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The CAWSES project in 2004 2008 and CAWSES phase II in 2009 2013 were conducted during the decreasing and rising phases of solar cycles 23 and 24, respectively B. CAWSES II: toward the solar maximum .
The data cover the pre-flare phase in the periods of 30 90 minutes preceding the flares, the rising phases, and the peaks of flares in X-ray intensity, and the beginnings of the decay phases.
The solar cycles represented by the monthly averaged sunspot numbers show characteristic nonlinear manifestations: a) non-sinusoidal time dependence with shorter rising phases and longer declining phases of moderate and strong cycles; b) smoother minima than maxima.
We present a comparative study of the properties of coronal mass ejections (CMEs) and flares associated with the solar energetic particle (SEP) events in the rising phases of solar cycles (SC) 23 (1996–1998) (22 events) and 24 (2009–2011) (20 events), which are associated with type II radio bursts.
The similarity between the rising phases of the 23-rd and 20-th solar cycles presents additional grounds for expectations of the lower maximum of the current solar cycle and the geomagnetic activity in the present solar cycle as compared with the 21-st and 22-nd solar cycles.
In addition, FS cells' EPSCs may have faster kinetics, as they exhibit sharper rising phases.
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During the whole measurement both feet were on a force plate (Zebris Medical, Germany) in order to determine the exact period between maximum vertical ground reaction force (start of the rising phase) and end of the rising phase.
b Spectrum on DOY 40 (rising phase of the eruption).
CAWSES-II focuses on the fundamental processes of the Sun-Earth system during the rising phase of solar cycle 24.
TESIS experiment will start at the rising phase of the 24th cycle of solar activity.
The resulting gating current exhibited a rising phase similar to that measured in voltage-dependent ion channels.
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