Study of Cosmic Rays on ISS Russian Segment
     Experiment BTN-Neutron
	 
	    Objective:
              
					    - 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.
 Tasks:
               
                            - 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.
 
 
           			             Science Hardware Used:
                          
                                - Electronics unit BTN-ME;
- Spare BTN;
- BTN unit.
Support Items:
 
                          
                                - Platform with locks;
- Cable set;
- Cable holder;
- Cable reel with cable.
 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.