Abstract
Interplanetary coronal mass ejections (ICMEs) and corotating interaction regions (CIRs) are the major characteristic events of the solar wind (SW). We used proton flux data with different energy levels provided by the Low Energy Magnetic Spectrometers (LEMS) 120 system of the Electron, Proton and Alpha Monitor (EPAM) for studying different ICME-driven and CIR-driven storms. Our main aim was to find, from the observational results, the nature of the proton flux during solar storms driven by different mechanisms that, in our cases, are related to ICMEs and CIRs, in the interplanetary regions. We analyzed the different parameters provided by the LEMS 120 system and compared them during the different storm types and during a selected quietest day as well. We studied four events: a geomagnetically quiet day, two ICME-driven storms and one CIR-driven storm. We also analyzed the interplanetary magnetic field (IMF) magnitude (\(B_{\mathrm{mag}}\)) and the different SW parameters during all these events. We observed that both the prolonged particle precipitations during CIRs and the intense particle precipitations during ICMEs result in the different nature of the fluxes with different energy levels compared with other parameters such as \(B_{\mathrm{mag}}\), and the SW velocity (\(V_{\mathrm{sw}}\)). Our quiet-period results show that there is a strong correlation between the higher energy proton fluxes and \(B_{\mathrm{mag}}\) and \(V_{\mathrm{sw}}\) and a weak correlation in the case of lower energy protons. Our storm-time results demonstrate that when the storm is either driven by ICMEs or CIRs, the lower energy protons also starts to show positive correlations with \(B_{\mathrm{mag}}\) and \(V_{\mathrm{sw}}\) with a 0 min time lag (TA) during ICMEs and with a \({\approx}\,{-}100~\mbox{min}\) TA during CIRs. During the quiet day, the proton flux observed was due to the perturbations created by ionization and the higher energy of the protons sufficiently weakened. Whereas, the CME speed, the preceding CMEs, and the presence of pre-existing solar energetic particles (SEPs) in the ambient medium, the makeup of CIR-related winds, and the nature of precipitation during both ICMEs and CIRs caused the proton fluxes with different energy levels during storm times.
Similar content being viewed by others
References
Adhikari, B., Baruwal, P., Chapagain, N.P.: 2017, Analysis of supersubstorm events with reference to polar cap potential and polar cap index. Earth Space Sci. 4, 2. DOI .
Adhikari, B., Dahal, S., Chapagain, N.P.: 2017, Study of field-aligned current (FAC), interplanetary electric field component (\(E_{y}\)), interplanetary magnetic field component (\(B _{z}\)), and northward (\(x\)) and eastward (\(y\)) components of geomagnetic field during supersubstorm. Earth Space Sci. 4, 257. DOI .
Adhikari, B., Sapkota, N., Baruwal, P., Chapagain, N.P., Braga, C.R.: 2017, Impacts on cosmic-ray intensity observed during geomagnetic disturbances. Solar Phys. 292(10), 149. DOI .
Adhikari, B., Dahal, S., Sapkota, N., Baruwal, P., Bhattarai, B., Khanal, K., Chapagain, N.P.: 2018, Field aligned current and polar cap potential and geomagnetic disturbances: a review of cross correlation analysis. Earth Space Sci. 5(9), 440. DOI .
Alves, M.V., Echer, E., Gonzalez, W.D.: 2006, Geoeffectiveness of corotating interaction regions as measured by Dst index. J. Geophys. Res. 111(A7), A07S05. DOI .
Barbas de Haro, B.F., Elias, A.G., Cnossen, I., de Artigas, M.Z.: 2013, Long-term changes in solar quiet (Sq) geomagnetic variations related to Earth’s magnetic field secular variation. J. Geophys. Res. Space Phys. 118(6), 3712. DOI .
Beutier, T., Boscher, D., France, M.: 1995, SALAMMBO: a three-dimensional simulation of the proton radiation belt. J. Geophys. Res. 100(A9), 17181. DOI .
Bolaji, O.S., Adimula, I.A., Adeniyi, J.O., Yumoto, K.: 2013, Variability of horizontal magnetic field intensity over Nigeria during low solar activity. Earth Moon Planets 110(1–2), 91. DOI .
Borovsky, J.E.: 2016, The plasma structure of coronal hole solar wind: origins and evolution. J. Geophys. Res. 121(6), 5055. DOI .
