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Seminar: Ausgewählte Themen der Plasma-Astrophysik

Wichtige Informationen zum Online-Betrieb

Die Lehrveranstaltungen findet als Online-Lehrveranstaltung statt.

Zur Anmeldung senden Sie bitte eine Email mit:

  • Name, Vorname
  • email-Kontaktadresse
  • Studiengang (ggf. Universität)
  • Matrikelnummer

an sekretariat@astro.physik.tu-berlin.de.

Weitere Instruktionen werden Sie dann per email erhalten.


Lecturer: Prof. Dr. W.-Ch. Müller
Time: Thursday 12-14, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, ?, Begin: 2020-04-23 (weekly)
Language: German

Content:

Berichte über laufende Forschungsarbeiten und Fortschritte im Bereich Plasma-Astrophysik.

Performance:

Student talks supervised by professors and research assistants.

Target group:

Studierende im Bachelor-, Master- und Diplomstudiengang.

Das Seminar ist für Mitglieder der Arbeitsgruppe Plasma-Astrophysik.

Note:

Das Seminar findet in institutseigenen Räumen statt: Raum ER 373.

Language: German, English on demand.

Seminar: Ausgewählte Themen der Astrophysik

Wichtige Informationen zum Online-Betrieb

Das Seminar wird online stattfinden. Teilnehmer*innen müssen sich bis zum 22. April bei folgender E-Mail Adresse anmelden: schulreichtu-berlin.de. Wie immer ist die Teilnahme für Mitglieder der AG Prof. Breitschwerdt verpflichtend.


Lecturer: Prof. Dr. D. Breitschwerdt
Time: Friday 14-18, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 114, Begin: 2020-04-24 (weekly)
Language: German

Content:

Berichte über laufende Forschungsarbeiten und Fortschritte im Bereich Astronomie und Astrophysik.

Performance:

Student talks supervised by professors and research assistants.

Target group:

Studierende im Bachelor-, Master- und Diplomstudiengang.

Das Seminar ist für Mitglieder der Arbeitsgruppe Astrophysik.

Talks
DayTimeThema
Friday 2020-04-24 14 Semesterbeginn: Seminar-Vorbesprechung
The seminar takes place as a ZOOM video conference
Friday 2020-05-15 14 Lilla Vano: Carbon content and transport in plasmas of the Wendelstein 7-X stellarator
The seminar takes place as a ZOOM video conference
Friday 2020-05-22 14 Yeon Joo Lee: Venus' puzzling clouds
The seminar takes place as a ZOOM video conference
Friday 2020-06-05 14 Frederik Berberich: Numerical studies on the magnetic field structure in the vicinity of superbubbles and the impact of the magnetic field on their dynamical evolution
The seminar takes place as a ZOOM video conference
Friday 2020-06-12 14 Xin Yao: Modification of electron distributions allowing radioastronomical diagnostics of magnetic reconnection
The seminar takes place as a ZOOM video conference
Friday 2020-06-19 14 Felix Pollak: Investigation of Antarctic Micrometeorites and Analysis of their Radionuclide Composition and Cosmic Lifetimes
The seminar takes place as a ZOOM video conference
Friday 2020-06-26 15 Amir Chatraee: Current sheet diagnostics
The seminar takes place as a ZOOM video conference
Friday 2020-07-03 14 Maurice Künicke: Calculating stellar Orbits: A comparison between the theory of epicycles and numerical integrator in GalPy
The seminar takes place as a ZOOM video conference
Friday 2020-07-03 15 Philipp Nelde: Influence of Systematic Errors on the Electron Density and Temperature Measured with Thomson Scattering at W7-X
The seminar takes place as a ZOOM video conference
Friday 2020-07-10 14 Thomas Garmatter: Modellierung der zirkumstellaren Staubhülle des extremen C-Sterns IRAS 07077+1536
The seminar takes place as a ZOOM video conference
Friday 2020-07-10 15 Annabelle Spanier: Characterisation of Neutral Beam Injection into the Wendelstein 7-X Stellarator
The seminar takes place as a ZOOM video conference
Friday 2020-07-17 14 Lucía Navarro: Searches for Dark Matter using Run-2 data from the ATLAS detector
The seminar takes place as a ZOOM video conference
Friday 2020-07-17 15 Illés Lohay: Interior dynamics and thermal evolution of Mars
The seminar takes place as a ZOOM video conference
Friday 2020-07-24 14 Antonius Otto: Magnetic Reconnection
The seminar takes place as a ZOOM video conference

Astrophysikalisches Seminar

Wichtige Informationen zum Online-Betrieb

Das Seminar wird online stattfinden. Ab sofort ist die Anmeldung über das SAP-System möglich. Zusätzlich müssen sich Teilnehmer*innen bis zum 20. April unter der Angabe von:

  • Name, Vorname
  • email-Kontaktadresse
  • Studiengang (ggf. Universität)
  • Matrikelnummer

bei folgender E-Mail Adresse anmelden: schulreichtu-berlin.de.


