BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Machine Learning: The elegant way to extract information from data
DTSTART;VALUE=DATE-TIME:20170213T090000Z
DTEND;VALUE=DATE-TIME:20170223T110000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-30@cern.ch
DESCRIPTION:The human brain is able to recognize patterns in the data due 
 to the millions of years of evolution. Today\, we try to use and further d
 evelop computer algorithms that can reproduce this ability to distinguish 
 patterns in large statistical samples and images\, to find correlations be
 tween events\, to classify objects based on their similar and different fe
 atures in an objective and automatic way. Machine Learning is a subfield i
 n computer science that explores pattern recognition in the data analysis 
 and characterize already known trends in sets of observations.\n\nThis cou
 rse focuses on the basic most applied up-to-date techniques in the machine
  learning that can be used in any branch of science and industry. We start
  with a broad introduction about the topic\, followed by detailed discussi
 on about the theory and application of the different types of the machine 
 learning — supervised and unsupervised learning. In the field of supervi
 sed learning\, for example\, we will discuss regression\, support vector m
 achines\, and neural networks\, while the field of unsupervised learning w
 e will cover clustering techniques\, principal component analysis\, and di
 mensionality reduction.\n\nThe final goal of the course is to give the han
 ds–on knowledge needed to pick and apply machine learning tools in Pytho
 n. Discussions of the underlying mathematical principles will illustrate t
 he inner workings of these tools.\n\nThis course forms part of the series 
 of Black Board Lectures offered at the International Max Planck Research S
 chool (IMPRS) of Astronomy and Astrophysics hosted by the Max–Planck–I
 nstitute for Radioastronomy. Please also consult the course homepage at th
 e IMPRS website.\n\nhttps://events.mpifr-bonn.mpg.de/indico/event/30/
LOCATION:
URL:https://events.mpifr-bonn.mpg.de/indico/event/30/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Dynamics of Star Clusters Containing Stellar Mass Black Holes
DTSTART;VALUE=DATE-TIME:20170725T080000Z
DTEND;VALUE=DATE-TIME:20170728T130000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-51@cern.ch
DESCRIPTION:Hyung Mok Lee (Seoul National University)\n\n​\n\nLIGO has d
 etected three gravitational wave events due to the merger of black hole bi
 naries. The black hole binaries could have formed through the evolution of
  binaries composed of massive stars. However\, such binaries could have be
 en formed in globular clusters purely by the dynamical processes because o
 f high stellar density. Also globular clusters are very old objects with l
 ow metallicity. Among three black hole binaries\, two are known to have be
 en composed of relatively massive ones. Such a massive black holes can be 
 formed in low metallicity environment.  In the presence of massive compon
 ents such as black holes\, the mass segregation could take place rapidly\,
  forming very dense core purely composed of black holes. Binaries of black
  holes can form either three-body or two-body processes. Under typical phy
 sical conditions of the central parts of the globular clusters\, three-bod
 y processes are thought to be more efficient. The binaries formed via thre
 e-body processes are relatively wide and the time scale for the binaries t
 o merge would be much longer than Hubble time. However\, the close interac
 tions between binaries and single black holes make the orbits tighter. Suc
 h a tightening of binary orbit continues until the binaries get ejected si
 nce the recoil energy per interaction increases as the orbit becomes small
 er. Some fraction of the ejected binaries eventually will undergo merger w
 ithin Hubble time. This lecture intends to provide an overview of the grav
 itational waves\, dynamical evolution of dense stellar systems\, formation
