Abstract
The age-specific indicators of the functions of the cardiovascular system and its responses to the lower body negative pressure (LBNP) test were studied in career cosmonauts for the first time. The results of 174 LBNP tests implemented within the standard medical monitoring program on board the “Mir” orbital station (OS “Mir”), using a Gamma-01 device, and aboard the International Space Station (ISS), using the Gamma-1M complex, were subjected to comparative analysis. In total, 38 cosmonauts from 25 long-duration space missions on board the “Mir” OS and ISS, who were examined in their pre-flight state and during in-flight periods, beginning, typically, on flight day (FD) 120, were subdivided into two age groups: 30- to 39-year-olds (their mean age was 36 ± 0.7 years; 39% of the total number of subjects) and 40- to 55-year olds (their mean age was 46 ± 0.8 years; 61% of the total number of subjects). We have revealed age-specific indicators for the hemodynamic status recorded at each stage of the investigation: at rest in a preflight state; responses of the indicators to the effects of microgravity; the relative dynamics of the indicators due to a simulated orthostatic posture, which was unidirectional but substantially different at the pre-and in-flight stages. For purposes of medical control, our results have shown that we need to establish age-specific references in our methodical approaches to the analysis and interpretation of the data received from monitoring cosmonauts’ health in their preflight state and during the entire mission and, which is particularly important in practical terms, when evaluating the LBNP test intolerance at different flight stages.
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Original Russian Text © V.F. Turchaninova, I.V. Alferova, V.V. Krivolapov, 2010, published in Aviakosmicheskaya i Ekologicheskaya Meditsina, 2010, Vol. 44, No. 1, pp. 20–15.
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Turchaninova, V.F., Alferova, I.V. & Krivolapov, V.V. Some aspects of the comparative analysis of hemodynamic responses to LBNP tests in cosmonauts of different age groups. Hum Physiol 38, 721–726 (2012). https://doi.org/10.1134/S0362119712070249
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DOI: https://doi.org/10.1134/S0362119712070249