Other
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh24a..01c&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH24A-01
Other
2104 Cosmic Rays, 2134 Interplanetary Magnetic Fields, 7524 Magnetic Fields, 7537 Solar And Stellar Variability (1650), 7974 Solar Effects
Scientific paper
McCracken (2007) inverted the galactic cosmic ray record for the interval 1428-2005 to estimate annual averages of the heliomagnetic field (HMF) near Earth during this interval. Quoting from his abstract, "There is good agreement with the results obtained by others using two independent methodologies based upon the sunspot [Solanki et al., 2002] and geomagnetic [Lockwood et al., 1999] records There is disagreement with another method based on the geomagnetic record [Svalgaard and Cliver, 2005] that needs to be resolved." We address the reported disagreement of our long-term reconstruction of the HMF strength with that obtained in the other three studies. We show that a recent reconstruction of the HMF by Rouillard, Lockwood, and Finch [2007] agrees much more closely with that of Svalgaard and Cliver than that of Lockwood et al. to the point where a consensus seems to be reached. We suggest that the discrepancy between McCracken's cosmic-ray-based HMF reconstruction and those based on geomagnetic data originates in the Forbush and Neher ionization chamber data (1933-1957) used to bridge the time gap between the 10Be time series (1428-1930) and the Climax neutron monitor record (1951-present).
Cliver Edward W.
Svalgaard Leif
No associations
LandOfFree
Towards a Consensus View of the Heliospheric Magnetic Field Strength Since 1900 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Towards a Consensus View of the Heliospheric Magnetic Field Strength Since 1900, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Towards a Consensus View of the Heliospheric Magnetic Field Strength Since 1900 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1247379