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Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during the current “exceptional” solar minimum: implications for climate change MIST/UKSP Session, RAS/NAM - EAS/JENAM, UoH, 22 April 2009

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Recent Data ► radial IMF, |B r | ► sunspot number, R ► Kp geomagnetic index ► PMOD composite of TSI Space Age Data

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Page 1: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Mike Lockwood(Southampton University

& Space Science and Technology Department, STFC/Rutherford Appleton Laboratory )

Open solar flux and irradiance during the current “exceptional” solar minimum:

implications for climate change

MIST/UKSP Session, RAS/NAM - EAS/JENAM, UoH, 22 April 2009

Page 2: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

RecentData

► radial IMF, |Br|

► sunspot number, R

► Kp geomagnetic index

► PMOD composite of TSI

Page 3: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

RecentData

► radial IMF, |Br|

► sunspot number, R

► Kp geomagnetic index

► PMOD composite of TSI

Space AgeData

Page 4: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

The “Ulysses Result”

ecliptic

Br(r1)

r1

r

|Br|

Balogh et al., 1995; Lockwood et al., 1999; 2004 Smith et al., 2001

Lockwood and Owens (2009) & Lockwood et al.

(2004) show that use of this equation is accurate to

within 2.5%

Thus total signed magnetic flux threading r1 = 1AU is

FS(r1) = (1/2)4r12 <|Br(r1)|>CR

Ulysses showed that|Br(r)| (r/r1)2 = |Br(r1)|

Page 5: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Open Solar Flux from IMF data (Lockwood, Rouillard and Finch 2009)

1970 1980 1990 2000 2010

7

6

5

4

3

2

1

Ope

n S

olar

Flu

x, F

S (

1014

Wb)

FS(r1)► using the

Ulysses result of the invariance of the radial IMF, Br & hourly mean data

► accurate to 2.5%

Page 6: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Open Solar Flux

ecliptic

Coronal Source Surface

quantified by PFSS from solar magnetograms

Br(r1)r1

r

|Br|

Balogh et al., 1995; Lockwood et al., 1999; Smith et al., 2001

total (“open”) magnetic flux leaving the sun, FS(ro) =

(1/2)x42 ro2<|Br(ro)|>CR

“excess”, FS(r) FS(ro) > 0

ro

Page 7: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Kinematic Excess Flux Correction (Owens et al. 2008, Lockwood et al. 2009)

► excess flux,

FS(r) =

2r2|Br(r)|

2r12|Br(r1)|

► ro = 2.5R

► PFSS values from photospheric magnetograms

FS(r1) = 0

FS(ro), from PFSS

Page 8: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Open Solar Flux from IMF data (Lockwood, Rouillard and Finch 2009)

1970 1980 1990 2000 2010

7

6

5

4

3

2

1

Ope

n S

olar

Flu

x, F

S (

1014

Wb)

► kinematic correction for effect of longitudinal solar wind structure, FS(ro)

► makes results consistent with PFSS

(Lockwood et al., 2009)

FS(ro) = FS(r1) FS(ro)

[ FS(ro) ]PFSS

FS(r1)

Page 9: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

► sunspot number, R

► open solar flux FS

► GCR counts C

► observations of TSI

► solar cycle length, L

running mean over T=[9:(1/4):13] yrs

running mean over T=L yrs

► global mean temperature

The current minimum follows from recent trends. (Lockwood and Fröhlich, 2007)

Page 10: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Millennial Variation composite 25-year means) from cosmogenic isotopes 14C & 10Be by Steinhilber et al. (2008)

Year AD

Solar Modulation Parameter, (MV)

-6000 -4000 -2000 0 2000

1000

800

600

400

200

0

composite from Solanki et al., 2004; Vonmoos et al., 2006 & Muscheler et al., 2007

we are still within recent grand maximum

Page 11: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

show the present minimum 23/24 is close to minima 19/20 and 16/17

earlier minima are lower

Cenntennial Variations- Geomagnetic Activity Indices

Page 12: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Geomagnetic activity annual means: correlations with solar wind & IMF

the corrected aa index is a range index & correlates best with BIMFVSW

2

the median index m is from hourly mean data & correlates best with BIMFVSW

0.3

aaC m

raa = 0.97Sr > 99.999% (AR-1 noise)

rm = 0.89 Sr = 99.995%(AR-1 noise)

Page 13: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Centennial Variationsgeomagnetic activity

the different dependences of aaC and m on VSW are significant at the 87% level.

0.87

Page 14: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Centennial Variations:reconstructed solar wind, IMF & open flux

use correlations to extrapolate VSW, BIMF & FS annual means back to 1905

Page 15: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Centennial Variations: the rise and fall of the current grand maximum

solar cycle running means

Abreu et al. (2008)

defining grand max. by > 600 MV it began in 1920 linear extrapolation gives end dates consistent with GSM durations

Page 16: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Has The Temperature Rise at Earth’s Surface Stalled in Recent Years?

Global Mean Air Surface Temperature (GMAST) composite from CRU, UEA

HadCRUR3v

Page 17: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

/2

time constant used to smooth data = 10 years

Has The Temperature Rise at Earth’s Surface Stalled in Recent Years?

3 example trends for the last /2 years:2 per 100yr0 per 100yr

+2 per 100yr

Page 18: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Variations about the trend

= 10 yr

for the last /2 years:

2 per 100yr

Page 19: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Variations about the trend

= 10 yr

for the last /2 years:

0 per 100yr

Page 20: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Variations about the trend

= 10 yr

for the last /2 years:

+2 per 100yr

Page 21: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Compare to the distribution of past variations about the trend

Distribution of deviations over /2 yrs

= 10 yrs

3 example trends for the last /2 years:2 per 100yr 0 per 100yr+2 per 100yr

= 10 yrs<x> = 0.001x = 0.034

Page 22: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Recent (last /2 yrs) fluctuations pdf:-

Page 23: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

Recent (last /2 yrs) fluctuations are consistent with past ones around a trend of +2c-1

For = 6 yr recent trend is most probably -2c-1 (but could be up to +4c-1)

For > 10 yr trend is most likely > 0

For > 18 trend +2c-1

Page 24: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during
Page 25: Mike Lockwood (Southampton University & Space Science and Technology Department, STFC/Rutherford Appleton Laboratory ) Open solar flux and irradiance during

► the present solar minimum is uniquely the present solar minimum is uniquely low - for the space agelow - for the space age► cosmogenic isotopes show that the cosmogenic isotopes show that the space age thus far has been a grand solar space age thus far has been a grand solar maximum (GSM)maximum (GSM)► geomagnetic activity data and the geomagnetic activity data and the statistics of GSM durations both indicate statistics of GSM durations both indicate that the present low minimum is consistent that the present low minimum is consistent with the end of the current GSMwith the end of the current GSM► the levelling off of global mean air surface the levelling off of global mean air surface temperatures is consistent with previous temperatures is consistent with previous fluctuations about the upward trend fluctuations about the upward trend