Simulations of gyrosynchrotron microwave emission from an oscillating 3D magnetic loop

AA Kuznetsov, VE Reznikova - Solar Physics, 2015 - Springer
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Van Doorsselaere… - Solar …, 2015 - search.proquest.com
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Van Doorsselaere… - Solar …, 2015 - ui.adsabs.harvard.edu
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

[引用][C] simulations of gyrosynchrotron microwave emission from an oscillating 3D magnetic loop

AA Kuznetsov, T Van Doorsselaere, VE Reznikova - Solar Physics, 2015 - elibrary.ru

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Doorsselaere, VE Reznikova - Solar Physics, 2015 - infona.pl
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

[PDF][PDF] Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Van Doorsselaere, VE Reznikova - 2015 - lirias.kuleuven.be
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop.

A Kuznetsov, T Doorsselaere, V Reznikova - Solar Physics, 2015 - search.ebscohost.com
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

A Kuznetsov, T Van Doorsselaere… - arXiv preprint arXiv …, 2015 - arxiv.org
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

[PDF][PDF] Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Van Doorsselaere, VE Reznikova - 2015 - perswww.kuleuven.be
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …

[PDF][PDF] Simulations of Gyrosynchrotron Microwave Emission from an Oscillating 3D Magnetic Loop

AA Kuznetsov, T Van Doorsselaere… - arXiv preprint arXiv …, 2015 - researchgate.net
Radio observations of solar flares often reveal various periodic or quasi-periodic
oscillations. Most likely, these oscillations are caused by magnetohydrodynamic (MHD) …