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Published byStanislaus Maus Modified over 6 years ago
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~130 Years of Solar Wind Data: The Floor and More
E.W. Cliver Space Vehicles Directorate Air Force Research Laboratory AGU 27-30 May 2008
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Outline Long-term solar wind reconstruction: Emerging consensus
Floor in the IMF: Then & Now Secular variation of solar wind speed Entering a Gleissberg Minimum?
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Long-term Solar Wind Magnetic Field Reconstruction:
2 2 2005 1 3 4 1 5 Br = 0.56Btot Long-term Solar Wind Magnetic Field Reconstruction: Emerging Consensus
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(Svalgaard & Cliver, JGR, 110(12), 2005)
The IDV index has the useful property of being highly correlated with B and independent of V
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Long-term Solar Wind Magnetic Field Reconstruction:
2 4 3 2 2005 1 3 5 4 2 1 5 Long-term Solar Wind Magnetic Field Reconstruction: Emerging Consensus (Exception: McCracken, 2007)
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- Annual averages of B show evidence for a floor ~ 4.5 nT
- The sharp drop from in the McCracken time series does not appear in geomagnetic data - The low value in 1901 from RL&F is in error (APR, priv. comm.)
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Floor in the Solar Wind Magnetic Field:
Direct Observations (27-Day Averages)
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Floor in the Solar Wind Magnetic Field: Recent Direct Observations
Last 13 rotations similar to 1901, 1902, 1913 Floor in the Solar Wind Magnetic Field: Recent Direct Observations
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Floor in the Solar Wind Magnetic Field: Cosmogenic Nuclei / long-term
(Muscheler et al., 2005) (Caballero-Lopez et al., 2004) Since SSN ~ 0 during MM, would expect B to be at floor level. Direct from C-L (parameterized). For M, modulation parameter vs. IDV-based B; IDV-based B vs. SSN Floor in the Solar Wind Magnetic Field: Cosmogenic Nuclei / long-term
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Interpretation of Floor: Baseline Open Magnetic Flux
SSW + HSS + CME º SSW + HSS * SSW B (nT) M ~250 μT M 245 μT M 200 μT M 115 μT (Fisk et al., 1999; Owens & Crooker, 2006) Year Interpretation of Floor: Baseline Open Magnetic Flux
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Svalgaard & Cliver, ApJ Lett. 661, L203, 2007 B(nT) = 0.27R½ + 4.6
For SSN = 0 Then: B Total (ecliptic) = 4.6 nT; B RADIAL (all latitudes) = 3.0 nT Now: B Total (ecliptic) ~ 4 nT; B RADIAL (all latitudes) ~ 2 nT
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~15% increase in solar wind speed during the last ~120 years
Floor (Rouillard et al., 2007; Svalgaard & Cliver, 2007) ~15% increase in solar wind speed during the last ~120 years
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Plea for Help to Magnetospheric Physicists
Open Question: Effect of ~10% decrease of Earth’s dipole since ~1850 on geomagnetic activity? - Siscoe et al. (2002) Decrease in activity (ISM model & Hill M/I coupling models) - Glassmeier et al. (2004) Weak/no effect (scaling relationships between magnetospheric parameters & M)
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A Coming Gleissberg Minimum? Cycle 24 may be smallest in ~100 years
Test of Long-term Reconstructions, Precursor Prediction Technique, Dynamo Models, … 164.5 158.5 120.8 75? (Svalgaard, Cliver, & Kamide, 2005)
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Conclusions Consensus long-term B & V / Validation of IDV
Floor in IMF in ecliptic Btot ~4 nT & Br ~ 2 nT (SSN = 0) ~15% increase in solar wind V since 1872?
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