Published 1980 | Version v1
Report Open

3. Nonlinear development of a gasdynamical instability

Creators

Description

The problem on solar spots formation caused by the development of a convective instability is considered. The magnetic field strengthening effect is explained by a magnetic flux pushing off from a large area. Problems on waterspout formation because of gasodynamical instability development are studied. The generation of great rotation velocities is connected with pushing off from a great rotary moment volume. The development of connective instability in a gravitating gas ball (star) which results in surfacing internal gas hot layers which must increase a star luminosity by many orders is analyzed

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Additional titles

Original title (Russian)
3. Нелинейное развитие газодинамических неустойчивостей

Publishing Information

Imprint Pagination
56 p.
Report number
IAE--3289/6

INIS

Country of Publication
USSR
Country of Input or Organization
USSR
INIS RN
13655040
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BOUNDARY CONDITIONS; CONVECTIVE INSTABILITIES; EQUATIONS OF MOTION; GRAVITATION; KINETIC ENERGY; MAGNETIC FIELDS; MAGNETIC FLUX; NONLINEAR PROBLEMS; NUMERICAL SOLUTION; ORIGIN; SOLAR FLARES; STARS; SUNSPOTS; TIME DEPENDENCE; VARIATIONAL METHODS; VELOCITY
Descriptors DEC
DIFFERENTIAL EQUATIONS; ENERGY; EQUATIONS; INSTABILITY; PLASMA INSTABILITY; SOLAR ACTIVITY

Optional Information

Notes
8 refs.; 27 figs.