Online Data

On this page, I'm collecting various pieces of computer codes and observational data for public distribution. In most cases, each item is linked to a published paper, and the list below is in approximate inverse chronological order.

 

Cranmer, S. R., van Ballegooijen, A. A., and Edgar, R. J. 2007, "Self-consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence," Ap. J. Suppl., 171, 520. [see also arXiv preprint: astro-ph/0703333]

Tabulated plasma properties for three of the models included in this paper (i.e., polar coronal hole, quiescent equatorial streamer, and representative "active region slow wind") are available here. (See the "readme" file for details about the file format.)

Owocki, S. P., and Cranmer, S. R. 2002, "The Link between Radiation-Driven Winds and Pulsation in Massive Stars," Radial and Nonradial Pulsations as Probes of Stellar Physics, IAU Colloquium 185, 26-31 July 2001, Leuven, Belgium, p. 512.

For reasons of space, only a subset of the plots generated for the BW Vul simulations are included in the paper. Additional plots (in postscript format) are available here.

Cranmer, S. R. 2000, "Ion Cyclotron Wave Dissipation in the Solar Corona: The Summed Effect of More than 2000 Ion Species," Ap. J., 532, 1197.

The Fortran code used to compute the ionization equilibrium of ions from hydrogen to uranium, along with sample output files, is publically available as a gzipped UNIX tar file (112 K). The uncompressed files are also available individually:

Cranmer, S. R., Smith, M. A., and Robinson, R. D. 2000, "A Multiwavelength Campaign on gamma Cassiopeiae. IV. The Case for Illuminated Disk-Enhanced Wind Streams," Ap. J., 537, 433.

Some of the Hubble Space Telescope data that was used in this paper (and in the preceding papers in this series) are archived by the Multi-Mission Archive at Space Telescope (MAST) at this URL.

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