29 april 2011viereck: space weather workshop 2011 the recent solar minimum: how low was it? what...
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29 April 2011 Viereck: Space Weather Workshop 2011
The Recent Solar Minimum:How Low Was It?
What Were The Consequences?
Rodney ViereckNOAA Space Weather Prediction Center
With Contributions fromEduardo Araujo-Pradere, CU
Stan Solomon, NCAR
John Emmert, NRL
Judith Lean, NRL
Nicolas Bergeot, Royal Observatory, Belgium
Space Weather Workshop29 April 2011
Outline
Part 1: The recent solar minimum…. How low did it go? How does it compare? Are we headed for another Maunder Minimum?– Smoothed Sunspot Number– Geomagnetic Indices– F10.7– Space Weather: Will we have any this coming solar cycle?
Part 2: What were some of the consequences of this recent minimum?– Impact on neutral density and satellite drag– Impact on TEC and the ionosphere– Impact on climate
2
Smoothed Sunspot Number
3
Dalton Minimum
PredictedMax
Recent Min
DaltonMinimum
Modern Maximum• 13 Month Running
Average
• Note the two previous periods of low solar cycles…
– 1825– 1900
• Predicted Maximum for next cycle = 90
Smoothed SSN
• Solar minima have significant variability.
• Recent minimum was lowest since 1913.
• Two minima in the early 1800s were lower than the current minimum.
4
Current Min. Compared to the Previous Six
5
Current Min. Compared to the Lowest Three
6
All of the Last 21 Solar Cycles
7
Longer SSN Record
8
Longer SSN Record
9
• Current minimum not as low as Dalton minimum
• Maunder and Spörer minima are lower than Dalton minimum
• Modern Maximum is larger than any maximum in 1200 years
Aa Geomagnetic Record
10
• Derived from only two ground magnetometer stations
• England• Australia
• Longer record than Ap or Kp
• Not a strong solar cycle signal– CME driven
geomagnetic storms during solar max
– Coronal hole geomagnetic storms during solar min
Smoothed Aa Index
11
• Recent minimum shows a significant departure from the trends of the last 80 years.
• Recent minimum is the lowest since 1913
• There have been lower minima
14 Jan 2011 Viereck SWW 2011
F10.7
• F10.7 is a solar radio emission used as a proxy for solar EUV irradiance
• Shows strong solar cycle signal
• Reaches similar minimum values during each solar min.
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Details of F10.7
13
• Lower daily values were observed in the late 1950s
• The 13 month running average values have never been observed as low as the recent cycle
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Why Was This Recent Solar Minimum so Low?
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• In F10, previous solar minimum (1996) had similar low values but also had 27-day variations
• Recent solar minimum had nearly two years with little or no 27-day modulation making the the 13 month running average values significantly lower.
• In Aa the opposite was true… less 27 day modulation but lower values
Geomagnetic Activity
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• Really big storms can occur during any size solar cycle.
• Even big storms don’t show strong correlation with sunspot number
• Two of the biggest on record occurred during moderate sized solar cycles
• The next solar cycle is expected to be of moderate size.
Other Space Weather:Proton/Particle Events
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D. F. Smart, M. A. Shea, G. A. M. Dreschhoff, H. E. Spence, and L. Kepkoc, 2009McCracken et al., 2001
Ice core data shows a strong spike (red bar) in the atmospheric nitrate (NOx) abundances during the 1859 storm, along with lesser spikes for many other storms since 1500
Part 1: Summary
• Recent solar minimum was the lowest in nearly 100 years– Lowest smoothed sunspot min since 1913– Lowest smoothed geomag min since 1913– Lowest smoothed F10.7 on record (since 1947)
• There have been lower and longer minima as recorded in the sunspot record.– Dalton minimum (two minima) in the 1800s was lower– Maunder minimum was probably much lower
• Even if this Cycle is Small, Space Weather Will Continue– Geomagnetic Storms will still occur
• Maybe less frequent but likely as large– Particle Events will still occur
• Seem to be less correlated with SSN
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Part 2: Response of the Terrestrial System
• Density has been getting lower each solar min
• The change from each successive min to min…– 10% Drop– 12% Drop– 38% Drop
• Recent minimum is much lower.
