Scientific Research and Essays

  • Abbreviation: Sci. Res. Essays
  • Language: English
  • ISSN: 1992-2248
  • DOI: 10.5897/SRE
  • Start Year: 2006
  • Published Articles: 2768

Full Length Research Paper

Geoeffectiveness of the inner magnetosphere under the impact of fast solar wind currents: Case of solar cycles 20 to 23

Gnanou Inza
  • Gnanou Inza
  • Laboratoire de Recherche en Energétique et Météorologie de l’Espace (LAREME), Université Norbert Zongo, Koudougou, Burkina Faso.
  • Google Scholar
Zoundi Christian
  • Zoundi Christian
  • Laboratoire de Recherche en Energétique et Météorologie de l’Espace (LAREME), Université Norbert Zongo, Koudougou, Burkina Faso.
  • Google Scholar
Sawadogo W. Emmanuel
  • Sawadogo W. Emmanuel
  • Laboratoire de Recherche en Energétique et Météorologie de l’Espace (LAREME), Université Norbert Zongo, Koudougou, Burkina Faso.
  • Google Scholar
Ouattara Frédéric
  • Ouattara Frédéric
  • Laboratoire de Recherche en Energétique et Météorologie de l’Espace (LAREME), Université Norbert Zongo, Koudougou, Burkina Faso.
  • Google Scholar


  •  Received: 17 January 2022
  •  Accepted: 22 February 2022
  •  Published: 31 March 2022

References

Abdullrahman HM, Marwa AM (2020). The Effects of Solar Activity and Geomagnetic Disturbance on Human Health. Open Access Journal of Biomedical Science 2(5).
Crossref

 

Bame SJ, Asbridge JR, Feldman WC, Gosling JT (1976). Solar cycle evolution of high-speed solar wind streams, Astrophysical Journal 207(3):977-980
Crossref

 

Baumjohann W, Haerendel G, Melzner F (1985). Magnetospheric convection observed between 0600 and 2100 LT: Variations with Kp. Journal of Geophysical Research 90(A1):393-398.
Crossref

 

Belisheva NK, Kanao M, Kakinami Y, Toyokuni G (2019). The Effect of Space Weather on Human Body at the Spitsbergen Archipelago. Arctic Studies - A Proxy for Climate Change, IntechOpen.
Crossref

 

Bharati K, Amar K, Durbha SR, Gurbax SL (2019). Diminishing activity of recent solar cycles (22-24) and their impact on geospace. Journal of Space Weather and Space Climate 9(A1).
Crossref

 

Broussard RM, Sheeley NR, Tousey R, Underwood JH (1978). A survey of coronal holes and their solar wind associations throughout sunspot cycle 20. Solar Physics 56(1):161-183.
Crossref

 

Crutcher HL (1975). A note on the possible misuse of the Kolmogorov- Smirnov test. Journal of Applied Meteorology 14:1600-1603.
Crossref

 

Despirak IV, Lubchich AA., Kleimenova NG (2018). High-latitude substorm dependence on space weather conditions in solar cycle 23 and 24 (SC23 and SC24). Journal of Atmospheric and Solar-Terrestrial Physics 177:54-62.
Crossref

 

Despiraka IV, Lyubchicha AA, Kleimenovab NG (2019). Solar Wind Streams of Different Types and High-Latitude Substorms. Geomagnetism and Aeronomiy 59(1):1-6.
Crossref

 

Du ZL (2011). The correlation between solar and geomagnetic activity - Part 1: Two-term decomposition of geomagnetic activity. Annales Geophysicae 29(8):1331-1340.
Crossref

 

Durney BR (2000). On the differences between odd and even solar cycles. Solar Physics 196(2):421-426.
Crossref

 

Ebert RW, McComas DJ, Elliott HA, Forsyth RJ, Gosling JT (2009). Bulk properties of the slow and fast solar wind and interplanetary coronal mass ejections measured by Ulysses: Three polar orbits of observations. Journal of Geophysical Research: Space Physics 114(A1)
Crossref

 

Echer E, Gonzalez W, Gonzalez AL, Prestes A, Vieira LE, Dal LA, Guarnieri FL, Schuch NJ (2004). Long-term correlation between solar and geomagnetic activity. Journal of Atmospheric and Solar-Terrestrial Physics 66(12):1019-1025.
Crossref

 

Elena S, Yolanda C, Consuelo C, Venera D, Pavel H, Petko N, Peter S, Josef B, Dimitar D, Crisan D, Walter DG, Georgeta M, Dimitar T, Fridich V (2013). Geomagnetic response to solar and interplanetary disturbances. Journal of Space Weather and Space Climate 3(A26).
Crossref

