Applications for the 2021 Kavli Summer Program in Astrophysics are now open (deadline for students February 19th).
The Kavli Summer Program in Astrophysics normally runs for six weeks every summer in alternance between various institutions world-wide and UC Santa Cruz. It involves up to 15 established faculty and 15 graduate students, as well as additional postdoctoral and senior scientists who contribute to the supervision of the research students.… continue to the full article
We are pleased to announce that pre-registration for the Solar Orbiter school at Ecole de Physique des Houches (April 6th-9th 2021) is now open at https://solarorbiter.sciencesconf.org .
While we are still facing an on-going worldwide pandemic, the conference center may open but only to a very limited amount of participants.… continue to the full article
First announcement of the Solar Orbiter school at Ecole de Physique des Houches (France)
We are pleased to announce that we are organising a school dedicated to Solar Orbiter, to be held at the Ecole de Physique des Houches, April 6th-9th (2021).… continue to the full article
Registration is now open for an STFC-funded summer school on the Solar-Stellar Connection.
The summer school will run online between 14th-18th September 2020. Registration is free and the deadline to register is 31st August 2020.
More details can be found here: https://warwick.ac.uk/stellar_school
Our summer school aims to cover topics from solar and stellar interiors, through solar/stellar atmospheres, and out into interplanetary space and the interactions between stars and planets.… continue to the full article
https://www.birmingham.ac.uk/research/activity/physics/astronomy/stfc-intro-2020/index.aspx
Registration for this year’s introductory School, which will be delivered online, is now open. To register, please visit:
https://www.birmingham.ac.uk/research/activity/physics/astronomy/stfc-intro-2020/registration.aspx
Registration is free for all delegates.
The School will provide young researchers with introductory lectures covering the key areas and latest results from across the discipline, with core content agreed by the UK Solar Physics (UKSP) and Magnetosphere, Ionosphere and Solar-Terrestrial (MIST) communities.… continue to the full article
Online Summer School for Time Domain Science
Applications are now being accepted for the online GROWTH astronomy school “The Dynamic Universe at all Wavelengths”. The school will include live webinars and interactive virtual workshops scheduled on Aug 17-21, 2020.
This school is designed for graduate and advanced undergraduate students with strong research interests in time-domain astronomy.… continue to the full article
This year’s STFC Introductory Summer School will be an online meeting.
It was due take place in Birmingham from 24 – 28 August. However, owing to COVID-19, an in-person meeting is no longer possible (University restrictions mean we can no longer run face-to-face conferences/events at that time).… continue to the full article
SOLARNET school “High-resolution Solar Physics”
Date & Venue: August 31 – September 4, 2020 at Institute of Physics, University of Graz, Univ.-Platz 5 8010 Graz, Austria
The Sun is the only star where fine structures down to sizes below 100 km can be observed directly.… continue to the full article
Date & Venue: March 23-27, 2020 at UCL – Mullard Space Science Laboratory (Dorking, UK)
The school aims towards the introducing the approaches and analysis methods needed to successfully combine space and ground-based observations of the solar atmosphere from the photosphere to the corona, to provide a complete understanding of the underlying physical processes occurring in a range of different solar phenomena.… continue to the full article
Date & Venue: March 23-27, 2020 at UCL – Mullard Space Science Laboratory (Dorking, UK)
The school “A holistic view of the solar atmosphere – combining space and ground-based observations” has for a goal to provide an introduction to the approaches and analysis methods needed to successfully combine space and ground-based observations of the solar atmosphere from the photosphere to the corona, in order to a complete view of the underlying physical processes at work in a range of different solar phenomena.… continue to the full article