Synthetic Observables

We intend to provide intensity maps at ALMA wavelengths, which have been calculated based on the provided numerical models with the listed radiative transfer tools.

Quiet Sun model co5bold_w04hdgr_seq1

  • Continuum brightness temperature images for 0.3mm, 1.0mm, 3.0mm and 9.0mm and different view angles from mu=1.0 (disk-centre) to mu=0.2 (close to the solar limb).
  • Sequence of 60 snapshots with 10s cadence.
  • File format: g'zipped tar file containing 20 files (for each combination of wavelength and view angle). Each file contains one data cube for the brightness temperature Tb [ nx, ny, nt] with nt=60, ny=140 and nx ranging from 140 at mu=1.0 to 28 for mu=0.2 (due to foreshortening).
  • File size: 45 MB
  • Reference: Wedemeyer-B. et al. (2007) containing a description and analysis of this data set.
  • Data link: http://astro-ursafs.uio.no/vol/ssalmon/co5bold_w04hdgr_seq1/w04hdgr_seq1_linfor3D_mmcont.tar.gz

Quiet Sun model co5bold_w11hdgr_seq1

  • Continuum brightness temperature images for 0.3mm, 1.0mm, 3.0mm, 6.0mm and 9.0mm for mu=1.0 (disk-centre)

Sequence with 4s cadence (on avg.)

Sequence with 1s cadence (on avg.)


Enhanced magnetic network Bifrost model en024048_hion

Published Jan. 31, 2016 5:10 PM - Last modified Mar. 11, 2016 2:51 PM