Lecturer: Prof. Dr. D. Breitschwerdt
Time: Tuesday 14-16, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 114, Begin: 2020-04-21 (weekly)
Language: German

Content:

Ausgewählte Themen aus dem Gebiet der Astronomie und Astrophysik. Vorträge von Studierenden. Betreuung durch Hochschullehrer und Wissenschaftliche Mitarbeiter.

Conditions:

Kenntniss der Vorlesung Grundlagen der Astronomie und Astrophysik erwünscht. Möglichst bereits Besuch der Integrierten Lehrveranstaltungen und / oder weiterführender Vorlesungen.

Performance:

Student talks supervised by professors and research assistants.

Target group:

Studierende, die in Astrophysik einen Seminarschein erwerben wollen. Sonstige Studierende mit Interesse an Astronomie und Astrophysik.

Talks
DayTimeThema
Tuesday 2020-04-21 14 Semesterbeginn: Vorbesprechung und Themenvergabe

Übungen zu Grundlagen der Astronomie und Astrophysik II

Wichtige Informationen zum Online-Betrieb

Die Übungen finden als Online-Lehrveranstaltung statt.

Online-Anmeldung bis 22.04.2020 18 Uhr über das MOSES-Konto: https://moseskonto.tu-berlin.de/moseskonto/

Die Übungen beginnen erst in der 2. Vorlesungswoche.


Lecturer: Prof. Dr. D. Breitschwerdt
Time: Monday 14-16, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 226, Begin: 2020-04-20 (weekly)
Time: Tuesday 12-14, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 226, Begin: 2020-04-21 (weekly)
Time: Tuesday 14-16, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 226, Begin: 2020-04-21 (weekly)
Time: Wednesday 12-14, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 226, Begin: 2020-04-22 (weekly)
Time: Thursday 12-14, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 226, Begin: 2020-04-23 (weekly)
Time: Thursday 16-18, Place: Eugene-Paul-Wigner-Gebäude der TU, Hardenbergstr. 36, EW 114, Begin: 2020-04-23 (weekly)
Language: German

Content:

Aufsuchen astronomischer Objekte, Massenbestimmung von Doppelsternen, Klassifikation von Sternspektren, Bestimmung der Entfernung und des Alters von Sternhaufen, Sternstromparallaxe der Hyaden, Beobachtungen am Teleskop, Entfernungsbestimmung extragalaktischer Objekte (Cepheidenmethode).

Conditions:

Knowledge of mathematics and physics.

Performance:

Two-hour tutorial. Teamwork (small groups) on different exercises.

Target group:

Übungen für Studierende, die das Modul Grundlagen der Astronomie und Astrophysik zusammen mit der Vorlesung Grundlagen der Astronomie und Astrophysik II im Bachelor-Studiengang wählen.

Note:

Begrenzte Anzahl der Übungsplätze!

Online-Anmeldung bis 14.04.2020 18 Uhr über das MOSES-Konto: https://moseskonto.tu-berlin.de/moseskonto/

Übungen beginnen erst in der zweiten Vorlesungswoche.

Die Lehre am Zentrum (Neufassung)

Hinweis

Nachweise über erbrachte Studienleistungen/Scheine erhält man für alle vom Zentrum für Astronomie und Astrophysik verantwortlich an TU und an FU betreuten Lehrveranstaltungen nur im Sekretariat (Frau Kieschke) des Zentrums.

Sekretariatsadresse:

Technische Universität Berlin
Zentrum für Astronomie und Astrophysik
Sek. EW 8-1
Hardenbergstr. 36
10623 Berlin

Tel.: 314-23734
Raum: EW 818 (8. Stock - Fahrstuhl am Pförtneraufgang nehmen!)

