We present the key components of a 3-D code designed for simulating the hydrodynamics and magnetohydrodynamics of stellar atmospheres and envelopes. Some particular properties of the code are: (1) the ability to handle strong stratification (extensive simulations with bottom/top pressure ratios of 3
โฆ LIBER โฆ
Solar surface magnetoconvection simulations: A brief review of solar dermatology
โ Scribed by Robert Cameron
- Publisher
- Science in China Press (SCP)
- Year
- 2009
- Tongue
- English
- Weight
- 510 KB
- Volume
- 52
- Category
- Article
- ISSN
- 1672-1799
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In the 0879s\ advances in the passivation of both cell surfaces led to the \_rst crystalline silicon solar cells with conversion ef\_ciencies above 19)[ With today|s industry trend towards thinner wafers and higher cell ef\_ciency\ the passivation of the front and rear surfaces is now also becoming