Scientists have developed a new theoretical model for measuring congestion in the solar corona produced by a disorder in the electric fluid, a magnetic field that exists as plasma.The solar corona is a very powerful method. It has been well established since a few decades ago that electromagnetic fluid, a magnetic field such as plasma that causes magneto-hydrodynamic (MHD) wave turbulence, plays a vital role in warming the solar corona by millions of degrees.
Temperature is a thousand times more than a solar system. The exact reason for heating the sun corona at such a high temperature is still an open question and is known as the ‘problem of coral heating’ in the solar physics community.
The moving movements of the liquid are characterized by dramatic changes in pressure and flow velocity. However, because of the extremely hot temperatures in the solar corona, the material in the solar corona becomes like a soup of charged particles, called plasma. The distribution of MHD waves in the plasma area can cause confusion. When the MHD-wave differs in space, it carries energy, and the amount of energy depends on the growth of medium inhomogeneity.
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Scientists from the Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, an independent institution under the auspices of the Department of Science and Technology, Government of India, have developed a new method of measuring density inhomogeneity in the solar system, not to mention. by the density filling factor (the fraction of the volume taken by the overcrowded regions in relation to the total volume). This method involves the imitation of numbers.
This model, Developed by Drs. Samrat Sen, a post-doctoral researcher at KU Leuven, Belgium, and Drs. Vaibhav Pant, published in the Astrophysical Journal, discusses two different ways to calculate the component filling component. One of the methods involves calculating the component filling factor from the local scale obtained from the simulated data. Although, in the second method, advanced modeling (the use of a particular model to produce an effect according to users’ preferences) used spectroscopic measurements to measure the complement factor component.
The researchers found that the theoretical values ​​were consistent with the values ​​observed in the solar corona. According to research, the chaos driven by the MHD wave increases the filling factor of the most dense structures, and the medium becomes more congested.
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