scholarly journals Palaeosecular variation and the current loop model of the geomagnetic field

1982 ◽  
Vol 71 (1) ◽  
pp. 269-273 ◽  
Author(s):  
M. Roy ◽  
J. - J. Wagner
2020 ◽  
Author(s):  
Zhaojin Rong ◽  
Yong Wei ◽  
Masatoshi Yamauchi ◽  
Wenyao Xu ◽  
Dali Kong ◽  
...  

2020 ◽  
Author(s):  
Zhaojin Rong ◽  
Yong Wei ◽  
Wenyao Xu ◽  
Dali Kong ◽  
Jun Cui ