scholarly journals A statistical study of the low‐altitude ionospheric magnetic fields over the north pole of Venus

2015 ◽  
Vol 120 (8) ◽  
pp. 6218-6229 ◽  
Author(s):  
T. L. Zhang ◽  
W. Baumjohann ◽  
C. T. Russell ◽  
M. N. Villarreal ◽  
J. G. Luhmann ◽  
...  
2002 ◽  
Vol 20 (2) ◽  
pp. 275-280 ◽  
Author(s):  
T. K. Yeoman ◽  
P. G. Hanlon ◽  
K. A. McWilliams

Abstract. The large-scale and continuous monitoring of the ionospheric cusp region offered by HF radars has been exploited in order to examine the statistical location and motion of the equatorward edge of the HF radar cusp as a function of the upstream IMF BZ component. Although a considerable scatter is seen, both parameters have a clear influence from the north-south component of the IMF. Excellent agreement is achieved with previous observations from low altitude spacecraft data. The HF radar cusp region is seen to migrate equatorward at a rate of 0.02° min-1 nT-1 under IMF BZ south conditions, but remains static for IMF BZ north. The motion of the cusp implies an addition of magnetic flux of ~ 2 × 104 Wbs-1 nT-1 under IMF BZ south conditions, equivalent to a reconnection voltage of 20 kV nT-1, which is consistent with previous estimates from case studies on both the dayside and nightside regions.Key words. Ionosphere (auroral ionosphere) – Magnetospheric physics (magnetosphere-ionosphere interaction; solar wind magnetosphere interactions)


2017 ◽  
Vol 36 (1) ◽  
pp. 64-72 ◽  
Author(s):  
Lanyu Li ◽  
Changqing Ke ◽  
Hongjie Xie ◽  
Ruibo Lei ◽  
Anqi Tao
Keyword(s):  
Sea Ice ◽  

JAMA ◽  
2009 ◽  
Vol 302 (10) ◽  
pp. 1121
Keyword(s):  

1823 ◽  
Vol 9 (2) ◽  
pp. 353-364 ◽  
Author(s):  
William Scoresby

The value of the Chronometer for finding the Longitude at Sea, being, by the experience of many years trial, fully established, I am induced to offer to the Royal Society some remarks on the change of rate observed in this instrument, when on ship-board. This change of rate, that had usually been supposed to arise from the motion of the ship, has recently heen attributed, by Mr Fisher, who accompanied Captain Buchan in his Voyage towards the North Pole in the year 1818, ‘to the magnetic action exerted by the iron in the ship upon ‘the inner rim of the Chronometer's balance, which is composed of steel.’ I apprehend, however, that it will be very easy to show, that although the alteration of rate may be, and most probably is, owing to magnetism, yet the magnetic action of the iron in the ship, excepting in cases where chronometers are placed in immediate contact with large masses of iron, can contribute but in a very small degree to the error in question.


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