Published March 2010 | Version v1
Journal article

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

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