2012
DOI: 10.5194/angeo-30-421-2012
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Solar wind and geomagnetism: toward a standard classification of geomagnetic activity from 1868 to 2009

Abstract: Abstract. We examined solar activity with a large series of geomagnetic data from 1868 to 2009. We have revisited the geomagnetic activity classification scheme of Legrand and Simon (1989) and improve their scheme by lowering the minimum Aa index value for shock and recurrent activity from 40 to 20 nT. This improved scheme allows us to clearly classify about 80 % of the geomagnetic activity in this time period instead of only 60 % for the previous Legrand and Simon classification.

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Cited by 35 publications
(67 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: 93%
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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: 93%
“…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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“…Indonesia (10) MAGDAS (8), SID (2) 48. Ireland (14) AWESOME (1), CALLISTO(4), SID (9) 49. Israel (4) AWESOME (1), ULF_ELF_VLF(3) 50.…”
Section: Listingmentioning
confidence: 99%
“…Since it is well known that the CMEs occur in majority on the maximum phase of the solar cycle and the high stream solar wind following from coronal holes occur during the declining of solar cycle, we choose in this paper to investigate the natural links between solar wind parameters (B, V) and the Polar Cap Index (PCI) introduced by Troshichev et al, 1988, and used in a statistical sense as a measure of electric field. Our interest is to learn more about the link between the solar dynamo and the energy dissipated in interplanetary medium in the context of geomagnetic activity (Legrand and Simon, 1989;Zerbo et al, 2012).…”
Section: Introductionmentioning
confidence: 99%