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Structure of convective flows on supergranular scales in the solar photosphere
The exploration of the velocity field of the real solar convection was performed using neutral iron line λ ≈ 639.3 nm profile from the observations with high spatial resolution. The inverse procedure was applied for each profile to reproduce the velocity field in the solar photosphere. Acoustic wave...
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Main Author: | |
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Format: | Article |
Language: | English |
Published: |
Головна астрономічна обсерваторія НАН України
2012
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Series: | Advances in Astronomy and Space Physics |
Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/119189 |
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