Borovsky, J.E., Denton, M.H.: 2006, Differences between CME-driven storms and CIR-driven storms. J. Geophys. Res. 111(A7), A07S08. DOI .
Brown, R.R., Driatsky, V.M.: 1973, Further studies of ionospheric and geomagnetic effects of sudden impulses. Planet. Space Sci. 21(11), 1931. DOI .
Brown, R.R., Hartz, T.R., Landmark, B., Leinbach, H., Ortner, J.: 1961, Large-scale electron bombardment of the atmosphere at the sudden commencement of a geomagnetic storm. J. Geophys. Res. 66(4), 1035. DOI .
Brown, R.R., Leinbach, H., Akasofu, S.I., Driatsky, V.M., Schmidt, R.J.: 1972, Quadruple conjugate pair observations of the sudden commencement absorption event on June 17. J. Geophys. Res. 77(28), 5602. DOI . 1965.
Cane, H.V., Reames, D.V., Rosenvinge, T.T.: 1988, The role of interplanetary shocks in the longitude distribution of solar energetic particles. J. Geophys. Res. 93(A9), 9555. DOI .
Cane, H.V., Sheeley, N.R., Howard, R.A.: 1987, Energetic interplanetary shocks, radio emission, and coronal mass ejections. J. Geophys. Res. 92(A9), 9869. DOI .
Chapman, S.: 1919, I. The solar and lunar diurnal variations of terrestrial magnetism. Phil. Trans. Roy. Soc. London 218(561–569), 1. DOI .
Chupp, E.L.: 1988, Solar neutron observations and their relation to solar flare acceleration problems. Solar Phys. 118(1–2), 137. DOI .
Cornwall, J.M.: 1972, Radial diffusion of ionized helium and protons: a probe for magnetospheric dynamics. J. Geophys. Res. 77(10), 1756. DOI .
Dmitriev, A.V., Crosby, N.B., Chao, J.K.: 2005, Interplanetary sources of space weather disturbances in 1997 to 2000. Adv. Space Res. 3(3), 1. DOI .
Emslie, A.G., Dennis, B.R., Shih, A.Y., Chamberlin, P.C., Mewaldt, R.A., Moore, C.S., et al.: 2012, Global energetics of thirty-eight large solar eruptive events. Astrophys. J. 759(1), 71. DOI .
Fan, C.Y., Pick, M., Pyle, R., Simpson, J.A., Smith, D.R.: 1968, Protons associated with centers of solar activity and their propagation in interplanetary magnetic field regions corotating with the Sun. J. Geophys. Res. 73(5), 1555. DOI .
Finch, I., Lockwood, M.: 2007, Solar wind-magnetosphere coupling functions on timescales of 1 day to 1 year. Ann. Geophys. 25, 495. DOI .
Georgoulis, M.K., Papaioannou, A., Sandberg, I., Anastasiadis, A., Daglis, I.A., Rodríguez-Gasén, R., et al.: 2018, Analysis and interpretation of inner-heliospheric SEP events with the ESA Standard Radiation Environment Monitor (SREM) onboard the INTEGRAL and Rosetta missions. J. Space Weather Space Clim. 8, A40. DOI .
Gleisner, H., Watermann, J.: 2006, Solar energetic particle flux enhancement as an indicator of halo coronal mass ejection geoeffectiveness. Adv. Space Res. 4(6), 1. DOI .
Gold, R.E., Krimigis, S.M., Hawkins, S.E., Haggerty, D.L., Lohr, D.A., Fiore, E., et al.: 1998, Electron, Proton, and Alpha Monitor on the Advanced Composition Explorer spacecraft. Space Sci. Rev. 86(1–4), 541. DOI .
Gonzalez, W.D., Tsurutani, B.T., De Gonzalez, A.L.C.: 1999, Interplanetary origin of geomagnetic storms. Space Sci. Rev. 88(3–4), 529. DOI .
Gopalswamy, N., Yashiro, S., Kaiser, M.L., Howard, R.A.: 2003, Coronal mass ejection interaction and particle acceleration during the 2001 April 14–15 events. Adv. Space Res. 32(12), 2613. DOI .
Gopalswamy, N., Nunes, S., Yashiro, S., Howard, R.A.: 2004, Variability of solar eruptions during cycle 23. Adv. Space Res. 34(2), 391. DOI .
