A new model of spicule formation in the Sun chromosphere

Details A new model of spicule formation in the Sun chromosphere A new model of spicule formation in the Sun chromosphere

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311...25p&link_type=abstract

In ESA, Plasma Astrophysics p 25-27 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Chromosphere, Mathematical Models, Solar Atmosphere, Spicules, Boundary Layers, Coriolis Effect, Granular Materials, Magnetic Fields

Scientific paper

The physical processes occurring in the supergranule boundary cylinder layer are investigated. Taking into account the Coriolis force an expression for the phi component of the magnetic field and velocity are obtained. The estimated number of the spicules coming on each supergranule cell depends on the solar latitude theta. The time scale of the formation and the coalescence of the magnetic tubes is of the order of the observed life time of the spicules.

Affiliated with

Also associated with

No associations

Rating

A new model of spicule formation in the Sun chromosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A new model of spicule formation in the Sun chromosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A new model of spicule formation in the Sun chromosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1126789