The Spectrum of the 1/4 keV Band Diffuse Soft X-ray Background

Details The Spectrum of the 1/4 keV Band Diffuse Soft X-ray Background The Spectrum of the 1/4 keV Band Diffuse Soft X-ray Background

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1156...24e&link_type=abstract

THE LOCAL BUBBLE AND BEYOND II: Proceedings of the International Conference. AIP Conference Proceedings, Volume 1156, pp. 24-28

Computer Science

Databases

X-Ray, Particle Emission, Solar Wind, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc.

Scientific paper

The spectrum of the 145-284 eV (42-85 Angstrom) band of a portion of the diffuse x-ray sky was obtained in 1993 by the Diffuse X-ray Spectrometer. We compare these data to a model including a computation of the spectra of a few ions due to solar wind charge exchange in the heliosphere, obtaining solar wind parameter ranges by studying the in situ observations at a similar phase in the following solar cycle, i.e. in 2003. The one spectral feature which is consistent with an unblended, isolated line is coincident with the hydrogenic oxygen Balmer γ (n = 5 to 2) transition, which should be strongly pumped by charge exchange.

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