... A synoptic map of photosphere magnetic fields is given on the lower panel from observations at Stanford Station, USA (from Solar Geophysical Data, Carrington rotation no. ...
... solar system: the satellites of the planets; the large number of asteroids (small ... the boundary between the inner solar system and the outer solar system. by position ... Museum Community Solar System , the world's largest model of the solar system ...
... Owing to the interplay between solar wind outflow and the Sun's rotation, IMF field lines near Earth tend to lie close to the (x,y) plane, with B in the (x,-y) and (-x,y) quadrants and making an angle of about 450 with the x-axis, as predicted by Parker. ...
... The sense in which all planets in our solar system (and the Sun) rotate is presumably the same as that of the cloud from which the solar system condensed. ...
... The sense in which all planets in our solar system (and the Sun) rotate is presumably the same as that of the cloud from which the solar system condensed. ...
... Owing to the interplay between solar wind outflow and the Sun's rotation, IMF field lines near Earth tend to lie close to the (x,y) plane, with B in the (x,-y) and (-x,y) quadrants and making an angle of about 450 with the x-axis, as predicted by Parker. ...
... rotates by a rather small angle, 15 degrees, and if "open" field lines in the lobes ... solar wind would need 2-3 days to cover the corresponding distance (equal to about ... rotation axis, which itself is inclined by 23.5 degrees to the direction ...