Interviewing a MAARBLE Scientist – May 2013

Who is Who

ioannisdaglis-150x150Ioannis (Yannis) Daglis, the coordinator of the MAARBLE Project, is a space physicist and has been active in solar-terrestrial research for more than 20 years. He is a Professor of the Department of Physics at the University of Athens and he served as the Director of the Institute for Astronomy, Astrophysics, Space Applications & Remote Sensing at the National Observatory of Athens for 7 years (2006-2013).

Prof. Daglis received the Diploma of Physics in 1986 from the Aristotle University of Thessaloniki (Greece) and a PhD in Space Electrodynamics from the Democritus University of Thrace (Greece) in 1991. He is a full member of the International Academy of Astronautics; Editor for Magnetosphere and Space Plasma Physics, Annales Geophysicae; IAGA National Correspondent for Greece; Board Member of the Greek Research & Technology Network. Among others, he has served as member of the Solar System Working Group (advisory committee of ESA) and the Science Review Panel for the Radiation Belt Storm Probes Mission of NASA.

He is the author or co-author of 80+ refereed papers; Editor and co-author of the book Space Storms and Space Weather Hazards, Springer (2001), which is “Recommended teaching material” of the United Nations Space Science Curriculum; and editor and co-author of 3 more space physics / space weather related monographs.

The Sun is 150 million kilometres (93 million miles) away, yet is near enough to “affect terrestrial affairs in any sensible degree; and its influence upon them is such that it is hard to find the word to name it” (Charles Young 1896, an American astronomer who was the first to see the green spectral line of the solar corona). More than a century after Young’s statement, scientists are still striving to understand the complex ways through which the Sun influences our planet.

“My research interests focus on the Sun-Earth connection and the dynamic physical processes involved,” says Dr. Daglis. “As the Sun is our star and Earth is our home planet, their connection cannot be overemphasized and it is obvious that it is of particular interest! Apart from the “sentimental connection” though, the complex interplay of physical processes of Sun-Earth connection is scientifically very intriguing.”

The heat received by the Sun drives clouds and rain and ultimately the Earth’s climate; the sunlight drives plant photosynthesis, which is at the origin of the food chain that all living beings on Earth are part of. Yet the Sun influences the planet in a less perceptible by humans, though dramatic way, through the interplanetary magnetic field, the solar wind (plasma escaping the solar corona and invading the interplanetary space) and even more violent phenomena, such as coronal mass ejections (discharges of coronal material containing up to 11,000 million tons of solar matter traveling at a million miles per hour). These can trigger aurorae and other electromagnetic disturbances on Earth, the so-called magnetic storms, which may affect severely ground-based power systems, space-born satellite and navigation systems, communications, manned space flights and the Earth's climate, endangering human health or life.

“The major challenge is still the comprehensive understanding of the synergy of coupled elementary physical processes that results in complex collective phenomena of explosive energy dissipation” says Dr. Daglis. “The next major challenge is the ability to accurately forecast the dynamics of space weather processes” (space weather refers to conditions on the Sun and in the solar wind, the Earth's magnetosphere and ionosphere).

Scientists are still working hard in trying to accurately forecast space weather, as they do for Earth’s weather. Timely warning of an imminent geomagnetic storm could save the satellite operators, power and telecommunication companies millions of euros/dollars of damage and more importantly potentially save human lives. Dr. Daglis’ future research plans are clearly to “continue investigating the dynamic influence of the Sun on Earth and the other planets and to contribute to forecasting the phenomena involved”.

radiationbeltstormprobe


The Van Allen Probes (VAP) mission, which was launched just a few months ago, is an exciting new mission with excellent instrumentation that drives great expectations!

“I first became interested in space science during a summer visit to the Institute for Astrophysics and Extraterrestrial Research of the University of Bonn in Germany, when I was studying Physics at the Aristotle University of Thessaloniki in Macedonia, Greece.” Dr. Daglis worked on his PhD in Space Plasma Electrodynamics at the Max Planck Institute for Solar System Research (Germany) and the Johns Hopkins University Applied Physics Laboratory (USA). “The major challenge in my career was to stay active in space research under initially unfavourable conditions, when I returned to Greece after leaving a hyper-active group at the Max Planck Institute in Germany, where I had spent 7 years”.

Despite difficulties faced upon returning to Greece, Dr. Daglis excelled as a scientist and served in positions of highest responsibility, at home and abroad. “Nothing in life is easy - why should it?” he says. “Hard work and determination are key parameters to a successful career.” But he also adds: “It is of utmost importance to enjoy what you are doing; if you really enjoy your work, nothing else really matters”.

maarble final 

Speaking of the beginnings of the MAARBLE project, Dr. Daglis mentions: “I had become fascinated by the potentially decisive role of ultra-low frequency waves in radiation belt dynamics and by some special characteristics of them.” The wavelength of these waves is huge – comparable to the size of Earth itself! “I am intrigued by all kinds of waves. One of my favourite paintings is the “Great wave” of the famous Japanese artist Hokusai”.

great wave off kanagawa 

“Through my long-time research on the energetic plasma population known as the ring current, I also became very interested in the high-end of energetic plasma in geospace, namely the radiation belts” says Dr. Daglis. The radiation belts are – just like the ring current – very much influenced by the most complex impulsive phenomenon in geospace, the magnetic storms. But the question has always been HOW” he adds.

Dr. Daglis decided that a project investigating the role of low frequency waves in energetic electron dynamics, involving some of the best research teams worldwide, would be a worthwhile endeavour. “And I was lucky enough to receive positive responses from leading scientists in our field to the invitation to join the effort”. As a result, the MAARBLE project has united cutting-edge know-how, leading to important synergy in radiation belt research. “I feel very privileged and happy to coordinate this top consortium”, Dr. Daglis concludes. As a devoted mountain enthusiast, he is obviously very fond of tops!

The MAARBLE project will provide a significant boost to European and international research on radiation belt dynamics. The data products it will provide to the scientific community (electromagnetic waves database and statistical model) are of particular importance to comprehensive understanding of the dynamic variability of the Van Allen belts, because of the critical role of waves in electron acceleration, transport, scattering and loss. The wave database and statistical model will be complemented by in-depth studies of individual effects of waves on electron dynamics, as well as by data assimilation of various particle data sets into the ONERA radiation belt model. The NOA team participates in all parts of the MAARBLE project and the team members are happy and proud of their involvement in this state-of-the-art European space research project.