Andere Kunden interessierten sich auch für
![Analog Computing Techniques Applied to Atmospheric Diffusion [electronic Resource]: Continuous Line Source]( "Analog Computing Techniques Applied to Atmospheric Diffusion [electronic Resource]: Continuous Line Source")
Analog Computing Techniques Applied to Atmospheric Diffusion [electronic Resource]: Continuous Line Source17,99 €![An Interpolation Procedure for Calculating Atmospheric Band Aborptions From Laboratory Data; NBS Technical Note 178]( "An Interpolation Procedure for Calculating Atmospheric Band Aborptions From Laboratory Data; NBS Technical Note 178")
An Interpolation Procedure for Calculating Atmospheric Band Aborptions From Laboratory Data; NBS Technical Note 17815,99 €![The Dynamics of Long Waves in a Barotropic Westerly Current With a Three-dimensional Velocity Perturbation.]( "The Dynamics of Long Waves in a Barotropic Westerly Current With a Three-dimensional Velocity Perturbation.")
The Dynamics of Long Waves in a Barotropic Westerly Current With a Three-dimensional Velocity Perturbation.19,99 €![Atmospheric Processes]( "Atmospheric Processes")
Atmospheric Processes50,99 €![On Forecasting the Movement of Long Waves in the Westerlies at the 500 Millibar Level]( "On Forecasting the Movement of Long Waves in the Westerlies at the 500 Millibar Level")
On Forecasting the Movement of Long Waves in the Westerlies at the 500 Millibar Level15,99 €![What Really Causes Global Warming?]( "What Really Causes Global Warming?")
What Really Causes Global Warming?25,99 €![The Future of Atmospheric Boundary Layer Observing, Understanding, and Modeling]( "The Future of Atmospheric Boundary Layer Observing, Understanding, and Modeling")
The Future of Atmospheric Boundary Layer Observing, Understanding, and Modeling44,99 €
![Analog Computing Techniques Applied to Atmospheric Diffusion [electronic Resource]: Continuous Line Source](https://bilder.buecher.de/produkte/66/66192/66192556m.jpg "Analog Computing Techniques Applied to Atmospheric Diffusion [electronic Resource]: Continuous Line Source")
Corona, the outermost layer of the solar atmosphere, is made up with very hot and taneous plasma material. The density and temperature structuring of this layer, is largely inhomogenous. Temperatures, at certain locations, can reach upto tens of million kelvin (MK). One of the key questions regarding the coronal physics is to identify the ubiquitous source(s) which can sustain this high temperature profile of the coronal plasma. One of the potential candidates in this case, is the family of magnetohydrodynamic (MHD) waves. These waves can propagate from the lower atmosphere to the solar corona and can partially (or fully) dissipate their energy to the surrounding coronal medium. In fact, different physical parameters such as the density, magnetic field and temperature of the host structure can also be inferred by studying the different properties of the propagating MHD wave