311 research outputs found
Effect of suppressed excitation on the amplitude distribution of 5-min oscillations in sunspots
Five-minute oscillations on the Sun (acoustic and surface gravity waves) are
excited by subsurface turbulent convection. However, in sunspots the excitation
is suppressed because strong magnetic field inhibits convection. We use 3D
simulations to investigate how the suppression of excitation sources affects
the distribution of the oscillation power in sunspot regions. The amplitude of
random acoustic sources was reduced in circular-shaped regions to simulate the
suppression in sunspots. The simulation results show that the amplitude of the
oscillations can be approximately 2-4 times lower in the sunspot regions in
comparison to the quiet Sun, just because of the suppressed sources. Using
SOHO/MDI data we measured the amplitude ratio for the same frequency bands
outside and inside sunspots, and found that this ratio is approximately 3-4.
Hence, the absence of excitation sources inside sunspots makes a significant
contribution (about 50% or higher) to the observed amplitude ratio and must be
taken into account in sunspot seismology.Comment: 12 pages, 5 figures, accepted to ApJ
Prediction of Sunspot Cycles by Data Assimilation Method
Despite the known general properties of the solar cycles, a reliable forecast
of the 11-year sunspot number variations is still a problem. The difficulties
are caused by the apparent chaotic behavior of the sunspot numbers from cycle
to cycle and by the influence of various turbulent dynamo processes, which are
far from understanding. For predicting the solar cycle properties we make an
initial attempt to use the Ensemble Kalman Filter (EnKF), a data assimilation
method, which takes into account uncertainties of a dynamo model and
measurements, and allows to estimate future observational data. We present the
results of forecasting of the solar cycles obtained by the EnKF method in
application to a low-mode nonlinear dynamical system modeling the solar
-dynamo process with variable magnetic helicity. Calculations of
the predictions for the previous sunspot cycles show a reasonable agreement
with the actual data. This forecast model predicts that the next sunspot cycle
will be significantly weaker (by ) than the previous cycle,
continuing the trend of low solar activity.Comment: 10 pages, 3 figure
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