  processes of binaries in high density regions\, and the interaction betwe
 en binaries and singles.\n\n \n\nTopics to be covered:\n\n\n	Introduction
  - Gravitational Waves\n	Dynamical evolution driven by two-body relaxation
 \n	Methods of stellar dynamics\n	Formation Processes of Binary Stars\n	Clo
 se interaction of stars with binaries\n\n\n​\n\nhttps://events.mpifr-bon
 n.mpg.de/indico/event/51/
LOCATION:MPIfR 0.01 and 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/51/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Astronomical Instruments: How they work\, how they are planned\, b
 uilt and tested
DTSTART;VALUE=DATE-TIME:20180122T100000Z
DTEND;VALUE=DATE-TIME:20180124T113000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-62@cern.ch
DESCRIPTION:Carlos Durán\, Engineer and IMPRS Researcher\n\nDay 1 (10:00 
 – 11:15  +  11:30 – 12:45)\n\n1. Drivers for a telescope (and instru
 mentation)\n\n\n	Scientific Interest        \n	Technology    \
 n	Interface and Specification.\n	Project Management\n\n\n2. Constraints\, 
 limitations and barriers\n\n\n	Technology & technics\n	Site (Atmosphere)\n
 	Money\n	Logistics & Operation\n	Competitors / use.\n\n\n3. Telescopes and
  configurations\n\n\n	Single Dish / Arrays\n	Ground-base / Air- Balloon bo
 rned / Space   \n\n\n4. Testing\, Commissioning and Acceptance.\n\n\n	K
 ey concepts\n\n\n5. Operation: The non-visible backstage.\n\n\n	Data Handl
 ing\, Calibration and Archiving\n	Surface accuracy and efficiencies\n	Poin
 ting and Atmospheric models\n	Power\n	Cryogenics\n\n\nDay 2 (10:00 – 11:
 15  +  11:30 – 12:45)\n\n1. Receiver Technology used in (Radio) Astron
 omy\n\n\n	Front-end\n	\n		Heterodynes (single pixel and arrays)\n		Calorim
 eters / Bolometers\n	\n	\n	Backends\n	\n		Spectrometers: AOS / FFTs\n		Cor
 relators (Auto and Cross)\n		ADC and Total power detectors.\n	\n	\n\n\n2. 
 The need of low temperature: Cryostat and Cryogenics\n\n3. (Quasi) Optics\
 , Telescope Coupling and interfacing.\n\n4. The design of an instrument.\n
 \n            Modeling and simulations\n\n          
   Selection of Components\n\n            Optics Design (Mirror
 s\, filters\, windows\, etc)\n\n            Mechanical design\n
 \n            Electronics and Electrical Interfacing\n\n   
          Software\n\n5. Tune up\, characterization and commissioni
 ng\n\n            Lab Tests and Operation points\n\n     
        Merit figures: Allan Variance\, T_Rec\, Thermo/mech. Stabilit
 ies. Uncertainties\n\n            Commissioning.\n\nDay 3. 10:0
 0 -11:00 \n\nVisit to the GREAT / SOFIA Lab (1.39) at MPIfR.\n\n \n\n \n
 \n \n\nhttps://events.mpifr-bonn.mpg.de/indico/event/62/
LOCATION:MPIfR 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/62/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tools of Radio Astronomy: Problems and solutions
DTSTART;VALUE=DATE-TIME:20190115T100000Z
DTEND;VALUE=DATE-TIME:20190214T110000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-106@cern.ch
DESCRIPTION:Thomas L. Wilson\, MPIfR\n\nBased of his book "Tools of Radio 
 Astronomy: Problems and solutions"\, Tom Wilson will illustrate radioastro
 nomical methods and concepts by showing the audience how to solve typical 
 radio astronomical problems\, and thus extract the information you need fr
 om your observations. The book will be made available to IMPRS researchs e
 lectronically: https://link.springer.com/book/10.1007%2F978-3-319-90820-5\
 n\n \n\n \n\n \n\n \n\n \n\nhttps://events.mpifr-bonn.mpg.de/indico/e
 vent/106/
LOCATION:MPIfR Library
URL:https://events.mpifr-bonn.mpg.de/indico/event/106/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Tools of Radio Astronomy: Problems and solutions
DTSTART;VALUE=DATE-TIME:20190115T100000Z
DTEND;VALUE=DATE-TIME:20190214T110000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-130@cern.ch
DESCRIPTION:Thomas L. Wilson\, MPIfR\n\nBased of his book "Tools of Radio 
 Astronomy: Problems and solutions"\, Tom Wilson will illustrate radioastro
 nomical methods and concepts by showing the audience how to solve typical 
