<?xml version="1.0" encoding="UTF-8" standalone="no"?>
<Scenery>
  <Metric kind = "KerrBL">
    <Mass unit="sunmass">4.31e6</Mass>
    <Spin>0.9</Spin>
  </Metric>

  <Screen>
    <Distance unit="kpc"> 8.33 </Distance>
    Time of start of ray tracing
    <Time unit="yr"> 100e3 </Time>
    <FieldOfView unit="µas"> 300 </FieldOfView>
    This inclination is 180° minus the standard disk
    inclination (angle between spin vector and line of sight)
    <Inclination unit="°"> 95 </Inclination>
    <PALN> 3.1415  </PALN> 
    <Argument> -1.5708 </Argument>
    <Resolution>30</Resolution>
    Compute a spectrum with 50 frequencies from 10^10 Hz to 10^18 Hz
    <Spectrometer kind="freqlog" nsamples="5">10. 18.</Spectrometer>
  </Screen>

  <Quantities>Spectrum</Quantities>

  <Astrobj kind = "PolishDoughnut">

    Compute Bremsstrahlung spectrum?
    <!--<Bremsstrahlung/>-->
    
    Compute non-thermal synchrotron spectrum
    with a fraction delta of non-thermal electrons
    and a power-law exponent?
    <!--<NonThermalDeltaExpo>0.01 3.</NonThermalDeltaExpo>-->

    The default is to compute only the thermal synchrotron spectrum.
    
    Compute synchrotron averaged over angle between
    Bfield and direciton of emission?
    <AngleAveraged/>
    
    Constant angular momentum -u_phi / u_t, and inner radius
    <AngMomRinner> 3.2 4.2 </AngMomRinner>

    Typical SgrA* enthalpy hc = 9000 cgs; ne [cm^{-3}] ~ 700 * hc [cgs]
    <CentralEnthalpyPerUnitVolume unit="erg/cm3"> 
      9000
    </CentralEnthalpyPerUnitVolume>

    Typical SgrA* central temperature: 5e10K
    <CentralTemperature>5.3e10</CentralTemperature> 
    
    beta = p_gas / p_mag
    <Beta>10</Beta>
    
    <OpticallyThin/>
    
    RMax: caution, make sure the torus is smaller than that!
    <RMax>100.</RMax>
    
  </Astrobj>

  Computation stops for time less than following value
  to prevent infinite integration
  <MinimumTime> -1e10 </MinimumTime>
  
  Do we want to use multi-threading?
  <NThreads> 1 </NThreads>

</Scenery>

