The Time Dependence of Magnetic, Velocity, and Intensity Fields in the Solar Atmosphere
- 1 January 1971
- journal article
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 43, 310-315
- https://doi.org/10.1017/s0074180900022749
Abstract
Spectroheliogram movies of magnetic, velocity, and intensity fields have been obtained in a wide variety of spectral lines. The time resolution was typically 10–30 s. Some of the lines used were: CN λ 3883; CaI λ 6103; FeI λ 4071; FeI λ 5434; FeII λ 4924; CaII λ 3934; CaII λ 8542.Keywords
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- Simultaneous measurements of magnetic fields and brightness fields using a 4-image spectroheliographSolar Physics, 1970
- The evolution of the photospheric networkSolar Physics, 1969
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