|  SCIENCE HARDWARE USED: 
                           
                              
                                Electronics unit BTN-MESpare BTNBTN unit SUPPORT ITEMS: 
                           
                                Platform with locksCable setCable holderCable reel with cable. |  |  PURPOSE: 
					    Building a physical model for generation of charged and neutral particles during solar flares.Developing a physical model of neutron albedo of the earth atmosphere with regard to helio- and geophysical environment, measurement point longitude and altitude effects, time of the day and lighting conditions, atmosphere conditions.Developing a physical model of neutron background in the vicinity of the ISS in different flight conditions, as well as recording space gamma bursts.  OBJECTIVE: 
                            Mounting the onboard neutron telescope, cable
                              routing inside and outside the pressurized compartment
                              and conducting photo (video) imagery of their location
                              during EVAMeasuring direct and scattered fluxes of high-energy
                              neutrons of solar flares with energies from 10
                              to 15 MeV.Measuring neutrons resulted from nuclear reactions
                              induced by space rays in the earth’s upper atmosphere
                              in the range of thermal (0.001 – 0.1 eV), epithermal
                              (0.1 – 1.0 eV), resonance (1 – 0.3 eV) and fast
                              (0.3 – 15 MeV) energies.Measuring gamma radiation in energy ranges between
                          30 keV to 100 MeV.  EXPECTED RESULTS: Experimental spectrometric investigations of neutron
                          fields on the ISS will allow to 
                            Clarify the on-orbit radiation environment modelsClarify neutron source models in near-earth space
                              environment and evaluate their contribution in
                              a complete radiation dose received by cosmonauts
                              during EVAObtain data on high-energy neutron fluxes with
                              energies up to 16 MeV coming from powerful solar
                              flares with regard to albedo radiation of the earthBuild an operational model of neutron background
                              environment on the stationClarify existing solar activity modelsObtain data on fluxes of rigid electromagnetic
                              space rays component   EXPERIMENT RESULTS: 
                                Measurement data on spatial and time distributions
                                  of radiation characteristics of space ionizing
                                  radiation (neutron and gamma components) outside
                                  the Service Module of the ISS RS;Correlation data on radiation environment
                                  parameters outside the Service Module of the
                                  ISS RS obtained through calculation with the
                                  results of measurements made by science hardware
                                  BTN-M1 and results of other Russian and international
                                  experiments;Measurement data on solar flare parameters
                                  in neutron and gamma range. |