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                            SCIENCE HARDWARE USED: 
                           
                              
                           
                                - Electronics unit BTN-ME
 
                                - Spare BTN
 
                                - BTN unit
 
                           
                          SUPPORT ITEMS: 
                           
                                - Platform with locks
 
                                - Cable set
 
                                - Cable holder
 
                                - Cable reel with cable.
 
                           
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                            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 EVA
 
                            - Measuring 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 models
 
                            - Clarify neutron source models in near-earth space
                              environment and evaluate their contribution in
                              a complete radiation dose received by cosmonauts
                              during EVA
 
                            - Obtain data on high-energy neutron fluxes with
                              energies up to 16 MeV coming from powerful solar
                              flares with regard to albedo radiation of the earth
 
                            - Build an operational model of neutron background
                              environment on the station
 
                            - Clarify existing solar activity models
 
                            - Obtain 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.
 
                             
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