Terrestrial Consequences of Spectral and Temporal Variability in Ionizing Photon Events

Details Terrestrial Consequences of Spectral and Temporal Variability in Ionizing Photon Events Terrestrial Consequences of Spectral and Temporal Variability in Ionizing Photon Events

2006-04-26

arxiv.org/abs/astro-ph/0604556v3

Astrophys.J.654:373-384,2007

Astronomy and Astrophysics

Astrophysics

30 pages, to be published in ApJ. Replaced for conformity with published version, including correction of minor typos and upda

Scientific paper

10.1086/509106

Gamma-Ray Bursts (GRBs) directed at Earth from within a few kpc may have damaged the biosphere, primarily though changes in atmospheric chemistry which admit greatly increased Solar UV. However, GRBs are highly variable in spectrum and duration. Recent observations indicate that short (~0.1 s) burst GRBs, which have harder spectra, may be sufficiently abundant at low redshift that they may offer an additional significant effect. A much longer timescale is associated with shock breakout luminosity observed in the soft X-ray (~10^3 s) and UV (~10^5 s) emission, and radioactive decay gamma-ray line radiation emitted during the light curve phase of supernovae (~10^7 s). Here we generalize our atmospheric computations to include a broad range of peak photon energies and investigate the effect of burst duration while holding total fluence and other parameters constant. The results can be used to estimate the probable impact of various kinds of ionizing events (such as short GRBs, X-ray flashes, supernovae) upon the terrestrial atmosphere. We find that the ultimate intensity of atmospheric effects varies only slightly with burst duration from 10^-1 s to 10^8 s. Therefore, the effect of many astrophysical events causing atmospheric ionization can be approximated without including time development. Detailed modeling requires specification of the season and latitude of the event. Harder photon spectra produce greater atmospheric effects for spectra with peaks up to about 20 MeV, because of greater penetration into the stratosphere.

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