Small-Scale Photospheric Fields: Observational Evidence and Numerical Simulations

Details Small-Scale Photospheric Fields: Observational Evidence and Numerical Simulations Small-Scale Photospheric Fields: Observational Evidence and Numerical Simulations

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...560l.197e&link_type=abstract

The Astrophysical Journal, Volume 560, Issue 2, pp. L197-L200.

Astronomy and Astrophysics

Astronomy

56

Convection, Magnetohydrodynamics: Mhd, Sun: Magnetic Fields, Sun: Photosphere

Scientific paper

Observations suggest that magnetic fields at the solar photosphere may
be structured below the limit of the present resolution. We argue that
numerical simulations could be used in a complementary way to
observations in order to study the small-scale structure of photospheric
fields. We present a number of illustrative examples.

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