 

Gabriel CB (2014). Revisiting the critical values of the Lilliefors test: towards the correct agrometeorological use of the Kolmogorov- Smirnov framework, Bragantia, Campinas 73(2):192-202.
Crossref

 

Gazis PR (1996). Solar cycle variation in the heliosphere. Reviews of Geophysics 34(3):379-402.
Crossref

 

Gosling JT, Asbridge JR, Bame SJ, Feldman WC (1976). Solar wind speed variations: 1962-1974. Journal of Geophysical Research, 81(28):5061-5070.
Crossref

 

Hapgood M, Angling MJ, Attrill G, Bisi M, Cannon PS, Dyer C, Eastwood P, Elvidge S, Gibbs M, Harrison RA, Hord C, Horne RB, Jackson DR, Jones B, Machin S, Mitchell CN, Preston J, Rees J, Rogers NC, Routledge G, Ryden K, Tanner R, Thomson AWP, Wild JA, Willis M (2021). Development of Space Weather Reasonable Worst-Case Scenarios for the UK National Risk Assessment. Space Weather 19(4).
Crossref

 

Harvey JW, Sheeley NR (1978). Coronal holes, solar wind streams, and geomagnetic activity during the new sunspot cycle. Solar Physics, 59(1):159−173.
Crossref

 

Intriligator D (1973). Report UAG-27, WDCA Solar Terr. Phys., Boulder.

 

Intriligator D (1977). In M. Shea et al. (eds.), Study of Travelling Interplanetary Phenomena, D. Reidel Pub!. Co., Dordrecht, Holland 195 p.

 

Inza G, Christian Z, Salfo K, Frédéric O (2022). Variability of the magnetospheric electric field due to high-speed solar wind convection from 1964 to 2009. African Journal of Environmental Science and Technology 16(1):1-9.
Crossref

 

Jacob O, Yu L, Amobichukwu CA, Mingyu Z (2020). Responses and Periodic Variations of Cosmic Ray Intensity and Solar Wind Speed to Sunspot Numbers, Advances in Astronomy pp. 1-10.
Crossref

 

Jean-Baptist du P, Gerhard H, Bernd R, Maria B (2009). Confidence Interval or P-Value? Review article 106(19):335-339.

 

Jesper WS (2014). Null hypothesis significance tests. A mix-up of two different theories: the basis for widespread confusion and numerous misinterpretations. Scientometrics 102(1):411-432.
Crossref

 

Joshi NC, Bankoti NS, Pande S, Pande B, Pandey K (2011). Relationship between interplanetary field/plasma parameters with geomagnetic indices and their behavior during intense geomagnetic storms. New Astronomy 16(6):366-385.
Crossref

 

Kabore? S, Ouattara F (2018). Magnetosphere convection electric field (MCEF) time variation from 1964 to 2009: Investigation on the signatures of the geoeffectiveness coronal mass ejections. International Journal of Physical Sciences 13(20):273-281.
Crossref

 

Krieger AS, Timothy AF, Roelof EC (1973). A coronal hole and its identification as the source of a high velocity solar wind stream. Solar Physics, 29(2):505-525.
Crossref

 

Legrand JP, Simon PA (1981). Ten cycles of solar and geomagnetic activity. Solar Physics 70(1):173-195.
Crossref

 

Legrand JP, Simon PA (1989). Solar cycle and geomagnetic activity: a review for geophysicists. Part I. The contributions to geomagnetic activity of shock waves and of the solar wind. Annales Geophysicae 7(6):565-578.

 

Lilliefors HW (1967). On the Kolmogorov-Smirnov test for normality with mean and variance unknown. Journal of the American Statistical Association 62(318):399-402.
Crossref

 

Lindblad BA (1990). Coronal sources of high-speed plasma streams in the solar wind during the declining phase of solar cycle 20. Astrophysics and Space Science 170(1-2):55-61.
Crossref

 

Lindblad BA, Lundstedt H (1981). A Catalogue of High-Speed Plasma Streams in the Solar Wind. Physics of Solar Variations, 197−206.
Crossref

 

Luhmann JG, Lee CO, Li Y, Arge CN, Galvin AB, Simunac K, Petrie G (2009). Solar wind sources in the late declining phase of cycle 23: Effects of the weak. Solar Physics 256(1):285-305.
Crossref

 

