Statistical Anisotropic Gaussian Simulations of the CMB Temperature
  Field
  Although theoretically expected to be Statistically Isotropic (SI), the
observed Cosmic Microwave Background (CMB) temperature \& polarization field
would exhibit SI violation due to various inevitable effects like weak lensing,
Doppler boost and practical limitations of observations like non-circular beam,
masking etc. However, presence of any SI violation beyond these effects may
lead to a discovery of inherent cosmic SI violation in the CMB temperature \&
polarization field. Recently, Planck presented strong evidence of SI violation
as a dipolar power asymmetry of the CMB temperature field in two hemispheres.
Statistical studies of SI violation effect require non-SI (nSI) Gaussian
realizations of CMB temperature field. The nSI Gaussian temperature field leads
to non-zero off-diagonal terms in the Spherical Harmonics (SH) space covariance
matrix encoded in the coefficients of the Bipolar Spherical Harmonics (BipoSH)
representation. We discuss an effective numerical algorithm, Code for
Non-Isotropic Gaussian Sky (CoNIGS) to generate nSI realizations of Gaussian
CMB temperature field of Planck like resolution with specific cases of SI
violation. Realizations of nSI CMB temperature field are obtained for non-zero
quadrupolar $(L=2)$ BipoSH measurements by WMAP, dipolar asymmetry (resembles
$L=1$ BipoSH coefficients) with a \emph{scale dependent} modulation field as
measured by Planck and for Doppler boosted CMB temperature field which also
leads to $L=1$ BipoSH spectra. Our method, CoNIGS can incorporate any kind of
SI violation and can produce nSI realizations efficiently.
