Natchimuthuk Gopalswamy
Affiliations: | The Catholic University of America, Washington, DC |
Area:
Astronomy and Astrophysics, Atmospheric Sciences, GeophysicsWebsite:
https://science.gsfc.nasa.gov/sed/bio/natchimuthuk.gopalswamy-1Google:
"Natchimuthuk Gopalswamy"Mean distance: (not calculated yet)
Children
Sign in to add trainee| Steven M. Nunes | grad student | 2007 | Catholic University |
| Anshu Kumari | post-doc | 2023-2025 | (Astronomy Tree) |
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Publications
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| Gopalswamy N, Mäkelä P, Yashiro S, et al. (2020) Source of Energetic Protons in the 2014 September 1 Sustained Gamma-ray Emission Event. Solar Physics. 295: 18 |
| Gopalswamy N, Makela P, Xie H, et al. (2015) Low-frequency solar radio bursts and their space weather implications 2015 1st Ursi Atlantic Radio Science Conference, Ursi At-Rasc 2015 |
| Gopalswamy N, Mäkelä P, Yashiro S. (2014) An overview of STEREO/WAVES science results 2014 United States National Committee of Ursi National Radio Science Meeting, Usnc-Ursi Nrsm 2014 |
| Hariharan K, Ramesh R, Kishore P, et al. (2014) An estimate of the coronal magnetic field near a solar coronal mass ejection from low-frequency radio observations Astrophysical Journal. 795 |
| Wu CC, Gopalswamy N, Lepping RP, et al. (2013) Characteristics of magnetic clouds and interplanetary coronal mass ejections which cause intense geomagnetic storms Terrestrial, Atmospheric and Oceanic Sciences. 24: 233-241 |
| Cho KS, Gopalswamy N, Kwon RY, et al. (2013) A high-frequency type ii solar radio burst associated with the 2011 february 13 coronal mass ejection Astrophysical Journal. 765 |
| Gopalswamy N. (2013) Observations of CMEs and models of the eruptive corona Aip Conference Proceedings. 1539: 5-10 |
| Gopalswamy N. (2013) Coronal Mass Ejections and Type II Radio Bursts Solar Eruptions and Energetic Particles. 165: 207-220 |
| Gopalswamy N, Yashiro S. (2013) Obscuration of Flare Emission by an Eruptive Prominence Publications of the Astronomical Society of Japan. 65 |
| Kim RS, Gopalswamy N, Moon YJ, et al. (2012) Magnetic field strength in the upper solar corona using white-light shock structures surrounding coronal mass ejections Astrophysical Journal. 746 |