Gosling, J.T., Pizzo, V.J.: 1999, Formation and evolution of corotating interaction regions and their three-dimensional structure. In: Corotating Interaction Regions, Springer, Dordrecht, 21. DOI .
Guido, R.M.D.: 2016, Coronal mass ejections during geomagnetic storms on Earth. J. Astrophys. Astron. 5(2), 19. DOI .
Hudson, H.S.: 2011, Global properties of solar flares. Space Sci. Rev. 158(1), 5. DOI .
Illing, R.M.E., Hundhausen, A.T.: 1986, Disruption of a coronal streamer by an eruptive prominence and coronal mass ejection. J. Geophys. Res. 91(A10), 10951. DOI .
Kahler, S.W., Hildner, E., Van Hollebeke, M.A.I.: 1978, Prompt solar proton events and coronal mass ejections. Solar Phys. 57(2), 429. DOI .
Katz, R.W.: 1988, Use of cross correlations in the search for teleconnections. Int. J. Climatol. 8(3), 241. DOI .
Kennel, C.F., Scarf, F.L., Coroniti, F.V., Russell, C.T., Wenzel, K.P., Sanderson, T.R., et al.: 1984, Plasma and energetic particle structure upstream of a quasi-parallel interplanetary shock. J. Geophys. Res. 89(A7), 5419. DOI .
Kozyra, J.U., Rasmussen, C.E., Miller, R.H., Lyons, L.R.: 1994, Interaction of ring current and radiation belt protons with ducted plasmaspheric hiss: 1. Diffusion coefficients and timescales. J. Geophys. Res. 99(A3), 4069. DOI .
Lazutin, L.L., Kuznetsov, S.N., Podorol’skii, A.N.: 2007, Dynamics of the radiation belt formed by solar protons during magnetic storms. Geomagn. Aeron. 47(2), 175. DOI .
Longden, N., Denton, M.H., Honary, F.: 2008, Particle precipitation during ICME-driven and CIR-driven geomagnetic storms. J. Geophys. Res. 113(A6), A06205. DOI .
Malandraki, O.E., Lario, D., Lanzerotti, L.J., Sarris, E.T., Geranios, A., Tsiropoula, G.: 2005, October/November 2003 interplanetary coronal mass ejections: ACE/EPAM solar energetic particle observations. J. Geophys. Res. 110(A9), A09S06. DOI .
McCracken, K.G., Rao, U.R., Bukata, R.P., Keath, E.: 1971, The decay phase of solar flare events. Solar Phys. 18(1), 100. DOI .
Mewaldt, R.A., Stone, E.C., Vogt, R.E.: 1979, Characteristics of the spectra of protons and alpha particles in recurrent events at 1 AU. Geophys. Res. Lett. 6(7), 589. DOI .
Nakada, M.P., Dungey, J.W., Hess, W.N.: 1965, On the origin of outer-belt protons: 1. J. Geophys. Res. 70(15), 3529. DOI .
Ngwira, C.M., Pulkkinen, A., Wilder, F.D., Crowley, G.: 2013, Extended study of extreme geoelectric field event scenarios for geomagnetically induced current applications. Adv. Space Res. 11(3), 121. DOI .
Palmer, I.D., Gosling, J.T.: 1978, Shock-associated energetic proton events at large heliocentric distances. J. Geophys. Res. 83(A5), 2037. DOI .
Richardson, I.G.: 2004, Energetic particles and corotating interaction regions in the solar wind. Space Sci. Rev. 111(3–4), 267. DOI .
Richardson, I.G., Cliver, E.W., Cane, H.V.: 2000, Sources of geomagnetic activity over the solar cycle: relative importance of coronal mass ejections, high-speed streams, and slow solar wind. J. Geophys. Res. 105(A8), 18203. DOI .
Sergeev, V.A., Chernyaeva, S.A., Apatenkov, S.V., Ganushkina, N.Y., Dubyagin, S.V.: 2015, Energy-latitude dispersion patterns near the isotropy boundaries of energetic protons. Ann. Geophys. 33, 1059. DOI .
Sheeley, N.R., Howard, R.A., Koomen, M.J., Michels, D.J., Schwenn, R., Muehlhaeuser, K.H., Rosenbauer, H.: 1985, Coronal mass ejections and interplanetary shocks. J. Geophys. Res. 90(A1), 163. DOI .
