Space Weather: What IS the Sun Doing? Joe Kunches NOAA Space Weather Prediction Center (nee Space Environment Center) Boulder, CO ILA-36 Orlando October.

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Presentation transcript:

Space Weather: What IS the Sun Doing? Joe Kunches NOAA Space Weather Prediction Center (nee Space Environment Center) Boulder, CO ILA-36 Orlando October 17, 2007

Outline Solar Cycle 24 Prediction Solar Cycle 24 Prediction Extraordinary December 2006 Solar Radio Burst Extraordinary December 2006 Solar Radio Burst Future needs Future needs

The solar x-ray images are from the Yohkoh mission of ISAS, Japan. The x-ray telescope was prepared by the Lockheed Palo Alto Research Laboratory, the National Astronomical Observatory of Japan, and the University of Tokyo with the support of NASA and ISAS. G.L. Slater and G.A. Linford

Solar Cycle 24 Why is it important? Why is it important? Ionosphere “Bulks Up,” due to a factor of 4 increase in solar EUV (more affecting GPS) Ionosphere “Bulks Up,” due to a factor of 4 increase in solar EUV (more affecting GPS) Scintillation activity maximizes Scintillation activity maximizes Large events cluster near the peak Large events cluster near the peak Sunspot number prediction gives an “envelope” of activity, similar to forecasts of the hurricane season Sunspot number prediction gives an “envelope” of activity, similar to forecasts of the hurricane season

Why is solar cycle prediction important?

What is an Average Solar Cycle? Duration is 11.0±1.5 yrs [8.2, 15] Peak is 113.7±39.5 [48.7, 164.5] Rise to Max is 4.7±1.4 yrs [2.8, 7.5] Fall to Min is 6.3±1.3 yrs [3.5, 10.2]

What we’re dealing with Aware of 29 predictions of Cycle 24 peak –Well, 3 are ‘typical’ climatology from Pesnell Thanks for the table Dean The spread is from 42 to 185 – SSN AVG =117±38 Categories –Climatology -12 –Spectral – 8 –Precursor – 6 –physics-Based* – 2 –Neural Network – 1 * is this a good name for these?

How Does A Solar Cycle Happen? Need to create magnetic flux Need to create magnetic flux Does the flux come from the last cycle? Does the flux come from the last cycle? And how do you And how do you know it when you know it when you see it? see it?

On the One Hand… The flux is what’s left over from the previous cycle The flux is what’s left over from the previous cycle You see the remains when you measure the polar fields of the Sun You see the remains when you measure the polar fields of the Sun Lately the measurements of those fields are extremely low Lately the measurements of those fields are extremely low ERGO, a really small cycle is coming! ERGO, a really small cycle is coming!

Goddard Space Flight Center Space Weather Workshop, April 2007, W. Dean Pesnell, GSFC 10

But On the Other Hand…. A new physics model has replicated magnetic flux emergence over the past 80 years A new physics model has replicated magnetic flux emergence over the past 80 years It shows the meridional flow – “conveyor belt” – is the prime mover It shows the meridional flow – “conveyor belt” – is the prime mover It asserts the past 2 cycles are on the conveyor belt It asserts the past 2 cycles are on the conveyor belt ERGO, the next cycle will be very large! ERGO, the next cycle will be very large!

What We Know D. Hathaway, NASA

Analogy with ocean conveyor belt Broecker 1991

Calibrated Flux-transport Dynamo Model Near-surface diffusivity same as used by Wang, Shelley & Lean, 2002; Schrijver 2002 in their surface flux-transport models. N-Pole S-Pole Red: α -effect location Green: rotation contours Blue: meridional flow Magnetic diffusivity used Flows derived from observations

Contours: toroidal fields at CZ base Gray-shades: surface radial fields Observed NSO map of longitude-averaged photospheric fields Validity test of calibration (Dikpati, de Toma, Gilman, Arge & White, 2004, ApJ, 601, 1136)

Simulating relative peaks of cycles 12 through 24 (model fed by surface poloidal source continuously) Observed cycles  We reproduce the sequence of peaks of cycles 16 through 23  We predict cycle 24 will be 30-50% bigger than cycle 23  We obtain similar results for diffusivities between and (Dikpati, de Toma & Gilman, 2006, GRL, in press)

117.0±37.9 CYCLE 24 SSN PREDICTIONS

Cycle 24 ( ) Prediction

So.... A large cycle means: A large cycle means: More big storms More big storms More EUV and a “thicker” Ionosphere More EUV and a “thicker” Ionosphere A smaller cycle means: A smaller cycle means: The Ionosphere will be less of a contributor to the GPS/GNSS Error Budget The Ionosphere will be less of a contributor to the GPS/GNSS Error Budget There will be relatively few large storms There will be relatively few large storms

Outline Solar Cycle 24 Prediction Solar Cycle 24 Prediction Extraordinary Solar Radio Burst Extraordinary Solar Radio Burst Future needs Future needs

Record Radio Burst During Solar Minimum repeat of previous cycle Photo by Gary Palmer Radio noise level on GPS frequency Owens Valley Solar Array

Solar Radio Burst Of December 6, 2006: Observed by the Global GPS Network Galapagos: Sunlit during SRBGUAM: Nighttime during SRB GUAM GLPS Ultra-precise positioning (10-20 cm) Global coverage: Land, Air, Space Used by satellites in orbit Global GPS Network Applications Positioning FailsPositioning fails

Outline Solar Cycle 24 Prediction Solar Cycle 24 Prediction Extraordinary Solar Radio Burst Extraordinary Solar Radio Burst Future needs Future needs

Future Needs FCC to Require Full E911 Adherence by 2012 (Sept. 12, 2007) – eLoran here? FCC to Require Full E911 Adherence by 2012 (Sept. 12, 2007) – eLoran here? ADS-B ADS-B

Summary Solar Cycle 24 starting soon – predictions diverge! Solar Cycle 24 starting soon – predictions diverge! Solar Radio Burst of December 2006 severely affected GPS users (a new nemesis) Solar Radio Burst of December 2006 severely affected GPS users (a new nemesis) New demands from users raise the bar New demands from users raise the bar