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Enhancement of Trans-Iron Elements in Impulsive Solar Flares. Trans-iron elements are extremely rare in the solar system composition: in the mass range from germanium to bismuth (32≤Z≤83), their total meteoritic abundance is only ~10 -4 that of iron. - PowerPoint PPT Presentation
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SS
Space Science MO&DA Programs - January 2001 - Page 1
•We report a preliminary search for trans-iron particles from flares using the ACE/ULEIS instrument which is sensitive at energies (>30 keV/nuc) where solar-particle fluxes are highest.
•The figure shows abundances from a sum of at least 8 flares (black trace). The ULEIS mass scale beyond 70 is preliminary and will be verified by accelerator calibration of a backup unit.
•Compared to meteorites and the photosphere (blue trace) we find > 100-fold enrichments of elements beyond iron in particles from flares. Reames has also recently reported large enhancements of trans-iron elements in impulsive flares above ~3 MeV/nucleon.
10-7
10-5
10-3
10-1
101
10 100
abu
ndan
ce (
ox
yg
en=
1)
mass (amu)
C NO
NeMgSi
SCa
Fe
preliminary ACE/ULEIS trans-Fe abundances &
mass ranges
solar photosphere and meteorites(Grevesse & Sauval 1998)
ACE/ULEIS impulsive flares
As-Mo
Sb-Ce Tb-Bi
•Trans-iron elements are extremely rare in the solar system composition: in the mass range from germanium to bismuth (32≤Z≤83), their total meteoritic abundance is only ~10-4 that of iron.
Enhancement of Trans-Iron Elements in Impulsive Solar Flares
SS
Space Science MO&DA Programs - January 2001 - Page 2
•The impulsive flare particles are easily seen at the beginning of 7/1/99 where the high iron/oxygen ratio is typical for flares. The count rate of ultra-heavy ions peaked at the same time as the iron.
•The composition was more coronal-like on 7/2/99, but there were far fewer ultra-heavies.
•Most of the ions with mass > 70 amu arrived at ACE during impulsive solar flares. Shown above are oxygen and iron fluxes at ~0.2 MeV/nucleon energy for 4 days in 1999.
10-2
10-1
100
101
0
4
8
6/30/1999 7/2/1999 7/4/1999
part
icle
flu
x
counts per hour
oxygeniron
ions withmass >70 amu
•These preliminary results show that either before or during acceleration, an enrichment mechanism favoring higher mass species brings the rare trans-iron abundances within reach of present instrumentation.
Enhancement of Trans-Iron Elements in Impulsive Solar Flares (2)
Contributed by Joe Mazur, Glenn Mason, Joe Dwyer, Rob Gold and Tom Krimigis