What is recorded here?
Developed hydromagnetic models for the regeneration and amplification of magnetic fields in rotating conducting fluids, including wave-like behavior connected to solar magnetic activity.
Source-linked catalogue note. A detailed explanatory guide has not yet been prepared for this entry.
Scientific scope
The record is the exact 1955 Astrophysical Journal paper. Earlier dynamo ideas, later mean-field dynamo theory, observations and numerical simulations remain separate.
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People and systems
Eugene N. Parker
The named authors contributed to this scoped work; individual effort shares and later applications are not assigned by the byline.
Research locations and affiliations
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Documented countries / regions: United States
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English catalogue narrative
Parker: hydromagnetic dynamo models
Developed hydromagnetic models for the regeneration and amplification of magnetic fields in rotating conducting fluids, including wave-like behavior connected to solar magnetic activity.
Scientific scope
The record is the exact 1955 Astrophysical Journal paper. Earlier dynamo ideas, later mean-field dynamo theory, observations and numerical simulations remain separate.
Reading status
This is a source-linked WRS catalogue note. A full explanatory guide and independent scientific reconstruction have not been completed for this entry. Read the identified original work for its complete narrative and arguments.
People and systems
Eugene N. Parker
The named authors contributed to this scoped work; individual effort shares and later applications are not assigned by the byline.