Annex 1
Assessment
of the interference from MES/MSS into
radio astronomy observations
Annex 2
Step 1
methodology: Calculation of separation distances by default between RAS sites and MESs
1 Introduction
2 General principles used
in the methodology
2.1
Monte
Carlo methodology
2.2
Protection
of radio astronomy observations
3 Presentation of the
methodology of calculation
4 Calculation of the
interfering power experienced during a sub-time step – modelling of
traffic
4.1
Monte
Carlo random trials
4.2
Calculation
of the initial number of calls: iniiter
4.3
Calculation
of the number of dropped calls: droppediter,it
4.4
Calculation
of the potential number of attempted calls: borniter,it
4.5
Calculation
of the effective number of new calls newiter,it,
and of the number of calls ncalliter,it
4.6
Assignment
of the (new) calls to the available traffic channels
4.7
Calculation
of the call termination time of the (new) calls
4.8
Calculation
of the other parameters linked to the (new) calls
4.9
Calculation
of rec_poweriter,it( f )
5 Determination of mean_poweriter( f )
Appendix 1 to
Annex 2 - List of variables
Annex 3 - Step 2 methodology: Calculation of
restriction zones around RAS sites for
sharing with MES
1 Introduction
2 Possible enhancements to
Step 1 methodology
Annex 4 - Information needed from MSS operators as
input for the calculation of separation
distances by default between an RAS site and an MES