Magnetohydrodynamic Shocks and Solitons in the Solar Atmosphere: Recent Challenges in Observations and Theory. Planetary Radio Emissions| PLANETARY RADIO EMISSIONS VII 7|
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28 décembre 2011
- handle: 10670/1.uv3e3z
- GOid: 0xc1aa5576_0x002a1d30
info:eu-repo/semantics/openAccess
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Mathematics, Physics and Space ResearchSujets proches
Atmosphere, Solar Sun--Atmosphere Wireless (Radio) Telephone, Wireless Wireless telephone (Early radio)Citer ce document
H. O. Rucker et al., « Magnetohydrodynamic Shocks and Solitons in the Solar Atmosphere: Recent Challenges in Observations and Theory. Planetary Radio Emissions| PLANETARY RADIO EMISSIONS VII 7| », Elektronisches Publikationsportal der Österreichischen Akademie der Wissenschafte, ID : 10670/1.uv3e3z
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Magnetohydrodynamic shocks are believed to play a significant role in the dynamics of lower solar atmosphere. Here we review the recent theoretical developments in shock wave induced phenomena and first observational evidence of slow sausage soliton in the solar chromosphere.