The features of radiation dose variations onboard ISS and Mir space station: comparative study.

The dynamics of the ISS-measured radiation dose variations since August 2000 is studied. Use is made of the data obtained with the R-16 instrument, which consists of two ionization chambers behind different shielding thicknesses. The doses recorded during solar energetic particle (SEP) events are compared with the data obtained also by R-16 on Mir space station. The SEP events in the solar maximum of the current cycle make a much smaller contribution to the radiation dose compared with the October 1989 event recorded on Mir space station. In the latter event, the proton intensity was peaking during a strong magnetic storm. The storm-time effect of solar proton geomagnetic cutoff decreases on dose variations is estimated. The dose variations on Mir space stations due to formation of a new radiation belt of high-energy protons and electrons during a sudden commencement of March 24, 1991 storm are also studied. It was for the first time throughout the ISS and Mir dose measurement period that the counting rates recorded by both R-16 channels on ISS in 2001-2002 were nearly the same during some time intervals. This effect may arise from the decreases of relativistic electron fluxes in the outer radiation belt.

Radiation dose measurements aboard the Mir using the R-16 instrument.

NASA: Data from the R-16 radiation dosimeter mounted to the outside of the Mir space station are analyzed to determine the radiation environment and absorbed radiation dose inside Mir during the 22nd solar cycle. The outcome of the analysis demonstrated that data could be collected over a long period, dynamics of the daily mean absorbed doses correlated well with parameters of solar activity, seasonal variations of absorbed doses during the solar cycle were clearly observed, during periods of unfavorable conditions the absorbed dose rate within the living modules can reach up to 30 mrad/min for more than 10 minutes, and overall, the radiation environment inside the space station was low.^ieng

Variations of the radiation dose onboard Mir station.

Dose variations, associated with the 11-year solar activity cycle, seasonal variations of particle fluxes in the Earth's radiation belts at the station orbit, and solar proton events are studied, using prolonged measurements of radiation doses inside orbital station Mir. Daily averages of radiation doses during the declining phase of the 22nd solar cycle and during transition to the 23rd solar activity cycle reached very large values for astronauts and significantly exceed the values calculated according to existing models.