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A Solar Dynamo Model Driven by Mean-Field Alpha and Babcock-Leighton Sources: Fluctuations, Grand-Minima-Maxima and Hemispheric Asymmetry in Sunspot Cycles

机译:由mean-Field alpha和Babcock-Leighton驱动的太阳能发电机模型   来源:波动,大最小 - 千里马和半球不对称   太阳黑子周期

摘要

Extreme solar activity fluctuations and the occurrence of solar grand minimaand maxima episodes, are well established, observed features of the solarcycle. Nevertheless, such extreme activity fluctuations and the dynamics of thesolar cycle during Maunder minima-like episodes remain ill-understood. Weexplore the origin of such extreme solar activity fluctuations and the role ofdual poloidal field sources, namely the Babcock-Leighton mechanism and themean-field alpha effect in the dynamics of the solar cycle. We mainlyconcentrate on entry and recovery from grand minima episodes such as theMaunder minimum and the dynamics of the solar cycle. We use a kinematic solardynamo model with a novel set-up in which stochastic perturbations force twodistinct poloidal field alpha effects. We explore different regimes ofoperation of these poloidal sources with distinct operating thresholds, toidentify the importance of each. The perturbations are implementedindependently in both hemispheres which allows one to study the level ofhemispheric coupling and hemispheric asymmetry in the emergence of sunspots.From the simulations performed we identify a few different ways in which thedynamo can enter a grand minima episode. While fluctuations in any of the$\alpha$ effects can trigger intermittency we find that the mean-field alphaeffect is crucial for the recovery of the solar cycle from a grand minimaepisode which a Babcock-Leighton source alone, fails to achieve. Oursimulations also demonstrate other cycle dynamics. We conclude that stochasticfluctuations in two interacting poloidal field sources working with distinctoperating thresholds is a viable candidate for triggering episodes of extremesolar activity and that the mean-field alpha effect capable of working on weak,sub-equipartition fields is critical to the recovery of the solar cyclefollowing an extended solar minimum.
机译:太阳活动周期的极端特征是极端的太阳活动波动和太阳大极小值和极大值事件的发生。然而,这种极端的活动性波动和类似Maunder极小现象的发作期间的太阳周期动力学仍然缺乏理解。我们探索了这种极端的太阳活动波动的起因,以及双极电场场源的作用,即,Babcock-Leighton机理和主题场阿尔法效应在太阳周期动力学中的作用。我们主要集中于从极小事件的进入和恢复,如Maunder极小值和太阳周期的动力学。我们使用具有新颖设置的运动学日光发电模型,其中随机扰动迫使两个截然不同的极向场阿尔法效应。我们用不同的操作阈值探索这些多倍体来源的不同操作方式,以识别每种方法的重要性。扰动是在两个半球中独立实现的,这使人们可以研究黑子出现时的半球耦合水平和半球不对称性。从执行的模拟中,我们确定了发电机可以进入极小值的几种不同方式。尽管任何α效应的波动都可以触发间歇性,但我们发现,平均场α效应对于仅从Babcock-Leighton光源无法实现的宏伟的小型旋律恢复太阳周期至关重要。我们的模拟还演示了其他循环动力学。我们得出的结论是,在两个具有不同操作阈值的相互作用的极向场源中,随机波动是触发极端太阳活动发作的可行候选者,并且能够在弱,亚等分场上起作用的平均场阿尔法效应对于太阳能的恢复至关重要。遵循延长的日照最小值。

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