2009
DOI: 10.1007/978-3-540-76939-2_5
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Effects of Geomagnetic Variations on System Earth

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Cited by 10 publications
(7 citation statements)
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“…Son et al (2008), for example, have shown that the southward shift of the westerlies observed during recent decades can likely be attributed to the anthropogenic destruction of stratospheric ozone and related changes in temperature gradients. Provided that the Laschamp event also caused an ozone hole (Valet and Valladas, 2010;Vogt et al, 2009), one might analogously expect a southward shift of the westerlies at ∼39 ka. This, taken at face value, is the opposite of what one would expect from the apparent correlation between strong cosmic ray fluxes and northward shifts of the westerlies/glacial advances ( Fig.…”
Section: Discussion Of the Forcings Of The Westerliesmentioning
confidence: 99%
“…Son et al (2008), for example, have shown that the southward shift of the westerlies observed during recent decades can likely be attributed to the anthropogenic destruction of stratospheric ozone and related changes in temperature gradients. Provided that the Laschamp event also caused an ozone hole (Valet and Valladas, 2010;Vogt et al, 2009), one might analogously expect a southward shift of the westerlies at ∼39 ka. This, taken at face value, is the opposite of what one would expect from the apparent correlation between strong cosmic ray fluxes and northward shifts of the westerlies/glacial advances ( Fig.…”
Section: Discussion Of the Forcings Of The Westerliesmentioning
confidence: 99%
“…Since most of the ozone layer is located in the mid-stratosphere nitric oxide is more effective for ozone loss than OH which is found in the upper and lowermost stratosphere. Presently the loss of stratospheric ozone induced by major solar events does not exceed a few percents, but the simulations show that in the magnetosphere of a strongly reduced dipole moment, solar protons of several tens of MeV access the atmosphere even at midlatitudes (Vogt et al, 2007(Vogt et al, , 2009. In the extreme case of a vanishing field leaving the atmosphere entirely exposed to energetic particles, the simulations (Sinnhuber et al, 2003) show that the total ozone loss would reach 40% in the northern atmosphere after a typical series of three solar events.…”
Section: What Did Happen During the Laschamp Event?mentioning
confidence: 98%
“…The penetration is much larger at one of the poles depending on the respective signs of the two components, but ozone loss can reach up to 20e40% at latitudes of 45e50 ( Fig. 5) and persists several years after the solar events (Vogt et al, 2007(Vogt et al, , 2009. Thus, both the reduced field strength and complex magnetosphere which prevailed during the Laschamp favoured a significant depletion of ozone during many episodes of intense solar activity.…”
Section: What Did Happen During the Laschamp Event?mentioning
confidence: 99%
“…The model furthermore allows to determine the loss of total ozone in the atmosphere and the surface UV-B radiation. For details reference is made to Sinnhuber et al (2003), Winkler et al (2008), and Vogt et al (2009).…”
Section: Polarity Transitions and Uv-b Radiation Enhancementsmentioning
confidence: 99%