000003017 001__ 3017
000003017 005__ 20170106120421.0
000003017 0247_ $$2DOI$$a10.1007/s11207-016-0892-3
000003017 037__ $$aSCART-2017-0013
000003017 100__ $$aLefèvre, Laure
000003017 245__ $$aDetailed Analysis of Solar Data Related to Historical Extreme Geomagnetic Storms: 1868 - 2010
000003017 260__ $$c2016
000003017 520__ $$aAn analysis of historical Sun-Earth connection events in the context of the most extreme space weather events of the last ˜150 years is presented. To identify the key factors leading to these extreme events, a sample of the most important geomagnetic storms was selected based mainly on the well-known aa index and on geomagnetic parameters described in the accompanying paper (Vennerstrøm et al., Solar Phys. in this issue, 2016, hereafter Paper I). This part of the analysis focuses on associating and characterizing the active regions (sunspot groups) that are most likely linked to these major geomagnetic storms.
000003017 594__ $$aSTCE
000003017 6531_ $$aHistorical data
000003017 6531_ $$aExtreme events
000003017 6531_ $$aSolar storms
000003017 6531_ $$aGeomagnetic storms
000003017 6531_ $$aFlares, Active regions
000003017 6531_ $$aSunspots
000003017 6531_ $$aStatistics
000003017 700__ $$aVennerstrøm, Susanne
000003017 700__ $$aDumbović, Mateja
000003017 700__ $$aVršnak, Bojan
000003017 700__ $$aSudar, Davor
000003017 700__ $$aArlt, Rainer
000003017 700__ $$aClette, Frédéric
000003017 700__ $$aCrosby, Norma
000003017 773__ $$c1483-1531$$n5$$pSolar Physics$$v291$$y2016
000003017 8560_ $$flaure.lefevre@observatoire.be
000003017 905__ $$apublished in
000003017 980__ $$aREFERD