 radio astronomical problems\, and thus extract the information you need fr
 om your observations. The book will be made available to IMPRS researchs e
 lectronically: https://link.springer.com/book/10.1007%2F978-3-319-90820-5\
 n\n \n\n \n\n \n\n \n\n \n\nhttps://events.mpifr-bonn.mpg.de/indico/e
 vent/130/
LOCATION:MPIfR Library
URL:https://events.mpifr-bonn.mpg.de/indico/event/130/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Statistical Inference: Frequentist\, Bayesian and Likelihood analy
 sis
DTSTART;VALUE=DATE-TIME:20190715T090000Z
DTEND;VALUE=DATE-TIME:20190715T130000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-132@cern.ch
DESCRIPTION:Dr. María Paz Casanova Laudien\, Director of the Statistics D
 ept. at the University of Concepción\, Chile\n\nJuly 15th from 11 - 15h w
 ith 1h lunch break from 12:30-13:30 h\n\nThe first part will be on theory 
 and the second part on practise.\n\nhttps://events.mpifr-bonn.mpg.de/indic
 o/event/132/
LOCATION:AIfA Lecture Hall
URL:https://events.mpifr-bonn.mpg.de/indico/event/132/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Astronomical Instruments: How they work\, how they are planned\, b
 uilt and tested
DTSTART;VALUE=DATE-TIME:20191203T100000Z
DTEND;VALUE=DATE-TIME:20191205T113000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-139@cern.ch
DESCRIPTION:Dr. Carlos Durán\, Engineer\n\nDay 1 (10:00 – 11:15  +  1
 1:30 – 12:45)\n\n1. Drivers for a telescope (and instrumentation)\n\n\n	
 Scientific Interest        \n	Technology    \n	Interface and S
 pecification.\n	Project Management\n\n\n2. Constraints\, limitations and b
 arriers\n\n\n	Technology & technics\n	Site (Atmosphere)\n	Money\n	Logistic
 s & Operation\n	Competitors / use.\n\n\n3. Telescopes and configurations\n
 \n\n	Single Dish / Arrays\n	Ground-base / Air- Balloon borned / Space  
  \n\n\n4. Testing\, Commissioning and Acceptance.\n\n\n	Key concepts\n\n\
 n5. Operation: The non-visible backstage.\n\n\n	Data Handling\, Calibratio
 n and Archiving\n	Surface accuracy and efficiencies\n	Pointing and Atmosph
 eric models\n	Power\n	Cryogenics\n\n\nDay 2 (10:00 – 11:15  +  11:30 
 – 12:45)\n\n1. Receiver Technology used in (Radio) Astronomy\n\n\n	Front
 -end\n	\n		Heterodynes (single pixel and arrays)\n		Calorimeters / Bolomet
 ers\n	\n	\n	Backends\n	\n		Spectrometers: AOS / FFTs\n		Correlators (Auto 
 and Cross)\n		ADC and Total power detectors.\n	\n	\n\n\n2. The need of low
  temperature: Cryostat and Cryogenics\n\n3. (Quasi) Optics\, Telescope Cou
 pling and interfacing.\n\n4. The design of an instrument.\n\n      
       Modeling and simulations\n\n            Selection of
  Components\n\n            Optics Design (Mirrors\, filters\, w
 indows\, etc)\n\n            Mechanical design\n\n      
       Electronics and Electrical Interfacing\n\n          
   Software\n\n5. Tune up\, characterization and commissioning\n\n    
         Lab Tests and Operation points\n\n            Me
 rit figures: Allan Variance\, T_Rec\, Thermo/mech. Stabilities. Uncertaint
 ies\n\n            Commissioning.\n\nDay 3. 10:00 -11:00 \n\nVi
 sit to the GREAT / SOFIA Lab (1.39) at MPIfR.\n\n \n\n \n\n \n\nhttps:/
 /events.mpifr-bonn.mpg.de/indico/event/139/
LOCATION:MPIfR 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/139/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Principles and tools of statistics\, data analysis and machine lea
 rning: I. Statistics
DTSTART;VALUE=DATE-TIME:20220408T120000Z
DTEND;VALUE=DATE-TIME:20220428T140000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-239@cern.ch
DESCRIPTION:This course focuses on the basic most applied up-to-date techn
 iques in statistics\, data analysis\, and machine learning that can be use
 d in any branch of science and industry. The first block course will intro
 duce you to the principles of statistics.\n\nThe final goal of the course 
 is to give the hands–on knowledge needed to pick and apply statistics\, 
 data analysis and machine learning tools in Python. Discussions of the und
