About the venue

Alma Mater Chiloniensis, Kiel's university, was founded with a ceremony at Nikolaikirche (Church of St Nicholas) on Monday, 5 October 1665. Soon after, the university took on the name of its founder and has since been known as Christian-Albrechts-Universität zu Kiel (CAU). The number of students at the university is approximately 24 000, and the range of subjects offered cover economics, the natural sciences, agriculture, engineering, and science of education. In the former workplace of Max Planck and Heinrich Hertz, a teaching staff of 600 passes on their knowledge to students from Germany and more than a hundred other countries. The lectures will take place at the physics department.


Kiel is the state capital of Schleswig-Holstein, the northernmost state of Germany, between Denmark and Hamburg. Schleswig-Holstein is the land between the seas, it is located between the North Sea and the Baltic Sea. Kiel is at the east end of the Kiel Canal, the world's busiest artificial waterway, which connects the Baltic Sea with the North Sea. As a major harbor, Kiel is the home of the Gorch Fock, a tall ship of the German Navy.

Kiel is also the home of the largest sailing event in the world, the Kieler Woche which takes place every year at the end of June.

Besides sailing (Olympic Games 1936 and 1972), Kiel is also famous for Handball (German record Champion THW Kiel), soccer (German Champion 1912 Holstein Kiel), football (German Champion 2010), smoked fish (Kieler Sprotten) and the uniform of D. Duck (Kieler Anzug).

Application must be addressed at This email address is being protected from spambots. You need JavaScript enabled to view it.
(Further Information at wiki.hesperia-space.eu )

Understanding Solar Eruptions and Extreme Space Weather Events – The physics behind
HESPERIA Summer school
August 29, 2016 to September 2, 2016
Christian-Albrechts-Universität, Kiel, Germany


The Sun is both a source of all life and significant hazards. Solar energetic particle (SEP) events provoke extreme space weather. While not noticeable by humans on Earth, space weather caused radiation is a hazard for satellites, for the astronauts onboard the International Space Station (ISS), and in extreme cases for the aircrew on polar flights. But energetic particles are also of general astrophysical interest. Supernova remnants, pulsars, active galactic nuclei can only be seen because these objects accelerate particles. So does the Sun. Solar particles can not only be observed through their electromagnetic emission, but they can also be directly measured in space as SEP events and in extreme cases as ground level enhancements. We see their time evolution and can use it to constrain the acceleration processes. Therefore, scientists observe SEP events and incorporate methods to know or even forecast the radiation hazard associated with them.

Educational Objectives

The HESPERIA course at the Christian-Albrechts-Universität provides an introduction to the physics of the active corona, the variable solar wind including the interplanetary field embedded in, the acceleration and transport of energetic particles as well as their transport through the Earth magneto- and atmosphere and radiation effects. The lectures include a variety of interesting phenomena observed on the Sun and in interplanetary space.


Students will attend a variety of lectures on space physics and research topics related to space weather and will gain valuable hands-on experience under the mentorship of a HESPERIA scientist. This program also provides students with opportunities to develop their written communication skills, by presenting their research in a formal report at the end of the summer school.


The school is open to 25 graduate students currently enrolled in astro or space physics, planetary sciences, space engineering or a related field. Program acceptance is based primarily on the student’s academic record and nomination letter. Acceptance will also be based on the student's interest in attending the summer school and the benefit to the student of attendance, as demonstrated in the cover letter. Application must be addressed at This email address is being protected from spambots. You need JavaScript enabled to view it. . Further information at wiki.hesperia-space.eu.

Important Dates and Deadlines

1.    31.01.2016: Start of applications
2.    30.04.2016: Deadline for application
3.    30.04.2016: Deadline for support
4.    15.05.2016: Support application assignment and rating
5.    29.08.2016: Summer school starts
6.    02.09.2016; Summer school ends


We will provide free accommodation in a students guest house and daily allowance to cover local expenses. Traveling support can be arranged for a few cases.

Please include the following material with your application:

1.    Cover letter describing your research interests, why it would benefit you to attend
2.    Current CV including full list of publications and presentations
3.    Undergraduate transcripts
4.    Nomination letter from your advisor


•    Dr. Olga Malandraki (NOA): Introduction to the HESPERIA Project
•    Prof. Rami Vainio (University of Turku): Particle acceleration
•    Dr. Neus Agueda (University of Barcelona): Particle transport in the interplanetary medium
•    Dr. Ludwig Klein (Observatoire de Paris): The solar corona and non thermal radiation
•    Dr. Rolf Bütikofer (University of Bern): Particle transport in the Earth' magneto- and atmosphere
•    Prof. Bernd Heber (Christian-Albrechts-University Kiel): In-situ measurements of solar energetic particles

Researcher's night in Athens, 25 September 2015

Card 1

Card 2

HESPERIA workshop Paris, Feb 27 – Mar 2, Paris Observatory Schedule


Monday February 27

14:00 Opening
14:15 O. Malandraki: The HESPERIA project: an overview
14:30 C. Sarlanis: The HESPERIA host server set-up
15:00 N. Vilmer: The FLARECAST project
15:30 I. Usoskin: Extreme solar particle events: What is the worst case scenario?

