Interplanetary crew dose estimates for worst case solar particle events based on historical data for the Carrington flare of 1859.
Over the past two decades, hypothetical models of "worst-case" solar particle event (SPE) spectra have been proposed in order to place an upper bound on radiation doses to critical body organs of interplanetary crews on deep space missions. These event spectra are usually formulated using hypothetical extrapolations of space measurements for previous large events. Here we take a different approach. Recently reported analyses of ice core samples indicate that the Carrington flare of 1859 is the largest event observed in the past 500 years. These ice core data yield estimates of the proton fluence for energies greater than 30 MeV, but provide no other spectrum information. Assuming that the proton energy distribution for such an event is similar to that measured for other recent, large events, interplanetary crew doses are estimated for these hypothetical worst case SPE spectra. These estimated doses are life threatening unless substantial shielding is provided.
Stephens
Daniel L
DL
Department of Nuclear Engineering, The University of Tennessee, Knoxville, TN 37996-2300, USA.
Townsend
Lawrence W
LW
Hoff
Jennifer L
JL
D000535:Aluminum; D001110:Arctic Regions; D018480:Astronauts; D001822:Body Burden; D005118:Extraterrestrial Environment; D005123:Eye / Q000528:radiation effects; D006413:Hematopoietic System / Q000528:radiation effects; D006801:Humans; D046448:Ice Cover; D019047:Phantoms, Imaging; D011522:Protons; D011829:Radiation Dosage; D011835:Radiation Protection; D012062:Relative Biological Effectiveness; D018570:Risk Assessment; D012867:Skin / Q000528:radiation effects; D019445:Solar Activity; D013026:Space Flight
D011522:Protons; D000535:Aluminum