Effects of coronal holes on the propagation of solar energetic protons

Radiation Measurements

Volumn 30, Issue 3, 1999, Pages 281-286

  Kunches, Joseph M ^a   Zwickl, Ronald D ^a  

^a NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC RAYS; LIGHT PROPAGATION; PARTICLE ACCELERATORS; SOLAR ENERGY; SOLAR RADIATION; WEATHER FORECASTING; WEATHER SATELLITES;

CORONAL HOLES; GEOSYNCHRONOUS SATELLITE; HELIOLONGITUDE; PLASMA CONDITION; SOLAR ENERGETIC PROTONS;

PROTONS;

PROTON;

ARTICLE; COSMIC RADIATION; FORECASTING; INSTRUMENTATION; METHODOLOGY; SOLAR ENERGY; SPACE FLIGHT;

COSMIC RADIATION; FORECASTING; PROTONS; SOLAR ACTIVITY; SPACECRAFT;

EID: 0033237354     PISSN: 13504487     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1350-4487(99)00056-6     Document Type: Article

References (11)

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9. Sheeley, N.R., Howard, R.A., Koomen, M.J., Michels, D.J., Schwenn, R., Muhlhauswe, K.H., Rosenbauer, H., 1985. Coronal mass ejections and interplanetary shocks. J. Geophys. Res. 90, 163-175.
10. Smart, D.F., Shea, M.A., 1979. PPS76 - A computerized "event mode" solar proton forecasting technique. In: Solar-Terrestrial Predictions Proceedings, vol. 1. National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Boulder, CO, pp. 406-427.
11. Steinolfson, R.S., Mullan, D.J., 1980. Magnetohydrodynamic shock propagation in the vicinity of a magnetic neutral sheet. Astrophys. J. 241, 1186-1194.