Published 1989
| Version v1
Book
On the origin of solar wind turbulence
Creators
- 1. Observatoire de Paris, 92 - Meudon (France)
- 2. Max-Planck-Institut fuer Aeronomie, Katlenburg-Lindau (Germany, F.R.)
Description
The spectra of velocity and magnetic field fluctuations in de Solar Wind strongly suggests fully developed turbulence, as they cover several decades of frequencies. The possibility that nonlinear interactions play a rolein the origin of this turbulence is investigated by revisiting the Helios data. (H.W.). 16 refs.; 4 figs.; 1 tab
Additional details
Additional titles
- Subtitle (English)
- Helios data revisited
Publishing Information
- Publisher
- North-Holland.
- Imprint Place
- Amsterdam (Netherlands)
- ISBN
- 0 444 87396 1
- Imprint Title
- Turbulence and non-linear dynamics in MHD flows
- Imprint Pagination
- 288 p.
- Series
- North-Holland Delta Series.
- Journal Page Range
- p. 81-86.
Conference
- Title
- Workshop on turbulence and nonlinear dynamics in MHD flows.
- Dates
- 4-8 Jul 1988.
- Place
- Cargese (France).
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 21048170
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S30: DIRECT ENERGY CONVERSION;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; SOLAR WIND; SPECTRA; TURBULENCE
- Descriptors DEC
- FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS
Optional Information
- Notes
- Imprint:Includes author index and subject index.