Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions

Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions

Type III solar radio bursts are the Sun's most intense and frequent nonthermal radio emissions. They involve two critical problems in astrophysics, plasma physics, and space physics: how collective processes produce nonthermal radiation and how magnetic reconnection occurs and changes magnetic...

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Main Authors: Cairns, I., Lobzin, V., Donea, A., Tingay, Steven, McCauley, P., Oberoi, D., Duffin, R., Reiner, M., Hurley-Walker, Natasha, Kudryavtseva, N., Melrose, D., Harding, J., Bernardi, G., Bowman, J., Cappallo, R., Corey, B., Deshpande, A., Emrich, David, Goeke, R., Hazelton, B., Johnston-Hollitt, M., Kaplan, D., Kasper, J., Kratzenberg, E., Lonsdale, C., Lynch, Mervyn, McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Ord, S., Prabu, T., Roshi, A., Shankar, N., Srivani, K., Subrahmanyan, R., Wayth, Randall, Waterson, M., Webster, R., Whitney, A., Williams, A., Williams, C.
Format: Journal Article
Published: Nature Publishing Group 2018
Online Access:http://hdl.handle.net/20.500.11937/65908

Internet

http://hdl.handle.net/20.500.11937/65908

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