Free Newsletters - Space News - Defense Alert - Environment Report - Energy Monitor
by Staff Writers
Bochum, Germany (SPX) Oct 17, 2012
Dusty plasmas can be found in many places both in space and in the laboratory. Due to their special properties, dust acoustic waves can propagate inside these plasmas like sound waves in air, and can be studied with the naked eye or with standard video cameras.
The RUB physicists Prof. Dr. Dr. h.c. Padma Kant Shukla and Dr. Bengt Eliasson from the Faculty of Physics and Astronomy have published a model with which they describe how large amplitude dust acoustic waves in dusty plasmas behave. The researchers report their new findings in the journal Physical Review E.
Different acoustic phenomena in dusty plasmas
Recently, several laboratory experiments revealed nonlinear dust acoustic waves with extremely large amplitudes in the form of dust acoustic solitary pulses and shock waves, propagating in the plasma with speeds of a few centimeters per second. Padma Shukla and Bengt Elisasson have developed a unified theory explaining under which circumstances nonlinear dust acoustic shocks as well as dust acoustic solitary pulses occur in dusty plasmas.
Acoustic waves interacting with themselves
Due to the generation of harmonics (i.e., waves with frequencies that are a multiple integer of the original frequency) and due to constructive interference between dust acoustic waves of different wavelengths, the waves develop into solitary, spiky pulses, or into shock waves. The solitary pulses arise from a balance between the harmonic generation nonlinearities and the dust acoustic wave dispersion.
Shock waves, on the other hand, form when the dust fluid viscosity dominates over dispersion. This happens at high dust densities when the dust particles are close enough to interact and collide with neighboring dust particles.
Theory successfully explains data from experiments
These three international groups described the existence of large amplitudes dust acoustic solitary pulses and dust acoustic shocks in their low-temperature dusty plasmas. Applying the new nonlinear dust acoustic wave theory, one can infer the dust fluid viscosity from the width of the dust acoustic shock wave.
"Our results may also be important as a possible mechanism for understanding the cause of dust grain clustering and dust structuring in planets and in star forming regions," suggests Prof. Padma Kant Shukla.
Existence of dusty acoustic waves predicted more than two decades ago
APS Fellowship for contributions to computational and nonlinear plasma physics
The number of Fellows that are annually elected is less than one percent of the current number of APS members. Dr. Bengt Eliasson graduated with a Master degree in Engineering Physics from Uppsala University, Sweden, where he also obtained his PhD degree in Numerical Analysis. Since 2003, he works in the Faculty of Physics and Astronomy at the Ruhr-Universitat Bochum.
The contributions of Dr. Bengt Eliasson to various fields of space and plasma physics range from large-scale simulations of the Earth's ionosphere to new theoretical and numerical models of quantum plasmas at nanoscales.
The results of his research projects have been published in approximately 150 articles in refereed journals and he was invited to give talks at the European Geophysical Union, European Physical Society, American Physical Society, International Congress on Plasma Physics, and other meetings.
P. K. Shukla, B. Eliasson (2012): Nonlinear dynamics of large-amplitude dust acoustic shocks and solitary pulses in dusty plasmas, doi: 10.1103/PhysRevE.86.046402
Explore The Ring World of Saturn and her moons
Jupiter and its Moons
The million outer planets of a star called Sol
News Flash at Mercury
|The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement|