The investigation of powerful solar flares characteristics by analysis of excited states of 12C and various neutrons capture lines

Arkhangelskaja, I. V.; Arkhangelsky, A. I.; Troitskaya, E. V.; Miroshnichenko, L. I.

doi:10.1016/j.asr.2008.11.002

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Density Profiles Of Flaring Atmosphere1

Photospheric 3 He Abundance1

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Cited by 11 publications

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“…The EDE for this flare may be obtained only by involving an additional assumption (see Sect. 12.4) about enhanced abundance of 3 He nuclei in this extraordinary solar event (Arkhangelskaja et al 2009c;Troitskaia et al 2009Troitskaia et al , 2011. In spite of this controversial situation, these EDE findings (at least, for four major solar flares, see above) seem to be indirectly confirmed by recent optical results by Cessateur et al (2010).…”

Section: Density Profiles Of Flaring Atmospherementioning

confidence: 91%

“…One of the recent attempts to derive the photospheric 3 He/He ratio was undertaken by Arkhangelskaja et al (2009c) by the data of CORONAS/AVS-F for the flare of 20 January 2005. The authors have shown that this extraordinary solar event may be satisfactorily treated provided that strongly enhanced abundance of 3 He nuclei took place in the solar photosphere.…”

Section: Photospheric 3 He Abundancementioning

confidence: 99%

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