Update, or Lack Thereof, to the Solar Cycle 24 Prediction Doug Biesecker NOAA/SWPC.

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Presentation transcript:

Update, or Lack Thereof, to the Solar Cycle 24 Prediction Doug Biesecker NOAA/SWPC

Outline Status of the current prediction, made in 2009 Is the prediction still valid? What arguments drove the current prediction? Why has the forecast not been adjusted? – Because it’s right…enough Comparison between Cycle 24 (so far) and previous solar cycles Sunspots Flares

The Panel PanelistAffiliationPanelistAffiliationPanelistAffiliation D. BieseckerNOAA, ChairM. DikpatiNCARK. DowdyUSAF D. HathawayNASAT. HoeksemaStanford U.E. KihnNOAA H. Lundstedt Swedish Inst. of Space Sci. D. PesnellNASAM. RastU. Colorado L. SvalgaardETK Inc.R. ThompsonIPS Australia R. Van der Linden Royal Obs. Of Belgium J. Kunches NOAA, ex-officio O.C. St. Cyr NASA, ex-officio

Remember all that craziness from 2008? What were they thinking?

What the ‘Official’ Panel ‘Officially’ Predicted Updated prediction released in May, 2009 – Solar Minimum would occur in December, 2008 Remember, we only had smoothed data through October, 2008 – Solar Maximum will occur in May, 2013 – Solar Maximum will reach a peak SSN of 90 Average maximum is 114

What that prediction looks like

Geomagnetic Precursors  Utilize information from the declining phase of a cycle or from solar minimum to predict the intensity of the subsequent maximum  Based in dynamo theory, whereby poloidal field of cycle N is converted into toroidal field of cycle N+1  Historically, these techniques have provided the best skill at predicting the solar cycle. Ohl and Ohl 1979 Courtesy D. Hathaway

Richard Thompson (IPS) Geomagnetic Precursor based on Ap Year Peak Smoothed SSN Minimum 12-month average Ap red (monthly) green (6 monthly) blue (12 monthly) Average Ap

 A model calling for a small cycle – short recycle time  Skip the ‘proxy’ (geomagnetic disturbances) Polar Field Precursor Methods Schatten and Pesnell (1993) WSO

How is the Prediction Shaping Up? The cycle may be lagging slightly behind the prediction – Overall, it’s not far off

What is everyone else saying? Well, some of them anyway… IPS – 90 in April 2013 SODA – 82 in early 2014 NGDC (McNish-Lincoln) – 76 in June/July 2013 Hathaway – Geomag Precursor – 59 in June/July 2013

What is everyone else saying? Well, some of them anyway… IPS – 90 in April 2013 SODA – 82 in early 2014 NGDC (McNish-Lincoln) – 76 in June/July 2013 Hathaway – Geomag Precursor – 59 in June/July 2013

Why is there a lack of an update? Everybody seems to now agree the cycle will be small – Whether it ends up being 90 or 80, shouldn’t really matter. – We won’t chase a number, unless it’s clear we are ‘wildly’ wrong Should consider in the future choosing one of – Small, Average, Large

Cycle sizes Small <=90 Medium >90 - <140 Large >=140 Something for the next panel to consider SmallAverageLarge Smoothed SSN Sorted by size

How does Cycle 24 Compare? Clearly cycle 24 started from a lower SSN and is rising slower than recent cycles This is exactly what we expect for a prediction of a small cycle

A Functional Form for the Cycle Fitting the cycle to a functional form with amplitude a, starting time t 0, width b, and asymmetry c, provides a prediction for the current cycle and can account for systematic changes in cycle shape.

Solar Activity at the Start of the Cycle (Months 1-27) CYCLE27 month total SSN GOES M flares M Flares / SSN GOES X flares X Flares / SSN WHERE ARE ALL THE X-FLARES? Otherwise, this cycle looks normal compared to recent, larger cycles

Summary The Solar Cycle Prediction remains on track – Peak of 90 in May, 2013 – Or close enough to not go chasing a number Seems that everyone now agrees the cycle will be smaller than average The official prediction should be seen as guidance – Below average, average, above average The solar flare rate is consistent with recent solar cycles

One final movie

Accurate Predictions by 30 Months Asymmetry is constant (c=0.71) and width varies with amplitude. The remaining two parameters, amplitude and starting time, can be accurately determined by about 30 months from the start of the cycle.