166 citations · 1.1k across the 31 of their papers we have counts for
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Nonlinear dynamo models using quasi-biennial oscillations constrained by sunspot area data
Fadil Inceoglu, Rosaria Simoniello, Rainer Arlt +1
Contex: Solar magnetic activity exhibits variations with periods between 1.5--4 years, the so-called quasi-biennial oscillations (QBOs), in addition to the well-known 11-year Schwa…
22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics
Kiran Jain, Sushanta Tripathy, Rudolf Komm +2
Using continuous observations for 22 years from ground-based network GONG and space-borne instruments MDI onboard {\it SoHO} and HMI onboard {\it SDO}, we report both global and lo…
A New Challenge to Solar Dynamo Models from Helioseismic Observations: The Latitudinal Dependence of the Progression of the Solar Cycle
R. Simoniello, S. C. Tripathy, K. Jain +1
The solar cycle onset at mid-latitudes, the slow down of the sunspot drift toward the equator, the tail-like attachment and the overlap of successive cycles at the time of activity…
On the current solar magnetic activity in the light of its behaviour during the Holocene
F. Inceoglu, R. Simoniello, M. F. Knudsen +3
Solar modulation potential (SMP) reconstructions based on cosmogenic nuclide records reflect changes in the open solar magnetic field and can therefore help us obtain information o…
Properties of 42 Solar-type Kepler Targets from the Asteroseismic Modeling Portal
T. S. Metcalfe, O. L. Creevey, G. Dogan +39
Recently the number of main-sequence and subgiant stars exhibiting solar-like oscillations that are resolved into individual mode frequencies has increased dramatically. While only…
Towards solar activity maximum 24 as seen by GOLF and VIRGO/SPM instruments
R. A. Garcia, D. Salabert, S. Mathur +5
All p-mode parameters vary with time as a response to the changes induced by the cyclic behavior of solar magnetic activity. After the unusual long solar-activity minimum between c…