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地球与行星物理

ISSN  2096-3955

CN  10-1502/P

Citation: Wang, X.-D., Klecker, B., Nicolaou, G., Barabash, S., Wieser, M., Wurz, P., Galli, A., Cipriani, F., and Futaana, Y. (2022). Neutralized solar energetic particles for SEP forecasting: Feasibility study of an innovative technique for space weather applications. Earth Planet. Phys., 6(1), 42–51. http://doi.org/10.26464/epp2022003

2022, 6(1): 42-51. doi: 10.26464/epp2022003

SPACE PHYSICS: SOLAR PHYSICS

Neutralized solar energetic particles for SEP forecasting: Feasibility study of an innovative technique for space weather applications

1. 

Swedish Institute of Space Physics, Kiruna, Sweden

2. 

Max-Planck Institute für extraterrestrische Physik, Garching, Germany

3. 

Physics Institute, University of Bern, Bern, Switzerland

4. 

ESA/ESTEC, Research and Scientific Support Department, Noordwijk, The Netherlands

Corresponding author: Xiao-Dong Wang, wang@irf.se

Received Date: 2021-06-22
Web Publishing Date: 2021-12-06

Energetic neutral atoms (ENAs) are produced by the neutralization of energetic ions formed by shock-accelerated gradual solar energetic particle events (SEP). These high-energy ENAs (HENAs) can reach the Earth earlier than the associated SEPs and thus can provide information about the SEPs at the lower corona. The HENA properties observed at Earth depend on the properties of the coronal mass ejection (CME)-driven shocks that accelerate the SEPs. Using a model of HENA production in a shock-accelerated SEP event, we semi-quantitatively investigate the energy-time spectrum of HENAs depending on the width, propagation speed, and direction of the shock, as well as the density and ion abundances of the lower corona. Compared to the baseline model parameters, the cases with a wider shock width angle or a higher coronal density would increase the HENA flux observed at the Earth, while the case with an Earth-propagating shock shows a softened HENA spectrum. The comparison of expected HENA fluxes in different cases with a flight-proven ENA instrument suggests that solar HENAs can feasibly be monitored with current technologies, which could provide a lead time of 2−3 hours for SEPs at a few MeV. We propose that monitoring of solar HENAs could provide a new method to forecast shock-driven SEP events that are capable of significant space weather impacts on the near-Earth environment.

Key words: solar energetic particles; energetic neutral atoms; space weather; numerical simulation

Allen, L. A., Habbal, S. R., and Li, X. (2000). Thermal coupling of protons and neutral hydrogen with anisotropic temperatures in the fast solar wind. J. Geophys. Res. :Space Phys., 105(A10), 23123–23134. https://doi.org/10.1029/1999JA000437

Andersen, L. H., and Bolko, J. (1990). Radiative recombination between fully stripped ions and free electrons. Phys. Rev. A, 42(3), 1184–1191. https://doi.org/10.1103/PhysRevA.42.1184

Aschwanden, M. J. (2005). Physics of the Solar Corona: an Introduction with Problems and Solutions. Chichester, UK: Praxis Publishing Ltd.222

Barnett, C. F. , Hunter, H. T. , Kirkpatrick, M. I. , Alvarez, I. , Cisneros, C. , and Phaneuf, R. A. (1990). Atomic data for fusion volume 1: collisions of H, H2, He and Li atoms and ions with atoms and molecules. ORNL-6086/V1, Oak Ridge, Tennessee: Oak Ridge National Laboratory.222

D’Amicis, R., Orsini, S., Antonucci, E., Di Lellis, A. M., Hilchenbach, M., Telloni, D., Mura, A., Milillo, A., Fineschi, S., and Bruno, R. (2007). Numerical simulations of coronal hole-associated neutral solar wind as expected at the Solar Orbiter position. J. Geophys. Res. :Space Phys., 112(A6), A06110. https://doi.org/10.1029/2006JA011969

Gruntman, M. (1997). Energetic neutral atom imaging of space plasmas. Rev. Sci. Instrum., 68(10), 3617–3656. https://doi.org/10.1063/1.1148389

Gruntman, M., Roelof, E. C., Mitchell, D. G., Fahr, H. J., Funsten, H. O., and McComas, D. J. (2001). Energetic neutral atom imaging of the heliospheric boundary region. J. Geophys. Res. :Space Phys., 106(A8), 15767–15781. https://doi.org/10.1029/2000JA000328

