




Symposium program
Space Climate is an interdisciplinary science that deals with the long-term change in the Sun, and its effects in the heliosphere and in the near-Earth environment, including the atmosphere and climate. A special focus will be on studies of the causes, consequences and implications of the present, unusually low solar activity since solar cycle 23 that, most likely, indicates the imminent end of the Modern Grand Maximum of solar activity. Other topics include solar dynamo, solar irradiance variations, solar wind, geomagnetic field and activity, cosmic rays and cosmogenic isotopes, and solar effects on different layers of the atmosphere and on local and global climate, as well as possible solar effects on human health and on the development of human cultures.
The program is also available as a PDF file.
Oral program
Saturday 15.6.
Session 1: Solar dynamo as a Driver of Space Climate
0900-0920 | Welcome and practicalities | |
0920-1000 | Axel Brandenburg | Magnetic field generation on long time scales (Keynote talk) |
1000-1030 | Dario Passos | ILES global simulation of solar convection and dynamo action |
1030-1100 | Maarit Mantere | Cyclic magnetic activity due to turbulent convection |
Coffee break | ||
1130-1150 | Joern Warnecke | Dynamo driven coronal ejections |
1150-1210 | Caroline Dubé | Dynamo modeling of stellar activity cycles |
1210-1230 | Sylvaine Turck-Chièze | The activity of the inner Sun |
1230-1300 | Sacha Brun | The solar-stellar dynamo connection |
Lunch |
Session 2: Long-term Solar activity
1430-1500 | Frédéric Clette | Revisiting the long-term calibration of the international sunspot number |
1500-1530 | Alexei Pevtsov | Long-term trends in the magnetic fields of sunspots |
1530-1550 | Nadezhda Zolotova | Modeling of polar magnetic field reversals from sunspot impulses |
Coffee break | ||
1615-1645 | Rainer Arlt | Extending the solar butterfly diagram into the past |
1645-1715 | José Vaquero | Applied historical heliophysics: a review |
1715-1745 | Maria Dasi Espuig | Sunspot group tilt angles and the strength of solar cycles |
1745-1815 | Questions & discussion on Day 1 topics | |
1815-> | Ice breaker and poster viewing |
Sunday 16.6.
Session 3: Long-term Solar activity, continued
0830-0900 | Kiyoto Shibasaki | Long-term global solar activities studied by the Nobeyama radioheliograph |
0900-0930 | Ilya Usoskin | Occurrence probability of extreme SEP events on different time scales |
0930-1000 | Juerg Beer | Cosmogenic radionuclides and long-term solar activity |
1000-1020 | Rita Traversi | A potential new proxy of long-term solar variability: nitrate in Antarctic ice cores |
Coffee break |
Session 4: TSI/SSI
1050-1120 | Gaël Cessateur | An overview of the solar spectral irradiance variability |
1120-1150 | Cassandra Bolduc | MOCASSIM: A model for spectral solar irradiance |
1150-1220 | William Ball | Solar Spectral Irradiance intercomparison between a new SATIRE-S model dataset and the NRLSSI model and SORCE/SOLSTICE observations |
1220-1240 | Irina Kostyuchenko | The total solar irradiance, UV emission and magnetic flux during the last solar cycle minimum |
1240-1300 | Matthieu Kretzschmar | Energy released by solar flares in the EUV wavelength range |
Lunch |
Session 5: Special Session on Planetary influences on solar variability
1430-1500 | Jose Abreu | Is there a planetary influence on solar activity? |
1500-1530 | Pavel Hejda | Very long-term solar-terrestrial variability related to the two basic types of the solar inertial motion |
1530-1600 | Jan-Erik Solheim & Nicola Scafetta | Does the Sun work as a nuclear fusion amplifier of planetary tidal forcing? |
Coffee break | ||
1630-1700 | Katya Georgieva | Planetary influence on solar activity from the point of view of the flux transport dynamo |
1700-1730 | Paul Charbonneau | Sensivity of the solar dynamo to external multiperiodic forcing |
1730-1800 | Special Session Discussion | |
Questions & discussion on other Day 2 topics | ||
2000-2100 | Esa Turunen | Auroral lights in Finland: History and observations |
Monday 17.6.
Session 6: Special Session on Solar extreme events (flares, energetic particles etc) and their effects
0800-0830 | Karel Schrijver | Constraining the properties of extreme solar explosive events |
0830-0900 | Kazunari Shibata | What is the worst we can expect from the Sun? |
0900-0930 | Fusa Miyake | Rapid events in the carbon-14 content of tree-rings |
Coffee break | ||
0950-1020 | Seiji Yashiro | Difference in CME rate and other properties between solar cycles 23 and 24 |
1020-1050 | Margaret Shea | Comparison of solar-terrestrial phenomena for the first four years of six solar cycles |
1050-1120 | Gang Li | What causes a Ground Level Event - a "twin-CME" scenario? |
1120-1140 | Laure Lefevre | Historical analysis of Sun-Earth connections in the context extreme space weather events |
Special Session Discussion | ||
Lunch | ||
Afternoon freetime activities (sign in!) | ||
1900 | Conference Dinner at Hotel Radisson Blue (Restaurant Toivo) |
Tuesday 18.6.