 erlying mathematical principles will illustrate the inner workings of thes
 e tools.\n\nThis course forms part of the series of Black Board Lectures o
 ffered at the International Max Planck Research School (IMPRS) of Astronom
 y and Astrophysics hosted by the Max–Planck–Institute for Radioastrono
 my.\n\nA certificate will be provided to all participants who successfully
  participate in the lectures\, exercises\, and homework exercises.\n\nWebp
 age: https://www3.mpifr-bonn.mpg.de/staff/gwitzel/Teaching.html\n\nhttps:
 //events.mpifr-bonn.mpg.de/indico/event/239/
LOCATION:
URL:https://events.mpifr-bonn.mpg.de/indico/event/239/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Astronomical Instruments: How they work\, how they are planned\, b
 uilt and tested
DTSTART;VALUE=DATE-TIME:20221004T080000Z
DTEND;VALUE=DATE-TIME:20221006T110000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-286@cern.ch
DESCRIPTION:Dr. Carlos Durán\, Station Manager of the APEX telescope\n\nD
 ay 1 (4. October 2022 10:00 – 11:15  +  11:30 – 12:45)\n\n1. Drivers
  for a telescope (and instrumentation)\n\n\n	Scientific Interest     
    \n	Technology    \n	Interface and Specification.\n	Project Manag
 ement\n\n\n2. Constraints\, limitations and barriers\n\n\n	Technology & te
 chnics\n	Site (Atmosphere)\n	Money\n	Logistics & Operation\n	Competitors /
  use.\n\n\n3. Telescopes and configurations\n\n\n	Single Dish / Arrays\n	G
 round-base / Air- Balloon borned / Space   \n\n\n4. Testing\, Commissio
 ning and Acceptance.\n\n\n	Key concepts\n\n\n5. Operation: The non-visible
  backstage.\n\n\n	Data Handling\, Calibration and Archiving\n	Surface accu
 racy and efficiencies\n	Pointing and Atmospheric models\n	Power\n	Cryogeni
 cs\n\n\nDay 2 (6. October 202210:00 – 11:15  +  11:30 – 12:45)\n\n1.
  Receiver Technology used in (Radio) Astronomy\n\n\n	Front-end\n	\n		Heter
 odynes (single pixel and arrays)\n		Calorimeters / Bolometers\n	\n	\n	Back
 ends\n	\n		Spectrometers: AOS / FFTs\n		Correlators (Auto and Cross)\n		AD
 C and Total power detectors.\n	\n	\n\n\n2. The need of low temperature: Cr
 yostat and Cryogenics\n\n3. (Quasi) Optics\, Telescope Coupling and interf
 acing.\n\n4. The design of an instrument.\n\n            Modeli
 ng and simulations\n\n            Selection of Components\n\n 
            Optics Design (Mirrors\, filters\, windows\, etc)\n\n
             Mechanical design\n\n            Electro
 nics and Electrical Interfacing\n\n            Software\n\n5. T
 une up\, characterization and commissioning\n\n            Lab 
 Tests and Operation points\n\n            Merit figures: Allan 
 Variance\, T_Rec\, Thermo/mech. Stabilities. Uncertainties\n\n      
       Commissioning.\n\n \n \n\n\n \n\n \n\nhttps://events.mpifr-
 bonn.mpg.de/indico/event/286/
LOCATION:MPIfR 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/286/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (1/6)
DTSTART;VALUE=DATE-TIME:20230228T073000Z
DTEND;VALUE=DATE-TIME:20230228T100000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-300@cern.ch
DESCRIPTION:1) Stationary Processes\n\n\n	Stationarity\n	Autocovariance an
 d autocorrelation functions\n	Use of the autocorrelation function\n	Gaussi
 an processes and forward modeling\n	Autoregressive and moving average proc
 esses\n\n\n2) Spectral Analysis\n\n\n	The Fourier transform\n	Spectral Ana
 lysis of stationary processes\n	Spectral density\, autocovariance and auto
 correlation functions\n	Filter relationships\n\n\n3) Estimation in time an
 d frequency domain\n\n4) Practical spectral analysis\n\n\n	Aliasing and ch
 oice of window\n	DFTs -Lomb-Scargle priodograms\n	Phase dispersion minimis
 ation\n\n\nhttps://events.mpifr-bonn.mpg.de/indico/event/300/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/300/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (2/6)
DTSTART;VALUE=DATE-TIME:20230228T120000Z
DTEND;VALUE=DATE-TIME:20230228T150000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-301@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/301/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/301/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (3/6)
