Solar p-modes oscillations and heating of the corona

✍ Scribed by V. I. Zhukov

• Publisher: Springer
• Year: 1992
• Tongue: English
• Weight: 288 KB
• Volume: 139
• Category: Article
• ISSN: 0038-0938
• DOI: 10.1007/bf00147890

✦ Synopsis

Abst~'~{ct. The p:,operties of the resona~tor are considered for fast magnetoacoustie waves, it is shown that tunnel penetration of waves from the resonator leads either to heating of the mediu,~l Jn the ~ifv4n resonance vicinity7 (if the inclination angle of the magne' " ~'~le field is smaller than the critical ansle), or to excitation of Alfv$n waves at the Alfv6n ~oesonanee (if the inc!Jnation angle is larger than [he critical angle). This suggests that non-radiative heating of the corona can be due %o solaz' p-mode oscillations.