A mechanism for the formation of loop prominences

Details A mechanism for the formation of loop prominences A mechanism for the formation of loop prominences

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..283i&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 3, June 1977, p. 283-286.) Soviet Astronomy Letters, vol. 3, May-June 1977, p. 150-152.

Astronomy and Astrophysics

Astronomy

Loops, Solar Magnetic Field, Solar Prominences, Stellar Models, Kinematics, Lines Of Force, Magnetic Dipoles, Mass Transfer, Solar Corona, Sunspots, Two Dimensional Flow

Scientific paper

The kinematics of mass motion in the variable magnetic field of two
point dipoles is investigated. In the magnetohydrodynamic approximation
of a strong field and cool plasma, it is established that an increase in
the magnetic moments can result in the development of such phenomena as
loop prominences and coronal rain.

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