منابع مشابه
Saturn's Magnetic Field and Magnetosphere.
The Pioneer Saturn vector helium magnetometer has detected a bow shock and magnetopause at Saturn and has provided an accurate characterization of the planetary field. The equatorial surface field is 0.20 gauss, a factor of 3 to 5 times smaller than anticipated on the basis of attempted scalings from Earth and Jupiter. The tilt angle between the magnetic dipole axis and Saturn's rotation axis i...
متن کاملCassini observations of planetary-period magnetic field oscillations in Saturn’s magnetosphere: Doppler shifts and phase motion
[1] Cassini magnetic field observations show that few-nT oscillations near the planetary rotation period, first observed in Pioneer-11 and Voyager-1 and -2 fly-by data, are essentially ubiquitous in Saturn’s magnetosphere, though their character differs between the quasi-dipolar ring current region and the dawn tail. Examination of data from the ringcurrent region shows, however, that the obser...
متن کاملThe bottom magnetic field and magnetosphere evolution of neutron star in low mass X - ray binary
The accretion induced neutron star magnetic field evolution is studied through considering the accretion flow to drag the field lines aside and dilute the polar field strength, and as a result the equatorial field strength increases, which is buried inside the crust on account of the accretion induced global compression of star crust. The main conclusions of model are as follows: (i) the polar ...
متن کاملBottom magnetic field and magnetosphere evolution of neutron star in low mass X-ray binary
The accretion induced neutron star magnetic field evolution is studied through considering the accretion flow to drag the field lines aside and dilute the polar field strength, and as a result the equatorial field strength increases and is buried inside the crust. The main conclusions of model are as follows: (i) the polar field decays with increasing the accreted mass; (ii) The bottom magnetic...
متن کاملX-ray neutron star magnetic field and magnetosphere evolution in low mass X-ray binary
The accretion induced neutron star magnetic field evolution is studied through considering the accretion flow to drag the field lines aside and dilute the polar field strength, and as a result the equatorial field strength increases and is buried inside the crust. The main conclusions of model are as follows: (i) the polar field decays with increasing the accreted mass; (ii) The bottom magnetic...
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ژورنال
عنوان ژورنال: Science
سال: 1980
ISSN: 0036-8075,1095-9203
DOI: 10.1126/science.207.4429.407