Nature, Količina 420Sir Norman Lockyer Macmillan Journals Limited, 2002 |
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Stran
... magnetic fields and convection near the Sun's surface12 . The dark central umbra is surrounded by a filamentary penum- bra , whose complicated fine structure has only recently been revealed by high - resolution observations - 14 . The ...
... magnetic fields and convection near the Sun's surface12 . The dark central umbra is surrounded by a filamentary penum- bra , whose complicated fine structure has only recently been revealed by high - resolution observations - 14 . The ...
Stran
... magnetic field B = ( 0 , B ,, 0 ) , as shown in Fig . 2b , and adjust the density of the layer so that the pressure remains continuous , although the magnetic slab is nearly evacuated and hence very buoyant . b t = 0 t = 14.6 Z = 0 z ...
... magnetic field B = ( 0 , B ,, 0 ) , as shown in Fig . 2b , and adjust the density of the layer so that the pressure remains continuous , although the magnetic slab is nearly evacuated and hence very buoyant . b t = 0 t = 14.6 Z = 0 z ...
Stran
... magnetic diffusion is the main transport mechanism . Heavy lines denote the flux distributions at the beginning and end of each phase . At first magnetic flux moves upwards , owing to magnetic buoyancy , and some leaks out through the ...
... magnetic diffusion is the main transport mechanism . Heavy lines denote the flux distributions at the beginning and end of each phase . At first magnetic flux moves upwards , owing to magnetic buoyancy , and some leaks out through the ...
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