Cosmic rays, i.e., protons and atomic nuclei with high energy from astrophysical origin, are the dominant producers of enhanced radiation doses at aircraft altitudes. While the assessment of dose rates produced by the permanent galactic cosmic ray (GCR) component is well-established and operational, the evaluation of the sporadic solar cosmic ray (SCR) contribution during so-called Ground-Level Enhancements (GLEs) is an issue of current research. Several institutions developed codes for the assessment of solar radiation doses at flight altitudes. EURADOS Working Group WG11 conducted a study comparing route doses and dose rates at flight altitudes during two selected GLEs as calculated by means of nine computer codes. For GLE42 (29 September 1989) pre-defined solar particle characteristics were provided to the participants of the study. In contrast, for GLE69 (20 January 2005) the participants were asked to define the proton characteristics on their own based on published information made available to them.
In the study it was found that GCR route doses show a standard deviation from the median consistent with the results published in the earlier EURADOS report on GCR exposure. For GLE42 a standard deviation from the median of about 30% is obtained for the SCR route doses, while for GLE69 the standard deviation from the respective median amounts to 50%. The lowest and the highest SCR route doses obtained by the different codes for a given flight may differ by up to a factor of 10. One of the main reasons for the differences in the computed results is found to be the unequal identification and handling of the GLE characteristics, such as energy spectrum and directional distribution. Therefore, we strongly suggest developing a traceable method to identify and handle the solar particle characteristics during GLEs. Furthermore, we see an urgent need to validate codes used for dose assessment of radiation exposure due to solar particle events by in-flight measurements.
Veronika Olšovcová graduated in Dosimetry at the Czech Technical University in Prague. After a decade at the Czech Metrology Institute, she joined in 2010 the Institute of Physics of the Czech Academy of Sciences to work on the development of a...
Seibersdorf Laboratories, Tech Campus Seibersdorf, Austria
DI Dr. Peter Beck is Head of Radiation Protection Dosimetry at Seibersdorf Laboratories in Austria. Since the 1990s, he has supported to establish the field of flight dosimetry in Austria and in Europe and has played a major role in shaping it....
University of Bern - Physikalisches Institut / HFSJG
Erwin Flückiger, born in 1943, is a retired physics professor specializing in cosmic rays. From 1997 to 2009 he headed the cosmic ray research group at the Physikalisches Institut of the University of Bern, Switzerland. For ten years he also acted...
Dr. Rolf Bütikofer, born 1959, studied physics at the University of Bern/Switzerland. Dr. phil. nat. in the field of cosmic radiation. Since 1993 staff member at the Institute of Physics, University of Bern, in the field of cosmic rays. Research...
Paris Observatory, LESIA and Nancay Radio Observatory, France
Dr. Karl-Ludwig Klein is researcher in solar physics with special interest in solar activity and solar energetic particles. He is the scientific head of solar observing services at Paris Observatory and especially of cosmic ray monitoring with the...
Seibersdorf Laboratories, Tech Campus Seibersdorf, Austria
DI Dr. Marcin Latocha is a physicist with strong IT affinity working in the field of radiation protection dosimetry at Seibersdorf Laboratories in Austria, where he currently heads the aircrew dosimetry service. During his 20 years of experience,...
PhD in nuclear physics, speciality instrumentation and measurements. Current position: Deputy Director of Radiological Protection and Health at the Institute for Radiological Protection and Nuclear Safety (IRSN, France). Background in radiation...