The 1859 Solar–Terrestrial Disturbance And the Current Limits of Extreme Space Weather Activity

By E. Cliver, L. Svalgaard. 2004

217 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e4d1a86c648dfb4d68966a9173bb406119a791a3

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In Astronomy and Astrophysics

1. M. Temmer
2. Nat Gopalswamy
3. N. Lugaz
4. S. Yashiro
5. R. Howard
6. A. Vourlidas
7. G. Aulanier
8. R. Schwenn

In Molecular Biology

1. Nat Gopalswamy
2. M. Temmer
3. N. Lugaz
4. Etienne Pariat
5. R. Howard
6. J. Davies
7. A. Vourlidas
8. P. Démoulin

Citations in the corpus

• Coronal mass ejections and other extreme characteristics of the 2003 October–November solar eruptions (2005, methodology): “ Cliver and Svalgaard [2004] considered fast transit events (Sun-Earth travel time � 21.8 hours) for the period 1859–2003.”
• Space Weather: The Solar Perspective (2006, background): “It turned out that the September 1, 1859 event was among the fastest and most energetic flares ever since (Cliver and Svalgaard, 2004).”
• On the probability of occurrence of extreme space weather events (2012, background): “In soft X-rays, the flare has been estimated to be >X10 [Cliver and Svalgaard, 2004].”
• Geomagnetic storms: historical perspective to modern view (2016, background): “2003; Cliver and Svalgaard 2004; Vasyliunas 2011; Lakhina et al.”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “It has been suggested that it was the case for the Carrington event of 1859 (Cliver and Svalgaard, 2004), the Halloween events of 2003 (Tóth et al., 2007), and the 23 July 2012 event (Liu et al., 2014a), each of which is a case where the propagation lasted less than 20 hours, i.e. the average…”
• Sq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo Currents (2017, unknown): “Good agreement between the Sq amplitude and solar activity parameters presented in Table 4 suggests that those solar indices can be estimated or calibrated using Sq data (Svalgaard and Cliver 2007, Svalgaard 2016). However, such an application requires some caution; for example, as seen in Table 4, ”
• The standard flare model in three dimensions II: upper limit on solar flare energy (2012, background): “For example, the energy content of the first-ever observed solar flare on Sept 1, 1859 (Carrington 1859; Hodgson 1859) has been thoroughly debated (McCracken et al. 2001; Tsurutani et al. 2003; Cliver & Svalgaard 2004; Wolff et al. ar X iv :1 21 2.”
• Historical sunspot observations: A review (2007, background): “There are some recent reviews of this Carrington (1860a) and Hodgson (1860) flare observed on 1 September 1859 (Cliver and Svalgaard, 2004; Cliver, 2006; Tsurutani et al., 2003).”
• ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, background): “…was produced by a relatively slow CME from 1989 March 10 (with a Sun-to-Earth transit time of 54.8 hr), while the 1972 August 4 CME, which has the fastest transit on record (14.6 hr), generated a geomagnetic storm with the minimum Dst of only −125 nT (Cliver et al. 1990; Cliver & Svalgaard 2004).”
• Quantifying extreme behavior in geomagnetic activity (2011, background): “However, we know that larger storms have occurred in the past, most notably the Carrington event of September 1859 [e.g., Cliver and Svalgaard, 2004] and for which only limited information, in the form of analog paper records, is available.”