Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Big Bear Solar Observatory, Big Bear City, California, USA
Center for Solar-Terrestrial Research, New Jersey Institute of Technology;, Big Bear Solar Observatory
Big Bear Solar Observatory, New Jersey Institute of Technology
Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA 92314, USA
Big Bear Solar Observatory, Big Bear City, CA 92314
Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear City, CA 92314-9672 Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314, USA
Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear City, CA 92314
Big Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92316, USA
New Jersey Institute of Technology, Center for Solar-Terrestrial Research
Big Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314, USA Bear Solar Observatory, Big Bear City, CA, USA; Bear Solar Observatory, Big Bear City, CA 92314.
BBSO / NJIT, 40386 N. Shore Lane, Big Bear City, CA 92314 Bear Solar Observatory
BBSO / NJIT
BBSO
Big Bear Solar Observatory, Big Bear City, CA; Crimean Astrophysical Observatory, Nauchny, Crimea, Ukraine
Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear City, CA 92314 Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear City, CA 92314, USA Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314-9672.
Big Bear Solar Observatory, 40386 N. Shore Lane, Big Bear City, CA 92314, USA
Vasyl Yurchyshyn, 40386 North Shore Lane,
An Overview of Existing Algorithms for Resolving the 180° Ambiguity in Vector Magnetic Fields: Quantitative Tests with Synthetic Data
Analyses of magnetic field structures for active region 10720 using a data-driven 3D MHD model
Automatic Prediction of Super Geomagnetic Storms and Solar Flares
Calculation of Intermittency in the Photosphere and Corona From Hinode Data
Cancellations and structures in the solar photosphere: signature of flares
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Profile ID: LFWR-SCP-P-22013