Session 7: Solar corona, solar wind and HMF
0800-0830 | Sami Solanki | Solar spectral irradiance variability |
0830-0900 | Georgeta Maris Muntean | Long-term variability of the high speed solar wind |
0900-0930 | Olga Khabarova | The interplanetary magnetic field in the inner heliosphere: what we know from multi-spacecraft observations |
0930-0950 | Géza Erdős | Magnetic flux density in the heliosphere |
0950-1010 | Antoine Llebaria & Philippe Lamy | CME rate derived from SOHO/LASCO observations and comparison with sunspot number and other solar proxies |
1010-1030 | Kristian Snekvik | Alfvénic fluctuations in solar wind streams, and their potential geomagnetic effects |
Coffee break | ||
1100-1120 | Marius Echim | Solar system plasma intermittency: methods and observations over the solar cycle |
1120-1140 | Kalevi Mursula | Solar wind stream activity during the Modern Great Maximum |
Session 8: Magnetosphere and Ionosphere
1140-1210 | Walter Gonzalez | Geomagnetic response to the Long Solar Minimum phase of Solar Cycle 23 |
1210-1230 | Timo Asikainen | Long-term variation of energetic particles and their relation to geomagnetic activity |
1230-1300 | Ingrid Cnossen | The response of the ionosphere to the changing terrestrial magnetic field |
Lunch |
Session 9: Solar atmospheric and climate effects
1430-1500 | Ana Elias | Solar influence on the long-term change in the ionosphere |
1500-1530 | Thomas von Clarmann | Solar and geomagnetic effects in the middle and lower atmosphere |
1530-1600 | Eugene Rozanov | Modeling of the spectral solar irradiance and energetic particle effects on the atmospheric chemistry and climate |
1600-1630 | Hua Lu | Solar wind effect on planetary wave propagation and synoptic-scale Rossby wave breaking |
Coffee break | ||
1700-1730 | Alan Aylward | Solar Effects in Upper Atmosphere Circulation |
1730-1800 | Pekka Verronen | Mesospheric OH response to the impact of radiation belt electrons |
Questions & discussion on other Day 4 topics |
Wednesday 19.6.
Session 10: Solar atmospheric and climate effects, continued
0830-0900 | Mai Mai Lam | The interplanetary magnetic field influences middle-latitude surface atmospheric pressure |
0900-0930 | Josef Bochnicek | The association between long-lasting high solar/geomagnetic activity and geopotential height changes in the northern winter lower atmosphere |
0930-1000 | Radan Huth | Effects of variations in solar activity on tropospheric circulation |
1000-1030 | Maxim Ogurtsov | New evidence of the solar Gleissberg periodicity in summer temperature over Northern Fennoscandia |
Coffee break | ||
1100-1130 | Nils-Axel Mörner | Solar wind, Earth’s rotation and changes in terrestrial climate |
1130-1200 | Mirela Voiculescu | Possible relationship between space weather and cloud cover and role of various climatic factors |
1200-1220 | Benjamin Laken | Why don't composite studies agree? An example with cosmic rays and clouds |
1220-1300 | Alexei Pevtsov | Symposium Summary and Conclusions |
Lunch | ||
Departure |
Poster program
Solar/Stellar
Helispheric
Olga Khabarova | The solar wind plasma dynamics in a vicinity of the heliospheric current sheet as observed at different heliocentric distances |
Martin Leitner | Statistical analysis of the solar wind quasi-invariant using STEREO and WIND |
Alexander Mishev | Quasi real time analysis of GLEs using neutron monitor network data |
Costel Munteanu | The effect of wavelet denoising on the propagation time delay of solar wind discontinuities |
Mikhail Vokhmyanin | Geomagnetic superstorm of 1859 and sector structure of IMF |
Yu Xiao Xia | Cosmic-Ray Research for Space Weather Monitoring and Forecasting |
Ilpo Virtanen | Bashful ballerina unveiled: Multipole analysis of the coronal magnetic field |
Don Smart |
Magnetospheric/Ionospheric
Anita Aikio | EISCAT_3D, Next generation IS radar for geospace environment research |
Galina Gordiyenko | A long-term trend in the F2-layer critical frequency as observed at Alma-Ata ionosonde station |
Miroslaw Kowalinski | Energetic particle activity in separate magnetospheric polar regions as well as the SAA as determined from X-rays detectors in RESIK spectrophotometer aboard Coronas-F. |
Daniel Martini | Using recursive algorithm for defining solar regular geomagnetic variations |
Oleg Troschichev | Solar UV irradiation and solar wind effects in the polar cap magnetic activity (PC index): Distinctive features of the last cycle of solar activity |
Atmospheric/Climate
Late posters
Yana Asenovska | High speed solar wind influence on NAO index and surface air temperature |
Andrey Tlatov | Reversals of Gnevyshev - Ohl rule |
