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: Imaging of the solar atmosphere in the centimetre-millimeter band through Single-Dish observations (G. Murtas)

ESPOS
  • Datum: 31.01.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Giulia Murtas
  • University of Exeter
  • Ort: University of Exeter (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
Solar observations offer both a rich interdisciplinary laboratory on fundamental astrophysics and precious tools for Space Weather applications. The involved plasma processes determine a complex radio ... [mehr]

ESP Online Seminar: Chromospheric observations and magnetic configuration of a supergranular structure (Carolina Robustini)

ESPOS
  • Datum: 14.02.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Carolina Robustini
  • Stockholm University
  • Ort: Institute for Solar Physics, Stockholm University (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
We present high spatial resolution narrow-band images in three different chromospheric spectral lines, including Ca II K with the new CHROMospheric Imaging Spectrometer installed at the Swedish 1-m ... [mehr]

ESP Online Seminar: Emerging bipolar magnetic pairs in the solar photosphere: diffusion properties and contribution to the coronal heating (Luca Giovannelli)

ESPOS
  • Datum: 14.03.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Luca Giovannelli
  • University of Rome Tor Vergata
  • Ort: University of Rome Tor Vergata (broadcasted at MPS)
  • Raum: Aquila + Bootes
  • Gastgeber: Andreas Lagg
The ubiquitous presence of small magnetic elements in the Quiet Sun represents a prominent coupling between the photosphere and the upper layers of the Sun’s atmosphere. Small magnetic element ... [mehr]

ESP Online Seminar: 3D Whole-Prominence Fine Structure models: the current state of the affairs (Stanislav Gunár)

ESPOS
  • Datum: 28.03.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Stanislav Gunár
  • Astronomical Institute of the Czech Academy of Sciences
  • Ort: Astronomical Institute of the Czech Academy of Sciences (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
To understand the links between the distribution of the prominence plasma, the configuration of its magnetic field and the observations of prominence/filament fine structures obtained in UV/EUV ... [mehr]

ESP Online Seminar: The Sun from Coimbra: history, recent results and perspectives (João Fernandes)

ESPOS
  • Datum: 11.04.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): João Fernandes
  • University of Coimbra, Portugal
  • Ort: University of Coimbra, Portugal (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
The Astronomical Observatory of the Coimbra University has a collection of solar observations on a daily basis, since 1926. We obtain regular observations of the full solar disk using a classical ... [mehr]

ESP Online Seminar: 2D and 3D Kinematic Analysis of an Ideal-MHD Prominence Eruption (Thomas Rees-Crockford)

ESPOS
  • Datum: 25.04.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Thomas Rees-Crockford
  • Northumbria University, Newcastle upon Tyne, England
  • Ort: Northumbria University (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
We carry out multi-dimensional kinematic analysis of a prominence eruption in order to characterise the role of eruptive ideal-MHD instabilities. Using SDO/AIA and STEREO/EUVI-A we reconstruct the ... [mehr]

ESP Online Seminar: Formation and morphology of solar circular polarization with dichroism, atomic polarization and velocity gradients (Edgar S. Carlin)

ESPOS
  • Datum: 09.05.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Edgar S. Carlin
  • Instituto de Astrofísica de Canarias, Tenefrife, Spain
  • Ort: Instituto de Astrofísica de Canarias (broadcasted at MPS)
  • Raum: Auditorium
  • Gastgeber: Andreas Lagg
Since the work of Carlin et al. (2012), more studies have investigated, with the help of MHD models of the solar chromosphere, the behavior of scattering linear polarization (LP) in presence of ... [mehr]

ESP Online Seminar: Emergence of small-scale magnetic flux in the quiet Sun, observed from the photosphere to the corona (Ioannis Kontogiannis)

ESPOS
  • Datum: 20.06.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Ioannis Kontogiannis
  • Leibniz-Institut für Astrophysik Potsdam, AIP
  • Ort: Instituto de Astrofísica de Canarias (broadcasted at MPS)
  • Raum: Online only
  • Gastgeber: AIP

ESP Online Seminar: Swirls and Alfvén pulses in the Solar Atmosphere (JiaJia Liu)

ESPOS
  • Datum: 12.09.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): JiaJia Liu
  • University of Sheffield, Solar Physics and Space Plasma Research Centre
  • Ort: Plasma Dynamics Group, University of Sheffield (broadcasted at MPS)
  • Raum: Seminar rooms Aquila + Bootes
  • Gastgeber: Andreas Lagg

ESP Online Seminar: The largest flares of solar cycle 24 as potential clues for stellar superflares (Paolo Romano)

ESPOS
  • Datum: 26.09.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Paolo Romano
  • University of Catania / INAF - Catania Astrophysical Observatory
  • Ort: University of Catania / INAF - Catania Astrophysical Observatory (broadcasted at MPS)
  • Raum: Seminar rooms Cygnus + Draco
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: Nonequilibrium ionization and ambipolar diffusion in magnetic flux emergence processes (Daniel Nóbrega-Siverio)

ESPOS
  • Datum: 10.10.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Daniel Nóbrega-Siverio
  • Rosseland Centre for Solar Physics, University of Oslo
  • Ort: Rosseland Centre for Solar Physics, University of Oslo (broadcasted at MPS)
  • Raum: Seminar rooms Aquila + Bootes
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: Eruptions and flaring activity in emerging quadrupolar regions (Petros Syntelis)

ESPOS
  • Datum: 24.10.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Petros Syntelis
  • Solar and Magnetospheric Theory Group, University of St Andrews
  • Ort: University of St Andrews broadcasted at MPS
  • Raum: Seminar room Gemini
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: MHD wave modes in the solar magnetic flux tubes with elliptical cross-section (Anwar Ali Aldhafeeri)

ESPOS
  • Datum: 07.11.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Anwar Ali Aldhafeeri
  • Plasma Dynamics Group, The University of Sheffield
  • Ort: The University of Sheffield (broadcasted at MPS)
  • Raum: Seminar room Gemini
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: Spectral diagnostics of cool flare loops observed by SST (Julius Koza)

ESPOS
  • Datum: 07.11.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Julius Koza
  • Astronomical Institute, Slovak Academy of Sciences
  • Ort: Astronomical Institute, Slovak Academy of Sciences (broadcasted at MPS)
  • Raum: Seminar room Gemini
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: Penumbral brightening events (Mariarita Murabito)

ESPOS
  • Datum: 05.12.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Mariarita Murabito
  • INAF-OAR National Institute for Astrophysics, Italy
  • Ort: INAF-OAR National Institute for Astrophysics, Italy (broadcasted at MPS)
  • Raum: Seminar rooms Aquila + Bootes
  • Gastgeber: Pradeep Chitta

ESP Online Seminar: Solar irradiance variability and surface magnetism (Kok Leng Yeo)

ESPOS
  • Datum: 19.12.2019
  • Uhrzeit: 11:00 - 12:00
  • Vortragende(r): Kok Leng Yeo
  • Max Planck Institue for Solar System Research (MPS)
  • Ort: Max-Planck-Institut für Sonnensystemforschung
  • Raum: Auditorium
  • Gastgeber: Pradeep Chitta
The variation in solar irradiance is commonly assumed to be driven by its surface magnetism. Until recently, this assumption could not be verified conclusively as models of solar irradiance ... [mehr]
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