Solar variability as an input to the Earth's environment

By Andrew Wilson. 2003

285 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/3baf9cc3b62d5323701abf1cd295b14749d7bfd9

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. M. Temmer
2. Nat Gopalswamy
3. R. Schwenn
4. B. Vršnak
5. N. Lugaz
6. W. Manchester IV
7. S. Solanki
8. S. Yashiro

Citations in the corpus

• Fitting Flux Ropes to a Global MHD Solution: A Comparison of Techniques. Appendix 1 (2004, background): “Beginning with linear force-free models (Goldstein, 1983; Lepping et al., 1990), they have evolved to include the effects of expansion (Osherovich et al., 1993; Marubashi, 1997), data from multiple spacecraft (Mulligan et al., 2001), non-force-free effects (Mulligan et al., 2001; Hidalgo et al.,…”
• Coronal Mass Ejections and Solar Polarity Reversal (2003, background): “On the basis of the magnetic field data, the north polar reversal was reported to be in 2001 February (Bilenko 2002) and 2001 May (Durrant & Wilson 2003).”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…CMEs (Gopalswamy et al., 2000; Vršnak, 2001; Cargill, 2004; Liu et al., 2013), changes in the radial expansion rate of the magnetic ejecta (Gulisano et al., 2010; Poomvises, Zhang, and Olmedo, 2010) and, sometimes, its deflection (Wang et al., 2014) and rotation (Nieves-Chinchilla et al., 2012).”
• Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23 (2005, methodology): “Bothmer (2003) investigated in detail the solar sources of five MCs that are included in Table 2 (10–11 January 1997; 22 September 1997; 16–17 April 1999; 21–22 February 2000; 15–16 July 2000).”
• AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT? (2008, methodology): “In this paper we compare our statistics and measurements of CME parameters against the CDAW LASCO CME catalog (Gopalswamy et al. 2003; Yashiro et al. 2004) as reference catalog.”
• Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption (2004, methodology): “In such cases, the Thompson scattering measurements by the Solar Mass Ejection Imager (SMEI) combined with IPS observations (Jackson et al. 2003; Eyles et al. 2003) could be essential for the understanding of the IP propagation of CMEs and a successful prediction of 1 au transit time.”
• Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, background): “…and NIR bands barely exceeds 0.5 % over a solar cycle; in the near UV and shorter wavelengths variability increases with decreasing wavelength, reaching90 several percent at 200–250nm, and several tens of percent, and even more, below about 200nm (e.g. Floyd et al., 2003, and references therein).”