Waveform and envelope field statistics for waves with stochastically driven amplitudes
- 1. School of Physics, University of Sydney, Sydney, New South Wales 2006 (Australia)
- 2. Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire 03755 (United States)
- 3. Department of Physics, University of Iowa, Iowa City, Iowa 52242 (United States)
Description
The statistically steady distributions P(log E) and Pe(log Ee) of waveform field E and envelope field Ee are studied for time-varying waves with stochastically driven amplitudes. The waves are represented in one dimension (1D) by a single mode or superposition of multiple independent modes, whose amplitudes follow stochastic differential equations. Both distributions at low fields follow power laws: P(log E)∝Ep and Pe(log Ee)∝Eeq with distinct exponents p and q. Transitions in both distributions are found between the single-mode and multimode cases, with the distributions in the latter essentially independent of the number N (provided N≥2) of modes. For N≥2, p≅+1.0, q≅+2.0, and both distributions agree quantitatively with independent analytic predictions. Applications to Langmuir waves observed in Earth's polar cusp ionosphere show that both distributions for N≥2 agree quantitatively with the respective observations, suggesting that the Langmuir waves may be 1D and have a stochastic driver.
Additional details
Identifiers
- DOI
- 10.1063/1.3353092;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 17
- Journal Issue
- 3
- Journal Page Range
- p. 032110-032110.14
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41078357
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- DIFFERENTIAL EQUATIONS; DISTRIBUTION; IONOSPHERE; PLASMA SIMULATION; PLASMA WAVES; POLAR CUSP; STOCHASTIC PROCESSES; WAVE FORMS
- Descriptors DEC
- EARTH ATMOSPHERE; EQUATIONS; SIMULATION
Optional Information
- Notes
- (c) 2010 American Institute of Physics