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Cited article:
G. Bodo , S. Poedts , A. Rogava , P. Rossi
A&A, 374 1 (2001) 337-347
Published online: 2001-07-15
This article has been cited by the following article(s):
17 articles
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Self-heating in kinematically complex magnetohydrodynamic flows
Zaza Osmanov, Andria Rogava and Stefaan Poedts Physics of Plasmas 19 (1) 012901 (2012) https://doi.org/10.1063/1.3675865
ALFVÉN WAVES IN SHEAR FLOWS REVISITED
Joseph V. Hollweg and Edisher Kh. Kaghashvili The Astrophysical Journal 744 (2) 114 (2012) https://doi.org/10.1088/0004-637X/744/2/114
Multi-scale Physics in Coronal Heating and Solar Wind Acceleration
Enrico Camporeale Space Sciences Series of ISSI, Multi-scale Physics in Coronal Heating and Solar Wind Acceleration 38 397 (2011) https://doi.org/10.1007/978-1-4614-6461-7_26
Self-heating and its possible relationship to chromospheric heating in slowly rotating stars
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Magnetohydrodynamic wave mixing in shear flows: Hamiltonian equations and wave action
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Overreflection and Generation of Gravito‐Alfven Waves in Solar‐Type Stars
Andria Rogava, Grigol Gogoberidze and Stefaan Poedts The Astrophysical Journal 664 (2) 1221 (2007) https://doi.org/10.1086/518824
Quantifying Shear‐induced Wave Transformations in the Solar Wind
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Are Astrophysical Shear Flows Able to Heat Themselves?
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Virtual Astrophysical Jets
Andria Rogava Virtual Astrophysical Jets 189 (2004) https://doi.org/10.1007/978-1-4020-2664-5_21
Transient shear instability of differentially rotating and self-gravitating dusty plasma
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Swirling astrophysical flows – efficient amplifiers of Alfvén waves!?
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Amplification of MHD waves in swirling astrophysical flows
A. D. Rogava, G. Bodo, S. Massaglia and Z. Osmanov Astronomy & Astrophysics 408 (2) 401 (2003) https://doi.org/10.1051/0004-6361:20030454
Does spiral galaxy IC 342 exhibit shear induced wave transformations!?
S. Poedts and A. D. Rogava Astronomy & Astrophysics 385 (1) 32 (2002) https://doi.org/10.1051/0004-6361:20020079