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pro vyhledávání: '"Hulburt, N. E."'
We present results on modeling solar pores and sunspots using 2D axisymmetric magneto-hydrodynamic (MHD) simulations. These models are helpful for understanding the mechanisms of magnetic field concentration in sunspots, and the large-scale flow patt
Externí odkaz:
http://arxiv.org/abs/1006.4156
Publikováno v:
NASA Astrophysics Data System
We present results on modeling solar pores and sunspots using 2D axisymmetric magneto-hydrodynamic (MHD) simulations. These models are helpful for understanding the mechanisms of magnetic field concentration in sunspots, and the large-scale flow patt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1526707fbf0c5fafea19cdb5600711c7