This book is concerned with Ultra-Low-Frequency (ULF)-electromagnetic
waves observed on the Earth and in Space. These are so-called geomagnetic
variations or pulsations. Alfv´en’s discovery related to the influence of the
strong magnetic field on the conducting fluids (magnetohydrodynamics) led
to development of the concept that the ULF-waves are magnetospheric magnetohydrodynamic
MHD-waves at their propagation gather information about the magnetosphere,
ionosphere, and the ground. There are two applied aspects based on
using the ULF electromagnetic oscillations.
Tuyển tập báo cáo các nghiên cứu khoa học quốc tế ngành hóa học dành cho các bạn yêu hóa học tham khảo đề tài:
Research Article Global Existence and Uniqueness of Strong Solutions for the Magnetohydrodynamic Equations
Tuyển tập báo cáo các nghiên cứu khoa học quốc tế ngành hóa học dành cho các bạn yêu hóa học tham khảo đề tài: Research Article Variable Viscosity on Magnetohydrodynamic Fluid Flow and Heat Transfer over an Unsteady Stretching Surface with Hall Effect
Bài giảng Từ thủy động lực học (Magnetohydrodynamic) do Phạm Thanh Tâm biên soạn sau đây sẽ cung cấp cho các bạn những kiến thức về lịch sử của MHD; PLASMA = Magneto + hydrodynamic equations. Mời các bạn tham khảo bài giảng để hiểu rõ hơn về những nội dung này.
In this book, the chapters have been grouped as part according to the following
themes: Optical Communications Systems: Part 1, General Concepts; Optical
Communications Systems: Part 2, Amplifiers and Networks; Optical
Communications Systems: Part 3, Optical Multiplexing and Demultiplexing; Optical
Communications Systems: Part 4, Network Traffic. These categorisations of parts are
not fully perfect because some of the chapters are mixed i.e., like an inter-
What is computational physics? Here, we take it to mean techniques for simulating
continuous physical systems on computers. Since mathematical physics
expresses these systems as partial differential equations, an equivalent statement
is that computational physics involves solving systems of partial differential
equations on a computer.
This book is meant to provide an introduction to computational physics
to students in plasma physics and related disciplines. We present most of the
basic concepts needed for numerical solution of partial differential equations.
This textbook is intended as an introduction to the physics of solar and stellar
coronae, emphasizing kinetic plasma processes. It is addressed to observational
astronomers, graduate students, and advanced undergraduates without a background
in plasma physics.
Coronal physics is today a vast field with many different aims and goals. Sorting
out the really important aspects of an observed phenomenon and using the
physics best suited for the case is a formidable problem.