Results 341 to 350 of about 1,589,837 (361)

Magnetic Fields of the Solar Atmosphere

1994
The Sun is enveloped in a thick atmosphere which can be divided into the following three layers. As the lowest part, the photosphere has a thickness of only about 500 km. Above it is the chromosphere with a thickness of approximately 20,000 km. The outmost part is the corona, which has a scope of several to ten more solar radii.
openaire   +2 more sources

On the small-scale structure of solar magnetic fields

, 1972
E. Frazier, J. Stenflo
semanticscholar   +1 more source

Magnetic Fields of the Solar System

1994
In the preceding four chapters we have presented a comprehensive and overall description of the solar magnetic field. This chapter will be devoted to the magnetic fields of the other celestial bodies in the solar system as well as of interplanetary space.
openaire   +2 more sources

On the filamentary nature of solar magnetic fields

, 1972
R. Howard, J. Stenflo
semanticscholar   +1 more source

The magnetic field of the solar corona

2008
The structure of the solar corona, on all observable scales, is intimately controlled by the magnetic field. Although direct measurements of the magnetic field are from difficult to impossible, its presence is evident in all spectral ranges where the corona is observable. This review discusses the measurement of coronal magnetic fields and the indirect
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Observations of small-scale solar magnetic fields

, 1967
N. Sheeley
semanticscholar   +1 more source

Studies of solar magnetic fields

, 1974
R. Howard
semanticscholar   +1 more source

A model combining the polar and the sector structured solar magnetic fields

, 1974
L. Svalgaard, J. Wilcox, T. L. Duvall
semanticscholar   +1 more source

Global resonances in the evolution of solar magnetic fields

Nature, 1986
J. Stenflo, M. Vogel
semanticscholar   +1 more source

Coronal holes and solar magnetic fields

, 1979
J. Harvey, N. Sheeley
semanticscholar   +1 more source