Corpus ID: 222407339

Der gegenwärtige Stand der Theorie konvektiver Sonnenmodelle

@inproceedings{Biermann1941DerGS,
  title={Der gegenw{\"a}rtige Stand der Theorie konvektiver Sonnenmodelle},
  author={L. Biermann},
  year={1941}
}
19 Citations
Highly Influential Citations
3
Background Citations
8
Methods Citations
3
Results Citations
1

19 Citations

Citation Type

Citation Type

Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH
  • 1
  • Highly Influenced
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Coronal heating problem solution by means of axion origin photons
  • Highly Influenced
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Magnetic and Velocity Field of Sunspots in the Photosphere and Upper Chromosphere
  • 2
  • Highly Influenced
Anticorrelation of Variations of the Magnetic Field of a Sunspot and the Brightness of Its Umbra in Long-Period Sunspot Oscillations
Relationship of the Magnetic-Field Strength and the Brightness of the Sunspot Umbra and the Center of a Facular Knot
Non-axisymmetric Magnetic Flux Transport in the Sun
Normal and counter Evershed flows in the penumbra of sunspots: HINODE observations and MHD simulations
Simulations of Flux Emergence in Cool Stars : What ’ s Convection , Rotation , and Stellar Structure got to do with it ?
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The small-scale structure of photospheric convection retrieved by a deconvolution technique applied to Hinode/SP data
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No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry
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