der Universität Oslo nimmt die MPS an der Reihe "European Solar Physics Online Seminar" (ESPOS) teil. Details finden Sie hier: https://folk.uio.no/tiago/espos/ 
Ziel dieser Videokonferenzreihe ist es, Ideen mit einem spezialisierten Publikum breiter zu verbreiten und Studenten und anderen jungen Forschern, die nicht regelmäßig zu Konferenzen reisen, einen Einblick in die Spitzenforschung zu geben. Die ESPOS-Serie soll jeden zweiten Donnerstag um 11 Uhr stattfinden.  

ESP Online Seminar: Magnetic Rayleigh–Taylor Unstable Plumes and Hybrid KH-RT Instability into a Loop-like Eruptive Prominence (Sudheer K. Mishra)

ESPOS

• Datum: 23.01.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): Sudheer K. Mishra
• Department of Physics, Indian Institute of Technology (BHU), India
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Aquila + Bootes
• Gastgeber: Pradeep Chitta

The magnetic Rayleigh–Taylor instability is a fundamental MHD instability and recent observations show that this instability develops in the solar prominences. We analyze the observations from Solar ... [mehr]

ESP Online Seminar: Learning to Invert Solar Flares with RADYN Physics

ESPOS

• Datum: 20.02.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): John Armstrong
• University of Glasgow, UK
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Aquila + Bootes
• Gastgeber: Pradeep Chitta

During a solar flare, it is believed that reconnection takes place in the corona followed by fast energy transport to the chromosphere. The resulting intense heating strongly disturbs the ... [mehr]

ESP Online Seminar: Learning to Invert Solar Flares with RADYN Physics

ESPOS

• Datum: 20.02.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): John Armstrong
• University of Glasgow, UK
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Aquila + Bootes
• Gastgeber: Pradeep Chitta

During a solar flare, it is believed that reconnection takes place in the corona followed by fast energy transport to the chromosphere. The resulting intense heating strongly disturbs the ... [mehr]

ESP Online Seminar: Magnetic properties of short-lived penumbral microjets (Azaymi Litzi Siu Tapi)

ESPOS

• Datum: 05.03.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): Azaymi Litzi Siu Tapia
• Instituto de Astrofísica de Andalucía (IAA-CSIC), Spain
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Aquila + Bootes
• Gastgeber: Pradeep Chitta

Studying the polarization properties of penumbral microjets that have the shortest durations requires spectropolarimetric observations with the fastest temporal cadence possible and is currently a ... [mehr]

ESP Online Seminar: Solar Flare Prediction Using Magnetic Field Diagnostics Above the Photosphere (Marianna Korsos)

ESPOS

• Datum: 14.05.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): Marianna Korsos
• Aberystwyth University, UK
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Zoom
• Gastgeber: Pradeep Chitta

We present the application of the weighted horizontal gradient of magnetic field (WGM) flare prediction method to 3D extrapolated magnetic configurations of flaring solar ARs. The main aim is to ... [mehr]

ESP Online Seminar: Understanding hooks of solar flare ribbons and the evolution of coronal mass ejections (Juraj Lorinčík)

ESPOS

• Datum: 28.05.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): Juraj Lorinčík
• Astronomical Institute of the Czech Academy of Sciences
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Zoom
• Gastgeber: Pradeep Chitta

Solar flares and eruptions are one of the most energetic phenomena occuring in the solar system. They are typically described by the cartoon-like 2D Standard model of solar flares. This model is ... [mehr]

ESP Online Seminar: Study of damping of propagating kink waves in the solar corona (Ajay Tiwari)

ESPOS

• Datum: 11.06.2020
• Uhrzeit: 11:00 - 12:00
• Vortragende(r): Ajay Tiwari
• Northumbria University, Solar Physics group (UK)
• Ort: Max-Plack-Institut für Sonnensystemforschung
• Raum: Zoom
• Gastgeber: Pradeep Chitta

Propagating kink waves have been reported recently and have been found to be ubiquitous in the solar corona including in the quiet Sun. It is imperative to understand the mechanisms that enable their ... [mehr]