MeV/nucleon 0010 and above/ A9660R Solar flares, bursts, and related phenomena A9660V Solar particle radiation, solar windThe influence of Coulomb collisions in two-component plasma on the nuclear composition and the charge-state of accelerated particles is investigated. The main characteristics are...
Plastic and glass track detectors on rockets and Apollo spacecraft have been used to determine the composition of particles from He to Ni at energies from 0.1 to 50 MeV per nucleon in several solar flares of widely varying intensities. At low energies the composition of solar particles is enric...
Fe, and Si) and their relative abundances are correlated well, while no clear correlation is observed between the C6+/C5+or C6+/C4+and C/O. Most interestingly, we find that the Ne/O ratios of ICMEs and slow solar wind have the ...
As more (less) fractions of ICMEs originate from active regions around solar maximum (minimum), and active-region ICMEs usually are associated with higher-class flares, our studies might answer why ICME composition measured near 1 au exhibits the solar cycle dependence. 展开 ...
The abundances of most of these heavy elements are enriched over the solar composition, providing a window into the evolution of the primordial nebula material incorporated into the gas giants during their formation (Lunine et al., 2004). Spectroscopic mapping from the UV to the submillimetre will...
of atmospheres that exist on these small planets by searching for evidence of molecules like water, carbon dioxide, and methane in their atmospheres. Because M dwarfs are typically much more active than the Sun and have energetic stellar flares that could potentially strip the atmospheres off of ...
Observations of newly ionized atoms that are picked up by the magnetic field in the expanding solar wind contain crucial information about the gas or dust compositions of their origins. The pickup ions (PUIs) are collected by plasma mass spectrometers and analyzed for their density, composition, ...
In a similar way, past (Messenger) and current (BepiColombo) missions to Mercury are expected to provide a new view of the bulk and exosphere composition of this planet, the only example of a hot close-in terrestrial planet in our Solar System. While remote sensing and in situ measurements...
The last five years represent a quite remarkable peak in the field of magnetospheric composition studies with, at times, up to six satellites carrying mass spectrometers and, in addition, with ISEE-3 monitoring the solar wind composition.
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