The evolution of magnetic network elements in the quiet Sun

Details The evolution of magnetic network elements in the quiet Sun The evolution of magnetic network elements in the quiet Sun

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..215l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 283, no. 1, p. 215-220

Astronomy and Astrophysics

Astrophysics

17

Photosphere, Solar Magnetic Field, Sun, Magnetic Flux, Magnetic Signatures

Scientific paper

Using the 155-h coordinated magnetograph data of Huairou and Big Bear Solar Observatories, we have studied the evolution and lifetime of magnetic network elements in an enhanced network region. Both statistical and counting methods give a mean lifetime of network elements of 50h. The network elements are divided into two categories according to their evolution: 'breakup' and 'merging'. They have similar average lifetimes. We also find that the number of the elements that disappear by merging is about twice that by breakup. This may indicate that the creation and disappearance of magnetic network elements are balanced.

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