##plugins.themes.bootstrap3.article.main##

The planetary K-index (Kp index) was a geomagnetic index in the H-component field. This index was calculated from data collected by a network of 13 ground-based magnetometer stations at mid-latitude locations from the International Real-time Magnetic Observatory Network (INTERMAGNET). The magnitudes of Kp index could indicate geomagnetic activity using the integer K-scale from 0 to 9 without dimension because the K-scale was estimated using the quasi-logarithms algorithm. The Kp index indicated geomagnetic storms under the condition of K-scale>4. The three-hourly Kp index has been commonly used. The three-hourly Kp index was relatively stable for low‐variability geomagnetic activity. The hourly Kp index represented the level of auroral absorption with a more accurate characterization. For future research, the Kp index with a high sampling rate (e.g., <1 hour) could be considered, so that a very accurate characterization was characterized the more detailed geomagnetic activity of global region.

References

  1. J. W. Lin, “Real-time Magnetic Observatory Network: A Review,” European Journal of Environment and Earth Sciences, Vol. 2(5), pp. 1-2, 2021. doi: 10.24018/ejgeo.2021.2.5.177.
     Google Scholar
  2. J. Bartels, N. H. Heck, H. F. Johnston, “The three‐hour‐range index measuring geomagnetic activity,” Journal of Geophysical Research, Vol. 44 (4), pp. 411-454, 1939. doi: 10.1029/TE044i004p00411.
     Google Scholar
  3. J. Bartels, J. Veldkamp, “International data on magnetic disturbances, fourth quarter,” Journal of Geophysical Research, Vol. 59 (2), pp. 297-302, 1954. doi: 10.1029/JZ059i002p00297.
     Google Scholar
  4. K. Davies, “Ionospheric Radio,” The Institution of Engineering and Technology, IET Digital Library, 600 pp, 1990. ISBN: 9780863411861 doi: 10.1049/PBEW031E.
     Google Scholar
  5. B. G. Hansen, E. Willekens, “The generalized logarithmic series distribution,” Statistics & Probability Letters, Vol. 9 (4), pp. 311-316, 1990. doi: 10.1016/0167-7152(90)90138-W.
     Google Scholar
  6. M. Menvielle, N. Papitashvili, L. Häkkinen, C. Sucksdorff, “Computer production of K indices: review and comparison of methods,” Geophysical Journal International, Vol. 123 (3), pp. 866–886, 1995. doi: 10.1111/j.1365-246X.1995.tb06895.x.
     Google Scholar
  7. Y. J. Chen, K. Suzuki, H. Mahara, T. Yamaguchi, “Quasi-logarithmic spacing law in dewetting patterns from the drying meniscus of a polymer solution,” Chemical Physics Letters, Vol. 529, pp. 74-78, 2012. doi: 10.1016/j.cplett.2012.01.046.
     Google Scholar
  8. E. Geerardyn, Y. Rolain, J. Schoukens, “Design of Quasi-Logarithmic Multisine Excitations for Robust Broad Frequency Band Measurements,” IEEE Transactions on Instrumentation and Measurement, Vol. 62 (5), pp. 1364–1372, 2013. doi: 10.1109/TIM.2012.2232474.
     Google Scholar
  9. P. Wintoft, M. Wik, J. Matzka, Y. Shprits, “Forecasting Kp from solar wind data: input parameter study using 3-hour averages and 3-hour range values,” Journal of Space Weather and Space Climate, Vol. 7, A29, 2017. doi: 10.1051/swsc/2017027.
     Google Scholar
  10. X. Luan, W. Wang, J. Lei, A. Burns, X. Dou, J. Xu, “Geomagnetic and auroral activity driven by corotating interaction regions during the declining phase of Solar Cycle 23,” Journal of Geophysical Research: Space Physics, Vol.118 (3), pp. 1255-1269, 2013. doi: 10.1002/jgra.50195.
     Google Scholar
  11. R. A. D. Fiori, L. Trichtchenko, C. Balch, E. Spanswick, S. Groleau, “Characterizing Auroral‐Zone Absorption Based on Global Kp and Regional Geomagnetic Hourly Range Indices,” Space Weather, Vol. 18 (12), 2020. e2020SW002572, doi: 10.1029/2020SW002572.
     Google Scholar