Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Johns Hopkins Univ., USA
Applied Physics Laboratory, Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723
JHU / APL
The Johns Hopkins University, Applied Physics Laboratory
Johns Hopkins University, Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099
Research Center for Astronomy and Applied Mathematics Academy of Athens, 4 Soranou Efesiou Street, Athens GR-11527, Greece
Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 of Astrophysics, Astronomy and Mechanics Department of Physics, University of Thessaloniki, GR-54006 Thessaloniki, Greece
Johns Hopkins University, Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723.
Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099.
The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723
The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723.
JHU / APL, 11100 Johns Hopkins Rd, Laurel, MD 20723 Physics Laboratory, Johns Hopkins University
JHU / Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723-6099, USA
Johns Hopkins University, Applied Physics Laboratory 11100 Johns Hopkins Rd., Laurel, MD 20723, USA Hopkins University, Applied Physics Laboratory, 11100 Johns Hoplkins Rd., Laurel, MD 20723, USA Hopkins University, Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723, USA Johns Hopkins University Applied Physics Laboratory, 1
A comparison between statistical properties of solar X-ray flares and avalanche predictions in cellular automata statistical flare models
A New Technique for a Routine Azimuth Disambiguation of Solar Vector Magnetograms
An Overview of Existing Algorithms for Resolving the 180° Ambiguity in Vector Magnetic Fields: Quantitative Tests with Synthetic Data
Are Solar Active Regions with Major Flares More Fractal, Multifractal, or Turbulent than Others?
Assessment Of The Eruptive Potential In Solar Active Regions
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