170 citations · 1.3k across the 27 of their papers we have counts for
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Power spectra of solar brightness variations at different inclinations
N. -E. Nèmec, A. I. Shapiro, N. A. Krivova +4
Magnetic features on the surfaces of cool stars cause variations of their brightness. Such variations have been extensively studied for the Sun. Recent planet-hunting space telesco…
Origin of the hemispheric asymmetry of solar activity
M. Schüssler, R. H. Cameron
The frequency spectrum of the hemispheric asymmetry of solar activity shows enhanced power for the period ranges around 8.5 years and between 30 and 50 years. This can be understoo…
The nature of solar brightness variations
A. I. Shapiro, S. K. Solanki, N. A. Krivova +3
The solar brightness varies on timescales from minutes to decades. Determining the sources of such variations, often referred to as solar noise, is of importance for multiple reaso…
Observing and modeling the poloidal and toroidal fields of the solar dynamo
R. H. Cameron, T. L Duvall, M. Schüssler +1
Context. The solar dynamo consists of a process that converts poloidal field to toroidal field followed by a process which creates new poloidal field from the toroidal field. Aims.…
An update of Leighton's solar dynamo model
R. H. Cameron, M. Schuessler
In 1969 Leighton developed a quasi-1D mathematical model of the solar dynamo, building upon the phenomenological scenario of Babcock(1961). Here we present a modification and exten…
Observed and Simulated Power Spectra of Kinetic and Magnetic Energy retrieved with 2D inversions
S. Danilovic, M. Rempel, M. van Noort +1
We try to retrieve the power spectra with certainty to the highest spatial frequencies allowed by current instrumentation. For this, we use 2D inversion code that were able to reco…