16:15 Coffee break

SEP Forecasting (1)

16:45  A. Papaioannou: SEP Data driven statistical approaches for Solar Energetic Particle (SEP) Events forecasting
17:15 E. Cliver: A Short-term Forecast Tool for ≥ S2 (≥ 100 pfu) Solar Proton Events: Preliminary Report
17:45 General discussion

18:00 Adjourn


Tuesday February 28

SEP Forecasting (2)
09:00 M. Nunez: Predicting the occurrence of GLE events
09:30 J. Labrenz: Near realtime forecasting of MeV protons on the basis of sub relativistic electrons
10:00 R. Bütikofer: GLE Inversion Software – Assessment of Source and Transport Parameters Based on Neutron Monitor Data
10:30 A. Papaioannou: HESPERIA data retrieval tool demonstration

10:45 Coffee break

11:30 K.-L. Klein: Microwave observations for forecasting energetic particles from the Sun
12:00 M. Dierckxens: SEP Scoreboard: Real-time Forecasting Validation
12:30  General discussion: SEP forecasting, HESPERIA, perspectives

13:00 Lunch
High-energy particles at the Sun: EM emissions
14:30 G. Share: Characteristics of 29 Sustained-Emission >100 MeV Gamma-Ray Events Associated with Impulsive Solar Flares
15:00 P. Zucca: A search for radio and X-ray counterparts of long-lasting solar gamma-ray emission from relativistic protons
15:30  A. Mackinnon: Secondary Electrons from Energetic Flare Ions

16:00 Coffee break

17:00 Guided tour of Paris Observatory

Wednesday March 1

High-energy particles from the Sun: SEPs
09:00 E. Valtonen: Energy Spectra and Abundance Ratios of Heavy Ions in HESPERIA Gamma-Ray Events
09:30 K. Tziotziou: Multi-spacecraft solar energetic particle analysis of FERMI gamma-ray flare events
10:00 P. Kühl: Solar Energetic Particle Events with Protons > 500 MeV between 1995 and 2015 Measured with SOHO/EPHIN

10:30 Coffee break

11:00 A. Afanasiev: Testing the shock origin of protons responsible for solar long-duration gamma-ray events
11:30 A. Aran: Modelling The 2012 January 23 And 2012 May 17 SEP Event With The Shock-And-Particle Model
12:00 A. Rouillard: CME and shock tracking during FERMI/LAT gamma-ray events (title TBC)

12:30 General discussion: High-energy particles at and from the Sun

13:00 Lunch

14:30 J. Kartavykh: Modeling of Energetic Particle Transport and Acceleration at Interplanetary Shock Waves in Mixed Solar Particle Events
15:00 S. Dalla: Solar Electron Deceleration in Interplanetary Space
15:30 W. Dröge: Multi-spacecraft observations and transport modeling of solar energetic particles in the inner Heliosphere

16:00 Coffee break

16:30 D. Strauss: Simulating Solar Energetic Particle Transport
17:00 D. Pacheco: Interplanetary Transport of Solar Electron Events Detected over a Narrow Range of Heliolongitudes
17:30 General discussion: Particle transport modelling

18:00 Adjourn

Thursday March 2

09:00 N. Dresing: Long-lasting solar energetic electron injection during the 26 Dec 2013 widespread SEP event
09:30 S. Masson: Flare-accelerated particles' escape in 3D solar eruptive events
10:00 O. Malandraki: Joint Ne/O and Fe/O Analysis to Diagnose Large Solar Energetic Particle Events during Solar Cycle 23
10:30 R. Vainio: Why is Solar Cycle 24 Inefficient in Producing High-Energy Particle Events?

11:00 Coffee break

11:30 General discussion: Political recommendations of the HESPERIA project – to be introduced by short presentations of the lead authors of the document
12:45 Closing

13:00 Lunch

Afternoon: HESPERIA consortium meeting (until Friday March 3, at noon)

Abstracts can be downloaded from here.

Workshop program can be downloaded in printable format here.

DMC Firewall is developed by Dean Marshall Consultancy Ltd