DTSTART;VALUE=DATE-TIME:20230301T073000Z
DTEND;VALUE=DATE-TIME:20230301T103000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-302@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/302/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/302/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (4/6)
DTSTART;VALUE=DATE-TIME:20230301T120000Z
DTEND;VALUE=DATE-TIME:20230301T150000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-303@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/303/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/303/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (5/6)
DTSTART;VALUE=DATE-TIME:20230302T073000Z
DTEND;VALUE=DATE-TIME:20230302T103000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-304@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/304/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/304/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Practical Time Series Analysis (6/6)
DTSTART;VALUE=DATE-TIME:20230302T120000Z
DTEND;VALUE=DATE-TIME:20230302T150000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-305@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/305/
LOCATION:MPIfR Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/305/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Turbulence and dynamos for astrophysicists (1/5)
DTSTART;VALUE=DATE-TIME:20230703T080000Z
DTEND;VALUE=DATE-TIME:20230703T100000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-328@cern.ch
DESCRIPTION:This is a 5 part black board lecture on Turbulence by Prof. An
 var Shukurov. This lecture was presented already in 2016 and had a very po
 sitiv resonance among our students. We are glad that Prof. Shukurov willin
 g to hold this lecture again\, this year with an additional part on dimens
 ional analysis.\n\nThe lecture will be presented in hybrid format and also
  include some exercises and problems. \n\nLecture hours have been extended
  with additional sessions so that the material can be presented in a more 
 understandable and less rushed manner.\n\n \n\nThe extended times for the
  lecture are now\n\n \n\nMonday\, 10-12 and 15-16\n\nTuesday\, 09-11 and 
 15:30-16:30\n\nWednesday 10-12 and 13-14\n\nThursday\, 10-12 and 13-14\n\n
 Friday\, 14-17\n\n \n\nPlease regsiter in advance so we get an overview h
 ow many participants we can expect!\n\n \n\nSyllabus (tentative)\n\nIntro
 duction\n\n\n	Turbulence and its defining features\n	Significance of turbu
 lence\n\n\nElements of random functions\n\n\n	Ensemble\, volume and time a
 veraging\n	The Reynolds rules of averaging\n	Correlation and structure fun
 ctions\n	Stationary random functions\n	Spectral representation\n	Correlati
 on versus statistical dependence\n\n\nDimensional analysis [New]\n\nPhenom
 enology of fluid turbulence\n\n\n	Energy conservation\n	Spectral energy tr
 ansfer\n	The Reynolds number\n	Kolmogorov's theory\n	Turbulent diffusion\n
 \n\nInterstellar turbulence\n\n\n	Energy sources\n	Turbulence driven by su
 pernovae\n	Observational signatures\n	Parameters of interstellar turbulenc
 e\n	The role of turbulence in galaxies\n\n\nMagnetohydrodynamic turbulence
 \n\n\n	Isotropic Alfven wave turbulence\n	Anisotropic Alfven wave turbulen
 ce\n\n\nTurbulent dynamos\n\n\n	The induction equation\n	The necessity of 
 dynamo action in astrophysics\n	Fast and slow dynamos\n	Turbulent dynamos\
 n	Mean-field dynamos in galaxies\n	Fluctuation dynamos\n	Seed magnetic fie
 lds\n\n\nhttps://events.mpifr-bonn.mpg.de/indico/event/328/
LOCATION:Max Planck Insitute for Radio Astronomy Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/328/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Turbulence and dynamos for astrophysicists (2/5)
DTSTART;VALUE=DATE-TIME:20230704T070000Z
DTEND;VALUE=DATE-TIME:20230704T090000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-329@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/329/
