Organization profile
Organization profile
The primary goal of the Center for Computational Heliophysics is to develop data analysis and modeling tools in the area of heliophysics – the study and prediction of the Sun’s magnetic activity – by combining expertise from computer scientists in the Ying Wu College of Computing with that of physicists and mathematicians in the College of Science and Liberal Arts. We work in partnership with NASA’s Advanced Supercomputing Division at the NASA Ames Research Center. The center’s work is focused on novel, innovative approaches, including the development of intelligent databases, automatic feature identification and classification, realistic numeric simulations based on first-physics principles and observational data modeling. The center develops synergies among these approaches to make substantial advances in heliophysics and computer science. Our new methods and tools can be used in broader scientific and engineering applications for developing new approaches to intelligent big data databases, as well as for image-recognition and characterization methodologies in collaboration with the Computer Science Department. The computational models have been used for modeling the magnetic activity of other stars in support of NASA’s Kepler mission and the search for extraterrestrial life.
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Collaborations and top research areas from the last five years
Profiles
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Alexander Kosovichev
- Center for Computational Heliophysics - Director
- Physics - Distinguished Professor
Person
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Working Toward a Better Regulatory Framework for Medical Cannabis
Oria, V. (PI), Mili@njitedu, A. M. (CoPI) & Arkell, T. T. (PI)
8/1/21 → 7/31/27
Project: Research project
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HELIOSEISMIC IMAGING OF EMERGING MAGNETIC FLUX FOR FORECASTING OF SPACE WEATHER EVENTS
Kosovichev, A. (PI)
9/23/20 → 9/22/21
Project: Research project
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Investigation of Solar Torsional Oscillations and Their Relation to Activity Cycles
Kosovichev, A. (PI)
7/13/20 → 7/12/23
Project: Research project
Research output
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Daily Predictions of F10.7 and F30 Solar Indices With Deep Learning
Wang, Z., Abduallah, Y., Wang, J. T. L., Wang, H., Xu, Y., Yurchyshyn, V., Oria, V., Alobaid, K. A. & Bai, X., Feb 2026, In: Journal of Geophysical Research: Space Physics. 131, 2, e2025JA034868.Research output: Contribution to journal › Article › peer-review
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Helioseismic evidence that the solar dynamo originates near the tachocline
Mandal, K. & Kosovichev, A. G., Dec 2026, In: Scientific reports. 16, 1, 4222.Research output: Contribution to journal › Article › peer-review
Open Access -
Simulations of Global Solar Convection with a Fully Compressible CHORUS++ Code
Hayashi, K., Kosovichev, A. G. & Liang, C., Feb 1 2026, In: Astrophysical Journal, Supplement Series. 282, 2, 58.Research output: Contribution to journal › Article › peer-review
Open Access
Press/Media
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The Source Of Solar Storms Exists 16 Earth Widths Under The Sun
3/28/26
1 item of Media coverage
Press/Media: Press / Media
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Scientists identify deep solar layer as origin of storms
3/28/26
1 item of Media coverage
Press/Media: Press / Media
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Scientists just found the hidden magnetic engine powering the sun’s explosive storms
3/28/26
2 items of Media coverage
Press/Media: Press / Media