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CO[5]BOLD

COnservative COde for the COmputation of COmpressible COnvection in a BOx of L Dimensions with l=2,3
Co5bold-example.jpg Co5bold-example.jpg

One of the models used to compute synthetic solar spectra. The simulations were created at the AIP using the radiative hydrodynamics code CO5BOLD. Dark lanes are the intergranular regions of cooler temperature that harbor magnetic field structures.

Credit: AIP

Contact at AIP

Dr. Matthias Steffen

Phone: +49 331 7499 371
msteffennothing@aip.de
[Project Website]

Code record at Astrophysics Source Code Library: http://ascl.net/1011.014

Project website: http://www.lsw.uni-heidelberg.de/co5bold/workshop/cws_intro.html

Partners:

Landessternwarte Heidelberg

Involved AIP sections and groups:

Stellar Physics and Exoplanets
Last update: 9. December 2020