Solar eruptions, numerical simulation and laboratory experiments

Simulation
Simulation
Lupe
Simulation
Labor
Lupe

Prof. Dr. Jörg Büchner
(Max-Planck-Institut für Sonnensystemforschung, Göttingen)
Freitag/Friday, 2015-12-18, 14 c.t., EW-561
Eugene-Paul-Wigner Gebäude, Hardenbergstr. 36, 10623 Berlin

Zusammenfassung/Abstract:The Sun releases its thermonuclear energy not only in form of the well know and a seemingly constant flow of white light but also by a highly variable stream of non-visible electromagnetic radiation, by plasma flows and energetic particles. Altogether these energy flows form the external environmental conditions for the planet Earth now called the "Space Weather". The Space Weather conditions are highly variable - even more than the atmospheric weather conditions. The reason is that the sources of the Space Weather are eruptive energy releases from the Sun with the most prominent Solar Flares and called Coronal Mass Ejections (CMEs). The increasing social relevance of the Space Weather conditions has recently led to intensive efforts to understand of the reason of solar eruptions. We present the main existing models of solar eruptions as they actually are under development and demonstrate their verification by means of numerical simulations directly comparable with solar observations. We further compare these findings with the results of current laboratory eruption experiments carried out at the Princeton Plasma Physics Laboratory (MRX).

From darkness to light – the emergence of star clusters from molecular clouds

ALMA
Lupe

Dr. James Dale
(Universitäts-Sternwarte München, Ludwig-Maximilians-Universität)
Dienstag/Tuesday, 2015-11-24 14:00 c.t., Raum EW-114
Eugene-Paul-Wigner Gebäude, Hardenbergstr. 36, 10623 Berlin

Zusammenfassung/Abstract:

The most important stage of a star cluster’s life is that in which it emerges from the molecular cloud in which it formed, and becomes optically visible. Over a short timescale, residual gas is expelled from the cluster, the remains of the cloud are dispersed, star formation is terminated, and the embedded stellar population, previously visible only in the infrared, becomes optically bright. I will present numerical simulations of this complex process, compare them with the latest observational results and discuss the implications of the current state of this field for the global star formation process.

Modelling the stellar winds from hot and cool stars

NGC 7635 (The Bubble Nebula) - A strong stellar wind and intense radiation from a star has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud.
NGC 7635 (The Bubble Nebula) - A strong stellar wind and intense radiation from a star has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud.
Lupe

Dr. Jonathan Mackey
(Argelander-Institut für Astronomie, Universität Bonn)
Dienstag/Tuesday, 2014-12-09 14:00 c.t., EW 229
Eugene-Paul-Wigner Gebäude, Hardenbergstr. 36, 10623 Berlin

Zusammenfassung/Abstract:
Mass loss from massive stars is very important for determining their evolution and death, but their wind properties can be difficult to measure and are often very uncertain.

Main sequence massive stars have fast and highly ionized winds, driving bubbles in their surroundings that have proven surprisingly difficult to detect. We have run simulations showing that wind bubbles are typically very asymmetric and do not fill their HII regions.

Coalescence of intermediate-mass black holes: Implications for GW Astronomy

 LIGO Scientific Collaboration (LSC) / NASA
An artist's representation of the burst of gravitational waves resulting from the collision of a colliding pair of black holes.
Lupe

Dr. Pau Amaro-Seoane
(AEI Potsdam-Golm)
Freitag/Friday, 2014-12-05, 14:00 c.t., EW 561
Eugene-Paul-Wigner Gebäude, Hardenbergstr. 36, 10623 Berlin

Zusammenfassung/Abstract:
Observations suggest that star clusters often form in binaries or larger bound groups. Therefore, mergers between two clusters are likely to occur. If these clusters both harbour an intermediate-mass black hole (IMBH; ~100-10,000 M$_\odot$) in their center, they can become a strong source of gravitational waves when the black holes merge with each other.

Neue Übungstermine im SS 2012 zu Grundlagen der Astronomie und Astrophysik

Für die Übungen zu Grundlagen der Astronomie und Astrophysik im SS 2012 gelten die folgenden Termine:

TU Übungstermine SS 2012
Tag Zeit Raum  
Di 10-12 EW 015    (neuer Raum)
Di 12-14 EW 226  
Di 14-16 EW 229  
Mi 16-18 EW 114  
Do 12-14 EW 226  
Do 14-16 EW 246  
Do 16-18 EW 114  
Fr 10-12 EW 114    (neu)

Zusatzinformationen / Extras