Matsui H, Quinn JM, Torbert RB, Jordanova VK, Baumjohann W, Puhl-Quinn PA, Paschmann G (2003). Electric field measurements in the inner magnetosphere by Cluster EDI, Journal of Geophysical Research 108(A9).
Crossref

 

Mavromichalaki H, Vassilaki A (1998). Fast plasma streams recorded near the earth during 1985-1996. Solar Physics, 183(1):181−200.
Crossref

 

Mavromichalaki H, Vassilaki A, Marmatsouri E (1988). A catalogue of high-speed solar-wind streams: Further evidence of their relationship to Ap-index. Solar Physics 115(2):345-365.
Crossref

 

McComas DJ, Bame SJ, Barraclough BL, Feldman WC, Funsten HO, Gosling JT, Riley P, Skoug R, Balogh A, Forsyth R, Goldstein BE, Neugebauer M (1998). Ulysses' return to the slow solar wind. Geophysical Research Letters 25(1):1-4.
Crossref

 

McGregor SL, Hughes WJ, Arge CN, Odstrcil D, Schwadron NA (2011b). The radial evolution of solar wind speeds. Journal of Geophysical Research 116(A3).
Crossref

 

McGregor SL, Hughes WJ, Arge CN, Owens MJ, Odstrcil D (2011a). The distribution of solar wind speeds during solar minimum: Calibration for numerical solar wind modeling constraints on the source of the slow solar wind, Journal of Geophysical Research 116(A3).
Crossref

 

Nick C, Graeme DR (2003). Confidence intervals are a more useful complement to nonsignificant tests than are power calculations, Behavioral Ecology 14(3):446-447.
Crossref

 

Ouattara F, Amory-Mazaudier C (2009). Solar-geomagnetic activity and Aa indices toward a standard classification. Journal of Atmospheric and Solar-Terrestrial Physics 71(17-18):1736-1748.
Crossref

 

Ouattara F, Nour AM, Franc?ois Z (2015). A Comparative Study of Seasonal and Quiettime fof2 Diurnal Variation at Dakar and Ouagadougou Stations during Solar Minimum and Maximum for Solar Cycles 21-22. European Scientific Journal 11(24).

 

Owens MJ, Lockwood M, Riley P (2017). Global solar wind variations over the last four centuries. Scientific Reports 7(1).
Crossref

 

Phillips JL, Bame SJ, Barnes A, Barraclough BL, Feldman WC, Goldstein BE, Gosling JT, Hoogeveen GW, McComas DJ, Neugebauer M, Suess ST (1995). Ulysses solar wind plasma observations from pole to pole. Geophysical Research Letters 22(23):3301-3304.
Crossref

 

Poletto G (2013). Sources of solar wind over the solar activity cycle, Journal of Advanced Research 4(3):215-220.
Crossref

 

Pulkkinen TI, Goodrich CC, Lyon JG (2007). Solar wind electric field driving of magnetospheric activity: Is it velocity or magnetic field?Geophysical Research Letters 34(21):L21101.
Crossref

 

Ranstam J (2012). Why the P-value culture is bad and confidence intervals a better alternative, OsteoArthritis Society International 20(8):805-808.
Crossref

 

Reeves GD, Morley SK, Friedel RHW, Henderson MG, Cayton TE, Cunningham G, Blake B, Christensen AR, Thomsen D (2011). On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited. Journal of Geophysical Research: Space Physics 116(A2).
Crossref

 

Revah I, Bauer P (1982). Rapport d'activite? du Centre de Recherches en Physique de l'environnement Terrestre et Plane?taire, Note technique CRPE/115, 38-40 Rue du Ge?ne?ral Leclerc 92131 Issy-Les Moulineaux.

 

Richardson IG, Cane HV, Cliver EW (2002). Sources of geomagnetic activity during nearly three solar cycles (1972-2000). Journal of Geophysical Research: Space Physics 107(A8):SSH-8.
Crossref

 

Richardson IG, Cliver EW, Cane HV (2000). Sources of geomagnetic activity over the solar cycle: Relative importance of coronal mass ejections, high-speed streams, and slow solar wind. Journal of Geophysical Research 105(A8):18203-18213.
Crossref

 

Richardson IG, Hilary VC (2012). Solar wind drivers of geomagnetic storms during more than four solar cycles. J. Space Weather Space Clim 2(A01).
Crossref

 

Rotter T, Veronig AM, Temmer M, Vrs?nak B (2015). Real- Time Solar Wind Prediction Based on SDO/AIA Coronal Hole Data. Solar Physics 290(5):1355-1370.
Crossref