Shibata, K., Magara, T.: 2011, Solar flares: magnetohydrodynamic processes. Solar Phys. 8(1), 6. DOI .
Smith, E.J., Wolfe, J.H.: 1976, Observations of interaction regions and corotating shocks between one and five AU: Pioneers 10 and 11. Geophys. Res. Lett. 3(3), 137. DOI .
Smolin, S.V.: 2010, Effect of magnetospheric convection on the energy distribution of protons from the Earth radiation belts. Geomagn. Aeron. 50(3), 298. DOI .
Søraas, F., Aarsnes, K., Lundblad, J., Evans, D.S.: 1999, Enhanced pitch angle scattering of protons at mid-latitudes during geomagnetic storms. Phys. Chem. Earth, Part C Solar-Terr. Planet. Sci. 24(1–3), 287. DOI .
Spjeldvik, W.N.: 1977, Equilibrium structure of equatorially mirroring radiation belt protons. J. Geophys. Res. 82(19), 2801. DOI .
Stauning, P.: 1996, Investigations of ionospheric radio wave absorption processes using imaging riometer techniques. J. Atmos. Terr. Phys. 58(6), 753. DOI .
Tsurutani, B.T., Lin, R.P.: 1985, Acceleration of \({>}\,47~\mbox{keV}\) ions and \({>}\,2~\mbox{keV}\) electrons by interplanetary shocks at 1 AU. J. Geophys. Res. 90(A1), 1. DOI .
Tsurutani, B.T., Gould, T., Goldstein, B.E., Gonzalez, W.D., Sugiura, M.: 1990, Interplanetary Alfvén waves and auroral (substorm) activity: IMP 8. J. Geophys. Res. 95, 2241. DOI .
Tsurutani, B.T., Gonzalez, W.D., Gonzalez, A.L., Guarnieri, F.L., Gopalswamy, N., Grande, M., et al.: 2006, Corotating solar wind streams and recurrent geomagnetic activity: a review. J. Geophys. Res. 111(A7), A07S01. DOI .
Tsurutani, B.T., Verkhoglyadova, O.P., Mannucci, A.J., Lakhina, G.S., Li, G., Zank, G.P.: 2009, A brief review of “solar flare effects” on the ionosphere. Radio Sci. 44(1), RS0A17. DOI .
Tylka, A.J., Lee, M.A.: 2006, A model for spectral and compositional variability at high energies in large, gradual solar particle events. Astrophys. J. 646(2), 1319. DOI .
Tylka, A.J., Cohen, C.M.S., Dietrich, W.F., Lee, M.A., Maclennan, C.G., Mewaldt, R.A., et al.: 2005, Shock geometry, seed populations, and the origin of variable elemental composition at high energies in large gradual solar particle events. Astrophys. J. 625(1), 474. DOI .
Vacaresse, A., Boscher, D., Bourdarie, S., Blanc, M., Sauvaud, J.A.: 1999, Modeling the high-energy proton belt. J. Geophys. Res. 104(A12), 28601. DOI .
Yizengaw, E., Moldwin, M.B., Komjathy, A., Mannucci, A.J.: 2006, Unusual topside ionospheric density response to the November 2003 superstorm. J. Geophys. Res. 111(A2), A02308. DOI .
Zurbuchen, T.H., Richardson, I.G.: 2006, In-situ solar wind and magnetic field signatures of interplanetary coronal mass ejections. Space Sci. Rev. 123(1–3), 31. DOI .
Acknowledgements
We are grateful to the OMNI Database for providing the data. The interplanetary magnetic field magnitude data and solar wind parameters for this study were obtained from https://omniweb.gsfc.nasa.gov/ . We thank the ACE instrument team and the ACE Science Center for providing the ACE data. We downloaded the proton flux data from http://www.srl.caltech.edu/ACE/ .
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Conflict of Interest
The authors declare that they have no conflict of interest.
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
About this article
Cite this article
Adhikari, B., Adhikari, N., Aryal, B. et al. Impacts on Proton Fluxes Observed During Different Interplanetary Conditions. Sol Phys 294, 61 (2019). https://doi.org/10.1007/s11207-019-1450-6
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-019-1450-6