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Volumn 38, Issue 2, 2006, Pages 226-231

The Carrington event: Possible doses to crews in space from a comparable event

Author keywords

Carrington Flare; Solar energetic particle event; Space radiation; Space radiation risks; Total ionizing doses

Indexed keywords

DATA REDUCTION; ELECTRONIC EQUIPMENT; PROTONS; SOLAR ENERGY; SPECTRUM ANALYSIS;

EID: 33749578681     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.01.111     Document Type: Article
Times cited : (56)

References (12)
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  • 4
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    • The Carrington event: Possible solar proton intensity-time profile
    • Smart D.F., Shea M.A., and McCracken K.G. The Carrington event: Possible solar proton intensity-time profile. Adv. Space Res. 38 (2006) 215-225
    • (2006) Adv. Space Res. , vol.38 , pp. 215-225
    • Smart, D.F.1    Shea, M.A.2    McCracken, K.G.3
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    • Interplanetary crew dose estimates for worst case solar particle events based on the historical data for the Carrington flare of 1859
    • Stephens Jr. D.L., Townsend L.W., and Hoff J.L. Interplanetary crew dose estimates for worst case solar particle events based on the historical data for the Carrington flare of 1859. Acta Astronaut. 56 (2005) 969-974
    • (2005) Acta Astronaut. , vol.56 , pp. 969-974
    • Stephens Jr., D.L.1    Townsend, L.W.2    Hoff, J.L.3
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    • Townsend, L.W., Stephens, D.L., Hoff, J.L., Braley, G.S., Moussa, H.M. Worst case solar energetic particle events for deep space missions, in: 2001 International Conference on Environmental Systems, Orlando, FL, July 9-12, SAE Paper No. 01ICES-292, 2001.
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    • Carrington flare of 1859 as a prototypical worst case solar energetic particle event
    • Townsend L.W., Zapp E.N., Stephens Jr. D.L., and Hoff J.L. Carrington flare of 1859 as a prototypical worst case solar energetic particle event. IEEE Trans. Nucl. Sci. 50 6 (2003) 2307-2309
    • (2003) IEEE Trans. Nucl. Sci. , vol.50 , Issue.6 , pp. 2307-2309
    • Townsend, L.W.1    Zapp, E.N.2    Stephens Jr., D.L.3    Hoff, J.L.4
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.