Generation and annihilation of three dimensional magnetic nulls in extrapolated solar coronal magnetic field: data-based Implicit Large Eddy simulation

- Maurya, Yogesh Kumar, Bhattacharyya, Ramit, Pontin, David

Magnetic reconnections as the underlying cause of spontaneous generation and annihilation of three-dimensional magnetic nulls

- Maurya, Yogesh Kumar, Bhattacharyya, Ramit, Pontin, David I.

Reconnection-generated Plasma Flows in the Quasi-separatrix Layer in Localized Solar Corona

- Mondal, Sripan, Srivastava, Abhishek K., Yuan, Ding, Mishra, Sudheer K., Sangal, K., Kayshap, Pradeep, Guo, Yang, Pontin, David I., Uritsky, Vadim M., Ofman, Leon, Wang, Tongjiang

Magnetic reconnection and the Kelvin-Helmholtz instability in the solar corona

- Howson, T. A., De Moortel, I., Pontin, D. I.

Magnetohydrodynamic Reconnection

- Pontin, D. I.

Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops

- Pontin, D. I., Peter, H., Chitta, L. P.

The Parker problem: existence of smooth force-free fields and coronal heating

- Pontin, David I., Hornig, Gunnar

Electrodynamic context of magnetopause dynamics observed by magnetospheric multiscale

- Anderson, Brian J., Russell, Christopher T., Cohen, Ian J., Westlake, Joseph H., Mauk, Barry H., Leinweber, Hannes K., Gershman, Daniel J., Giles, Barbara L., Le, Guan, Torbert, Roy B., Burch, James L., Strangeway, Robert J., Plaschke, Ferdinand, Magnes, Werner, Fischer, David, Korth, Haje, Merkin, Viacheslav G., Barnes, Robin J., Waters, Colin L.

Modeling the observed proton aurora and ionospheric convection responses to changes in the IMF clock angle: 1. persistance of cusp proton aurora

- Throp, K., Lockwood, M., Lanchester, B. S., Morley, S. K., Frey, H. U.