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10.12942/lrsp-2010-4 http://scihub22266oqcxt.onion/10.12942/lrsp-2010-4 C4841184!4841184!27194962     free     free     free       Living+Rev+Sol+Phys 2010 ; 7 (ä): ä Nephropedia Template TP {{tp|p=27194962|t=2010. Wave Modeling of the Solar Wind |pdf=|usr=}}{{27194962}} gab.com Text Wave Modeling of the Solar Wind JO: Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194962 #FOAvip The acceleration and heating of the solar wind have been studied for decades using satellite observations and models. However, the exact mechanism that leads to solar wind heating and acceleration is poorly understood. In order to improve the understanding of the physical mechanisms that are involved in these processes a combination of modeling and observational analysis is required. Recent models constrained by satellite observations show that wave heating in the low-frequency (MHD), and high-frequency (ion-cyclotron) range may provide the necessary momentum and heat input to coronal plasma and produce the solar wind. This review is focused on the results of several recent solar modeling studies that include waves explicitly in the MHD and the kinetic regime. The current status of the understanding of the solar wind acceleration and heating by waves is reviewed. Twit Text FOAVip Wave Modeling of the Solar Wind ????Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194962 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27194962 #FOAvip English Wikipedia <ref>{{Cite pmid|27194962}}</ref> Wave Modeling of the Solar Wind #MMPMID27194962 Ofman L Living Rev Sol Phys 2010[]; 7 (ä): ä PMID27194962show ga The acceleration and heating of the solar wind have been studied for decades using satellite observations and models. However, the exact mechanism that leads to solar wind heating and acceleration is poorly understood. In order to improve the understanding of the physical mechanisms that are involved in these processes a combination of modeling and observational analysis is required. Recent models constrained by satellite observations show that wave heating in the low-frequency (MHD), and high-frequency (ion-cyclotron) range may provide the necessary momentum and heat input to coronal plasma and produce the solar wind. This review is focused on the results of several recent solar modeling studies that include waves explicitly in the MHD and the kinetic regime. The current status of the understanding of the solar wind acceleration and heating by waves is reviewed. äWave Modeling of the Solar Wind (epmc).pdf DeepDyve Pubget Overpricing