 

Ruppert D (2004). Statistics and Finance. Springer Texts in Statistics. pp. 1-5.
Crossref

 

Schwenn R (2006). The Solar Perspective. Living Reviews in Solar Physics, Space Weather 3(2).
Crossref

 

Sheeley NR, Harvey JW (1981). Coronal holes, solar wind streams, and geomagnetic disturbances during 1978 and 1979. Solar Physics 70(2):237-249.
Crossref

 

Sheeley NR, Harvey JW, Feldman WC (1976). Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973-1976. Solar Physics 49(2):271-278.
Crossref

 

Shinichi W (2017). Geomagnetic storms of cycle 24 and their solar sources, Planets and Space 69(70).
Crossref

 

Simon PA, Legrand JP (1989). Solar cycle and geomagnetic activity: A review for geophysicists. Part. II. The solar sources of geomagnetic activity and their links with sunspot cycle activity. In Annales geophysicae 7(6):579-594.

 

Snyder C W, Neugebauer M, Rao UR (1963). The solar wind velocity and its correlation with cosmic-ray variations and with solar and geomagnetic activity, Journal of Geophysical Research 68(24):6361-6370.
Crossref

 

Steinskog DJ, Tjøstheim DB, Kvamstø NG (2007). A cautionary note on the use of the Kolmogorov-Smirnov test for normality. American Meteorological Society 135(3):1151-1157.
Crossref

 

Stephens MA (1992). Introduction to Kolmogorov (1933) On the Empirical Determination of a Distribution. Breakthroughs in Statistics pp. 93-105.
Crossref

 

Svalgaard L (1977). Geomagnetic activity: dependence on solar wind parameters, in: Coronal holes and high-speed wind streams, Colorado Association University Press, Boulder pp. 371-432.

 

Takalo J (2021). Comparison of Geomagnetic Indices During Even and Odd Solar Cycles SC17 - SC24: Signatures of Gnevyshev Gap in Geomagnetic Activity. Solar Physics 296(1).
Crossref

 

Tanskanen EI, Slavin JA, Tanskanen AJ, Viljanen A, Pulkkinen TI, Koskinen HEJ, Pulkkinen A, Eastwood J (2005). Magnetospheric substorms are strongly modulated by interplanetary high-speed streams. Geophysical Research Letters 32(16).
Crossref

 

Tukur D (2008). P-value, a true test of statistical significance? A cautionary note. Annals of Ibadan postgraduate medicine 6(1):21-26.

 

Verbanac G, Vrs?nak B, Veronig A, Temmer M (2011a). Equatorial coronal holes, solar wind high-speed streams, and their geoeffectiveness. Astronomy & Astrophysics 526(A20).
Crossref

 

Verbanac G, Vrs?nak B, Z?ivkovic? S, Hojsak T, Veronig AM, Temmer M (2011b). Solar wind high-speed streams and related geomagnetic activity in the declining phase of solar cycle 23. Astronomy & Astrophysics 533(A49).
Crossref

 

Villarreal DC, Schneiter M, Costa A, Vela?zquez P, Raga A, Esquivel A (2014). On the sensitivity of extrasolar mass-loss rate ranges: HD 209458b a case study. Monthly Notices of the Royal Astronomical Society 438(2):1654-1662.
Crossref

 

Vlc?ek O, Huth R, (2009). Is daily precipitation Gamma-distributed? Adverse effects of an incorrect application of the Kolmogorov- Smirnov test. Atmospheric Research 93(4):759-766.
Crossref

 

Wilks DS, (2011). Statistical methods in the atmospheric sciences. 3rd Edition. Academic Press 100 p.
Crossref

 

Wu L, Gendrin R, Higel B, Berchem J (1981). Relationships between the solar wind electric field and the magnetospheric convection electric field. Geophysical Research Letters 8(10):1099-1102.
Crossref

 

Yeeram T (2020). Solar activity phase dependence of the magnetospheric processes and relativistic electron flux at geostationary orbit. Astrophysics and Space Science 365(5):86.
Crossref

 

Zerbo JL, Amory-Mazaudier C, Ouattara F (2013). Geomagnetism during solar cycle 23: Characteristics, Journal of Advanced Research 4(3):265-274.
Crossref

 

Zerbo JL, Amory-Mazaudier C, Ouattara F, Richardson JD (2012). Solar wind and geomagnetism: toward a standard classification of geomagnetic activity from 1868 to 2009. Annales Geophysicae 30(2):421-426.
Crossref