Gruntman, M. A. (1994). Neutral solar wind properties: advance warning of major geomagnetic storms. J. Geophys. Res. :Space Phys., 99(A10), 19213–19227. https://doi.org/10.1029/94JA01571

Hsieh, K. C. , Shih, K. L. , McComas, D. J. , Wu, S. T. , and Wu, C. (1992). Forecasting the arrival of fast coronal-mass ejecta at Earth by the detection of 2-20keV neutral atoms. In Proceedings of SPIE 1744, Instrumentation for Magnetospheric Imagery (pp. 72-78). San Diego: SPIE.222

Kahler, S. W. (2001). The correlation between solar energetic particle peak intensities and speeds of coronal mass ejections: effects of ambient particle intensities and energy spectra. J. Geophys. Res. :Space Phys., 106(A10), 20947–20955. https://doi.org/10.1029/2000JA002231

Klein, K. L., and Dalla, S. (2017). Acceleration and propagation of solar energetic particles. Space Sci. Rev., 212(3-4), 1107–1136. https://doi.org/10.1007/s11214-017-0382-4

Kuang, Y. R. (1992). Electron capture by protons and alpha particles from two-electron targets. J. Phys. B:At. Mol. Opt. Phys., 25(1), 199–211. https://doi.org/10.1088/0953-4075/25/1/023

Lamy, P. L., Floyd, O., Boclet, B., Wojak, J., Gilardy, H., and Barlyaeva, T. (2019). Coronal mass ejections over solar cycles 23 and 24. Space Sci. Rev. , 215(5), 39. https://doi.org/10.1007/s11214-019-0605-y

Lee, M. A. (2005). Coupled hydromagnetic wave excitation and ion acceleration at an evolving coronal/interplanetary shock. Astrophys. J. Suppl. S., 158(1), 38–67. https://doi.org/10.1086/428753

Mewaldt, R. A., Leske, R. A., Stone, E. C., Barghouty, A. F., Labrador, A. W., Cohen, C. M. S., Cummings, A. C., Davis, A. J., von Rosenvinge, T. T., and Wiedenbeck, M. E. (2009). STEREO observations of energetic neutral hydrogen atoms during the 2006 December 5 solar flare. Astrophys. J., 693(1), L11–L15. https://doi.org/10.1088/0004-637X/693/1/L11

Mitchell, D. G., Cheng, A. F., Krimigis, S. M., Keath, E. P., Jaskulek, S. E., Mauk, B. H., McEntire, R. W., Roelof, E. C., Williams, D. J., … Drake, V. A. (1993). INCA: the ion neutral camera for energetic neutral atom imaging of the Saturnian magnetosphere. Opt. Eng., 32(12), 3096–3101. https://doi.org/10.1117/12.155609

Reames, D. V. (1997). Energetic particles and the structure of coronal mass ejections. In N. Crooker, et al. (Eds. ), Coronal Mass Ejections, Volume 99 (pp. 217-226). Washington, DC: American Geophysical Union.222

von Steiger, R., Schwadron, N. A., Fisk, L. A., Geiss, J., Gloeckler, G., Hefti, S., Wilken, B., Wimmer-Schweingruber, R. R., and Zurbuchen, T. H. (2000). Composition of quasi-stationary solar wind flows from Ulysses/Solar Wind Ion Composition Spectrometer. J. Geophys. Res. :Space Phys., 105(A12), 27217–27238. https://doi.org/10.1029/1999JA000358

Wang, L. H., Li, G., Shih, A. Y., Lin, R. P., and Wimmer-Schweingruber, R. F. (2014). Simulation of energetic neutral atoms from solar energetic particles. Astrophys. J. Lett., 793(2), L37. https://doi.org/10.1088/2041-8205/793/2/L37

Wurz, P. , and Gabriel, A. (1999). Working group 4: wind acceleration processes. In Proceedings of the 8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona (pp. 87). Paris, France: ESA, NASA, C. N. R. S. -I. N. S. U.222

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Neutralized solar energetic particles for SEP forecasting: Feasibility study of an innovative technique for space weather applications

Xiao-Dong Wang, B. Klecker, G. Nicolaou, S. Barabash, M. Wieser, P. Wurz, A. Galli, F. Cipriani, Y. Futaana