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400 km Neutral Density Derived from Satellite Drag(thanks to John Emmert, NRL)
Thermospheric DriversSolar EUV (F10), Geomagnetic Storms (Ap), Climate Change(CO2)
19
1970 1975 1980 1985 1990 1995 2000 2005 2010-100
-80
-60
-40
-20
0
20
40
60
80
100
120
140
160
180
200
220
F
10
Year
F10
-20
-10
0
10
20
30
40
50
60
Ap
Ap
300320340360380400420440460480500520540560580600620640660680700
CO2
CO
2 (pp
mv)
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Subtracting the Anthropogenic Correction
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Note the excellent fit during the first three minima
Note the improved fit during the last minimum
7.1E-14
5.2E-144.6E-14
MSIS Results Using the Three Solar Inputs(Details)
Mg II Index provides the best fit to the observed density
1970 1975 1980 1985 1990 1995 2000 2005 2010
4E-15
6E-15
8E-15
1E-14
1.2E-14
1.4E-14
1.6E-14
1.8E-14
2E-14
N
eu
tra
l De
nsi
ty
Year
Drag MSIS With Mg II - CO2 MSIS With SEM - CO2 MSIS With F10 - CO2
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Relative Magnitude of the Density ChangesModeled density changes for each input while holding the other two constant
22
1970 1975 1980 1985 1990 1995 2000 2005 2010
1E-14
De
nsi
ty (
gm
/cm
3)
Year
CO2 Solar Geomag
Relative Contributions of the change from(1996 to 2009)Solar 1.49E-15 = 48%Geomag 1.03E-15 = 33%Anthro 0.61E-15 = 19%
14 Jan 2011 Viereck: SWPC Seminar
Response of the Ionosphere
• Total Electron Content shows significant changes from last minimum to the most recent minimum…– At some local times
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Avg. of 250 Locations
One Location
Extracted from CODE Global Ionospheric maps (GIMs IONEX format)
Response of the Ionosphere
• Total Electron Content shows changes from last minimum to the most recent minimum…– But only during some seasons– And only at some latitudes
• Sometimes the response is the opposite of what is expected.
Courtesy of Nicolas BergeotRoyal Observatory of Belgium
Response of the Climate
• Globally-averaged surface temperature– 130 Year record showing
general warming of ~1oC• Four primary contributors to
global climate change– Solar– Anthropogenic – Volcanoes– El Nino/La Nina
• Simple empirical model can reproduce much of the observed climate change.
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Lean; NRLLean, NRL
Climate During the Recent Solar Minimum
• Up to 1998 Global climate was on a steady rise.
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Lean, NRL
Climate During the Recent Solar Minimum
• After 1998 global climate did not rise– Anthropogenic forcing
continued to rise during this period
– Global temperatures did not follow predictions made in 2000.
• Recent climate trends are driven by three of the four – Anthropogenic forcing has
warmed the climate– Solar and ENSO have been
cooling the climate– The result was a flat global
temperature for the last 6-8 years.
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Lean, NRL
Summary• Recent solar minimum was the lowest in nearly 100 years
– Lowest smoothed sunspot min since 1913– Lowest smoothed geomag min since 1913– Lowest smoothed F10.7 on record (since 1947)
• There have been lower and longer minima as recorded in the sunspot record.– Dalton minimum (two minima) in the 1800s was lower– Maunder minimum was probably much lower
• Even if this Cycle is Small, Space Weather Will Continue– Geomagnetic Storms will still occur
• Maybe less frequent but likely as large
– Particle Events will still occur• Seem to be less correlated with SSN
• The response of the thermosphere was significant– 38% reduction in the neutral density at 400 km
• The response of the ionosphere was more subtle– Generally lower TEC but not uniform across space and time
• The response of the climate was measureable– Contributed to the lower than expected temperatures from 2005-2011
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