Unusual Polar Conditions in Solar Cycle 24 and their Implications for Cycle 25
arXiv:1605.02217 · doi:10.3847/2041-8205/823/1/L15
Abstract
We report on the prolonged solar-maximum conditions until late 2015 at the north-polar region of the Sun indicated by the occurrence of high-latitude prominence eruptions and microwave brightness temperature close to the quiet Sun level. These two aspects of solar activity indicate that the polarity reversal was completed by mid-2014 in the south and late 2015 in the north. . The microwave brightness in the south-polar region has increased to a level exceeding the level of cycle 23/24 minimum, but just started to increase in the north. The north-south asymmetry in the polarity reversal has switched from that in cycle 23. These observations lead us to the hypothesis that the onset of cycle 25 in the northern hemisphere is likely to be delayed with respect to that in the southern hemisphere. We find that the unusual condition in the north is a direct consequence of the arrival of poleward surges of opposite polarity from the active region belt. We also find that multiple rush-to-the-pole episodes were indicated by the prominence eruption locations that lined up at the boundary between opposite polarity surges. The high-latitude prominence eruptions occurred in the boundary between the incumbent polar flux and the insurgent flux of opposite polarity.
12 pages, 4 figures, 1 table, Accepted for publication in ApJ Lett. on May 6, 2016
References in corpus (9)
- The Solar Cycle
- The crucial role of surface magnetic fields for the solar dynamo
- Solar Cycle Propagation, Memory, and Prediction: Insights from a Century of Magnetic Proxies
- On Polar Magnetic Field Reversal and Surface Flux Transport During Solar Cycle 24
- The cause of the weak solar cycle 24
- Source of a Prominent Poleward Surge During Solar Cycle 24
- Forecasting the Maxima of Solar Cycle 24 with Coronal Fe XIV Emission
- Kinematic and Energetic Properties of the 2012 March 12 Polar Coronal Mass Ejection
- The 17 GHz active region number
Cited by in corpus (18)
- Impact of Space Weather on Climate and Habitability of Terrestrial Type Exoplanets
- Solar cycle 24: an unusual polar field reversal
- Evidence for a New Component of High-Energy Solar Gamma-Ray Production
- Long-term Solar Activity Studies using Microwave Imaging Observations and Prediction for Cycle 25
- On Polar Magnetic Field Reversal in Solar Cycles 21, 22, 23, and 24
- Magnetic Structures at the Boundary of the Closed Corona: Interpretation of S-web Arcs
- Another Mini Solar Maximum in the Offing: A Prediction for the Amplitude of Solar Cycle 25
- The Association of Filaments, Polarity Inversion Lines, and Coronal Hole Properties with the Sunspot Cycle: An Analysis of the McIntosh Database
- On the Shock Source of Sustained Gamma-Ray Emission from the Sun
- Collective Study of Polar Crown Filaments in the Past Four Solar Cycles
- Structure and evolution of the photospheric magnetic field in 2010 - 2017: comparison of SOLIS/VSM vector field and potential field
- A Catalog of Prominence Eruptions Detected Automatically in the SDO/AIA 304 Å Images
- The Characteristics of Valley Phase as Predictor of the Forthcoming Solar Cycle
- Polarity imbalance of the photospheric magnetic field
- Comparative Study of Microwave Polar Brightening, Coronal Holes, and Solar Wind Over the Solar Poles
- Coronal mass ejections as a new indicator of the active Sun
- Ripples and Rush-to-the-Poles in the photospheric magnetic field
- Asymmetric Distribution of the Solar Photospheric Magnetic Field Values