Results 1 to 10 of about 28,762 (292)
In 1844 Schwabe discovered that the number of sunspots increased and decreased over a period of about 11 years, that variation became known as the sunspot cycle.
Abhishek K. Srivastava +19 more
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This paper summarizes the body of work that we have done over the years on the oscillation processes in sunspots, including their umbra, penumbra, and close vicinity.
Chelpanov A.A.
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The magnetic origin of the outer boundaries of sunspots
Context. Sunspot boundaries are commonly outlined by contours of the continuum intensity. However, their magnetic nature has not yet been fully characterised. Aims.
Schmassmann Markus +3 more
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Deciphering transmission spectra by exploring the solar paradigm
Aims. Transmission spectroscopy allows to measure the wavelength dependence of the transit signal of an exoplanet, thus enabling probing of its atmospheric composition.
Nèmec N.-E. +3 more
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Observations at (sub-)millimeter wavelengths offer a complementary perspective on our Sun and other stars, offering significant insights into both the thermal and magnetic composition of their chromospheres.
Sven Wedemeyer +37 more
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Observations of the Formation of a Proto-Spot in a Pre-Existing Field Environment
Bipolar emerging flux regions (EFRs) form active regions (ARs) that generally evolve into a pre-existing magnetic environment in the solar atmosphere. Reconfiguration of the small- and large-scale magnetic connectivities is invoked to explain a plethora ...
Mariarita Murabito +4 more
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Solar Surface Magneto-Convection
We review the properties of solar magneto-convection in the top half of the convection zones scale heights (from 20 Mm below the visible surface to the surface, and then through the photosphere to the temperature minimum).
Robert F. Stein
doaj
Where are Sunspots? The Practical Method of Galileo as an example of Mental Model
After the publication of Sidereus Nuncius, in the controversy with Ch. Scheiner, Galileo developed several arguments on behalf of the hypothesis that sunspots are contiguous to the surface of the Sun, and presented them in his Istoria e dimostrazioni ...
Tadeusz Sierotowicz
doaj
Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]
Toriumi S, Hotta H, Kusano K.
europepmc +1 more source
Characterizing the Solar Activity Using the Visibility Graph Method. [PDF]
Zurita-Valencia T, Muñoz V.
europepmc +1 more source

