Abstract

The processes of flare energy release, plasma heating, and particle acceleration and the modulation of optical and rf radiations and x rays in coronal magnetic arcs on the sun and stars are described by representing the arc as a cavity for magnetohydrodynamic waves, equivalent to an electric circuit and a trap with magnetic stoppers. © 2005 Optical Society of America

Spectroscopic Line-Profile Studies of Long Magnetically Confined High-Current, Steady-State Vacuum Arcs

J. R. McNally and M. R. Skidmore
Appl. Opt. 2(7) 699-706 (1963)

Applicability of moiré deflection tomography for diagnosing arc plasmas

Chen Yun-yun, Song Yang, He An-zhi, and Li Zhen-hua
Appl. Opt. 48(3) 489-496 (2009)

Vacuum Ultraviolet Plasma Arc Radiation Source for the 300–1000-A Wavelength Region

M. E. Levy and R. E. Huffman
Appl. Opt. 9(1) 41-47 (1970)

Studies of Coronal Lines with Electronic Cameras During the Eclipse of 7 March 1970

B. Fort
Appl. Opt. 9(12) 2643-2647 (1970)

Ionization effect on arc plasma’s optical diagnosis by the measurement of the refractive index

Yun-yun Chen, Cheng-yi Zhang, Fang Gu, Qing-hua Wang, and Zhen-hua Li
Appl. Opt. 51(16) 3397-3402 (2012)