Substorm energy budget during low and high solar activity: 1997 and 1999 compared
By E. Tanskanen, Tuija I. Pulkkinen, H. Koskinen, J. Slavin. 2002
149 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/75970128a86e5a4a8b767e81d7f094562678abd2
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Citations in the corpus
- Substorm onset observations by IMAGE-FUV (2004, background): “The development of large systems of groundbased magnetometers or riometers, like MIRACLE or CANOPUS [Amm et al., 2001; Tanskanen et al., 2002; Samson et al., 1992; Voronkov et al., 1999; Syrjäsuo, 1998], allowed for more systematic studies of the magnetic pulsations and absorption features that…”
- A comprehensive high‐throughput analysis of substorms observed by IMAGE magnetometer network: Years 1993–2003 examined (2009, methodology): “[30] As a check of the algorithmical search concept, the substorms found using the method described in chapter 2.2 were compared to substorms obtained for years 1997 and 1999 using the same IL index [Tanskanen et al., 2002].”