2009
DOI: 10.5194/angeo-27-2045-2009
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On the long term change in the geomagnetic activity during the 20th century

Abstract: Abstract. The analysis of the aa index series presented in this paper clearly shows that during the last century (1900 to 2000) the number of quiet days (Aa<20 nT) drastically diminished from a mean annual value greater than 270 days per year at the end of the nineteenth century to a mean value of 160 quiet days per year one hundred years later. This decrease is mainly due to the decrease of the number of very quiet days (Aa<13 nT). We show that the so-evidenced decrease in the number of quiet days cannot be a… Show more

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Cited by 23 publications
(19 citation statements)
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“…Placing now our study in the context of solar cycle phases (Minimum, Increasing, Maximum, and Decreasing) and geomagnetic classification proposed by Zerbo et al [7], we made interesting analysis: 1) During Minimum phase where Quiet activity (QA) is predominant [6][7][8], precipitations increase (Figure 1) and temperatures decreases (Figure 2). This phase is characterized by slow solar wind speed and high density of solar plasma 2) During Maximum phase where Shock Activity (SA) is predominant [6][7][8], precipitations increase (Figure 1) and temperatures fluctuates (Figure 2). Here Coronal mass ejections (CMEs) are the most important solar events with important energy dissipated in interplanetary medium modifying atmospheric circulation and chemistry (overpressure or depression).…”
Section: Data Sources and Data Analysismentioning
confidence: 99%
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“…Placing now our study in the context of solar cycle phases (Minimum, Increasing, Maximum, and Decreasing) and geomagnetic classification proposed by Zerbo et al [7], we made interesting analysis: 1) During Minimum phase where Quiet activity (QA) is predominant [6][7][8], precipitations increase (Figure 1) and temperatures decreases (Figure 2). This phase is characterized by slow solar wind speed and high density of solar plasma 2) During Maximum phase where Shock Activity (SA) is predominant [6][7][8], precipitations increase (Figure 1) and temperatures fluctuates (Figure 2). Here Coronal mass ejections (CMEs) are the most important solar events with important energy dissipated in interplanetary medium modifying atmospheric circulation and chemistry (overpressure or depression).…”
Section: Data Sources and Data Analysismentioning
confidence: 99%
“…These periods are characterized by high stream solar wind speed flowing from coronal holes [6][7][8] most disturbed magnetic field with important solar dynamo and joule effect. All that implies that there is no zero climate response to the non constant energy receive from sun (G. Tsiropoula [13]).…”
Section: Data Sources and Data Analysismentioning
confidence: 99%
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“…Not much solar information is available for the first episode, but more exists for the second. In this context it is worth commenting that some studies indicate a pronounced change in solar rotation around 1900 (Balthasar, Vázquez, and Wöhl, 1986) that surely also affected the heliosphere (Echer et al, 2004;Ouattara et al, 2009) and therefore the number of auroral events (see Silverman and Blanchard, 1983). Echer et al (2004) suggests that OMF structures have increased their activity relative to CMF structures during the last 130 years.…”
Section: Discussionmentioning
confidence: 95%
“…Geomagnetic activity indices bear more than 140 years of information on the evolution during the solar wind's (see, e.g., Rouillard et al, 2007) coupling with the magnetosphere and on the state of the ionized environment of the Earth (see, e.g., Ouattara et al, 2009). Geomagnetic indices have many other applications.…”
Section: Geomagnetic Indicesmentioning
confidence: 99%