Correction to: Wavelet Analysis of Forbush Decreases at High-Latitude Stations During Geomagnetic Disturbances.

The original article can be found online at DOI B Correction to: Solar Physics (2022) 297: 1-24 b https://doi.org/10.1007/s11207-022-01948-z The original publication has been corrected. HT <table frame="hsides" rules="groups"><thead><tr><th>Events</th><th>Date</th><th>Minm SYM-H Peak Time (UT)</th><th>Minm SYM-H Value</th><th>Type</th><th>Cause</th></tr></thead><tbody><tr><td>Event 1</td><td>25 Oct - 2 Nov 2003</td><td>2003/10/30 (22:55)</td><td>-432</td><td>Superintense</td><td>SH + MC (Zhang et al., 2007)</td></tr><tr><td>Event 2</td><td>23 Jul - 31 Jul 2004</td><td>2004/07/27 (13:35)</td><td>-208</td><td>Intense</td><td>SH + MC (Zhang et al., 2007)</td></tr><tr><td>Event 3</td><td>13 May - 21 May 2005</td><td>2005/05/15 (08:20)</td><td>-305</td><td>Superintense (HILDCAA)</td><td>Halo CME SH + MC (Zhang et al., 2007)</td></tr><tr><td>Event 4</td><td>13 Mar - 21 Mar 2015</td><td>2015/03/17 (22:47)</td><td>-234</td><td>Intense</td><td>SIRs with ICME (Chi et al., 2018)</td></tr><tr><td>Event 5</td><td>19 Jun - 27 Jun 2015</td><td>2015/06/23 (04:24)</td><td>-208</td><td>Intense</td><td>ICME (Patel et al., 2019)</td></tr></tbody></table> ht In subsection B 2.1.1 Wavelet Transform b , the tenth line has a typographical error, the correct version of this line is "This approach can work with the dynamic window; a window will be narrowed automatically to observe the high-frequency content and be widened to capture the low-frequency content in the signals (Strang and Nguyen, 1996; Foufoula-Georgiou and Kumar, 1995).". [Extracted from the article]