Add to ORKGThe charge states of heavy ions accelerated in the (3)He-Fe rich solar particle event of 1974 May 14-15 are determined using data from the Interplanetary Monitoring Platform-8. In addition to Fe(+11,12) both 0(+5) and Fe(+16,17,18) are also present suggesting variations in coronal temperatures over a range from approximately 400,000 to 5,000,000 K. The presence of 0(+5) and Fe(+16-18) may be explained by a resonant plasma heating mechanism proposed to account for the enhancements of (3)He and Fe
Recent advances in determining the elemental, charge state, and isotopic composition of or approxim...
We report on the ionization states of ∼0.5–50 MeV/nucleon ions in the 6 November 1997 solar particle...
The ionic charge states of solar energetic particles (SEPs) depend upon the temperature of the sourc...
The large solar event on November 6, 1997, was enriched in heavy elements (Fe/O ∼ 1) with very hard ...
Measurements of ionization states and energy spectra of carbon, oxygen, and iron accelerated in ten ...
The charge states of energetic iron have been measured directly for the first time in a solar partic...
Observed charge states of solar energetic ions by Solar, Anomalous, and Magnetospheric Particle Expl...
A survey of the approx. 1 MeV/nucleon heavy ion abundances in 66 He3-rich solar particle events was ...
[1] The Solar and Heliospheric Observatory/Charge, Element, and Isotope Analysis System/(Highly) Sup...
Sustained emission of low energy solar particles with a composition richer in iron than oxygen is ob...
The mean charge states of abundant heavy ions with ∼15–70 MeV nucleon ^(−1) in the two large solar e...
During the May 2–3, 1998 CME event, iron charge state distributions were observed on the ACE spacecr...
Following launch of the Advanced Composition Explorer in August 1997, the Solar Isotope Spectrometer...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
The mean charge states of abundant heavy ions with ~15 - 70 MeV/n in the two large solar energetic ...
Recent advances in determining the elemental, charge state, and isotopic composition of or approxim...
We report on the ionization states of ∼0.5–50 MeV/nucleon ions in the 6 November 1997 solar particle...
The ionic charge states of solar energetic particles (SEPs) depend upon the temperature of the sourc...
The large solar event on November 6, 1997, was enriched in heavy elements (Fe/O ∼ 1) with very hard ...
Measurements of ionization states and energy spectra of carbon, oxygen, and iron accelerated in ten ...
The charge states of energetic iron have been measured directly for the first time in a solar partic...
Observed charge states of solar energetic ions by Solar, Anomalous, and Magnetospheric Particle Expl...
A survey of the approx. 1 MeV/nucleon heavy ion abundances in 66 He3-rich solar particle events was ...
[1] The Solar and Heliospheric Observatory/Charge, Element, and Isotope Analysis System/(Highly) Sup...
Sustained emission of low energy solar particles with a composition richer in iron than oxygen is ob...
The mean charge states of abundant heavy ions with ∼15–70 MeV nucleon ^(−1) in the two large solar e...
During the May 2–3, 1998 CME event, iron charge state distributions were observed on the ACE spacecr...
Following launch of the Advanced Composition Explorer in August 1997, the Solar Isotope Spectrometer...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
The mean charge states of abundant heavy ions with ~15 - 70 MeV/n in the two large solar energetic ...
Recent advances in determining the elemental, charge state, and isotopic composition of or approxim...
We report on the ionization states of ∼0.5–50 MeV/nucleon ions in the 6 November 1997 solar particle...
The ionic charge states of solar energetic particles (SEPs) depend upon the temperature of the sourc...