LOCATION:Max Planck Insitute for Radio Astronomy Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/329/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Turbulence and dynamos for astrophysicists (3/5)
DTSTART;VALUE=DATE-TIME:20230705T080000Z
DTEND;VALUE=DATE-TIME:20230705T100000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-330@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/330/
LOCATION:Max Planck Insitute for Radio Astronomy Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/330/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Turbulence and dynamos for astrophysicists (4/5)
DTSTART;VALUE=DATE-TIME:20230706T080000Z
DTEND;VALUE=DATE-TIME:20230706T100000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-331@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/331/
LOCATION:Max Planck Insitute for Radio Astronomy Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/331/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Turbulence and dynamos for astrophysicists (5/5)
DTSTART;VALUE=DATE-TIME:20230707T120000Z
DTEND;VALUE=DATE-TIME:20230707T140000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-332@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/332/
LOCATION:Max Planck Insitute for Radio Astronomy Auditorium 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/332/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Lecture: Manifestations and Physics of Galactic Winds and Outflows
  (1/2)
DTSTART;VALUE=DATE-TIME:20240904T120000Z
DTEND;VALUE=DATE-TIME:20240904T140000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-412@cern.ch
DESCRIPTION:The lecture is held in two parts. 1st part on Wednesday\, 2nd 
 part on Thursday.\n\nBy registering you agree to be listed as participant 
 here on the event page.\n\n\nOutline:\n\n1. Manifestations of Galactic Out
 flows\n\n\n	emphasis on Milky Way\, but the physics is applicable to all G
 alaxies at all redshifts\n	observed features\n	\n		bipolar outflow on 10-p
 c scale\n		 the Galactic center chimneys\, radio an X-ray - large-scale s
 ynchrotron radio features\n		Fermi Bubbles\n		eRosita Bubbles\n	\n	\n\n\n2
 . Sources of gas outflow from galaxies\n\n\n	AGNs: jets versus winds\n	tid
 al disruption events\n	star formation\, —> supernovae\n	collective super
 novae\n\n\n3. The Galactic wind\n\n\n	broad angular distribution relative 
 to Galactic center\n	entrained neutral gas clumps as best evidence\n	fate 
 of dense gas clumps: disintegration or growth\n	\n		ablation\n		instabilit
 ies: Rayleigh-Taylor\, Kelvin-Helmholtz\n		compression —> enhanced cooli
 ng\, density growth\n	\n	\n\n\n4. Determinants of the expansion rate of ou
 tflows\n\n\n	initial ejection velocity\, if any\n	temperature (sound speed
 ) —> adiabatic expansion\n	\n		plasma cooling time versus expansion time
 \n	\n	\n	gravitational deceleration\n	shocks with ambient gas\, mass loadi
 ng\n\n\n5. The Galactic Magnetic Field\n\n\n	a collimator for the wind\n	\
 n		versus collimation caused by Galactic density gradient\n	\n	\n	magnetic
  pressure versus ram pressure versus gas pressure how strong does the fiel
 d need to be?\n\n\n6. Relativistic gas —> Cosmic Rays\n\n\n	acceleration
  mechanisms\n	diffusion\n	role of magnetic fields\n	anisotropy of diffusio
 n coefficients\n	synchrotron emission\n	application to Fermi Bubbles\n\n\n
 7. Interaction with the Galactic halo\n\n\n	shocks\n	sharp bubble edges: q
 uasi-steady shock or surface moving in response to energy injection?\n	wha
 t goes up must come down: the Galactic fountain\n	\n		cooling instabilitie
 s\n	\n	\n\n\n \n\nhttps://events.mpifr-bonn.mpg.de/indico/event/412/
LOCATION:MPIfR 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/412/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Lecture: Manifestations and Physics of Galactic Winds and Outflows
  (2/2)
DTSTART;VALUE=DATE-TIME:20240905T120000Z
DTEND;VALUE=DATE-TIME:20240905T140000Z
DTSTAMP;VALUE=DATE-TIME:20260314T132500Z
UID:indico-event-413@cern.ch
DESCRIPTION:https://events.mpifr-bonn.mpg.de/indico/event/413/
LOCATION:MPIfR 0.02
URL:https://events.mpifr-bonn.mpg.de/indico/event/413/
END:VEVENT
END:VCALENDAR