stones that are of smaller size at greater distance from the mountains, and where the streams flow more slowly; stones that appear pulverised in the shape of sand where the streams begin to stagnate near their mouths and near the sea - if you consider all this, you could scarcely help th...
Voyager I, II 1979 Galileo 1995–2003 Galilean moons Galileo 1995–2003 • Detection of Ganymede's dynamo-generated magnetic field • Detection of induced magnetic fields in global subsurface oceans of Europa, Ganymede, and Callisto Saturn Pioneer 11 1979 • Detection of dynamo-generated magneti...
Detailed study of these and Voyager 1 outbound data show that the magnetic structure near and within the current sheet was variable with time and distance from Jupiter, but generally corresponded to one of the following four types: (1) simple rotation of field across the sheet, with either a...
Surprisingly, from such a distance, the mission operators still can communicate with Voyager 2 as it enters this new phase of its journey. However, the information – moving at the speed of light – takes about 16.5 hours to travel from the spacecraft to Earth. On the other hand, comparati...
At the bottom of the figure the first two digits of the year and the doy, the cylindrical radial distance of Cassini, the vertical distance from the magnetic equator (offset by 0.04 RS from the rotational equator), and Cassini's local time are shown. [9] Two angles are also plotted on...
[3] have demonstrated that the solar wind temperature measured by the Voyager spacecraft remains nearly constant from 2 AU to 10 AU, decreasing with heliocentric distance in a manner inconsistent with both adiabatic and isothermal processes. A widely accepted explanation for this phenomenon is the ...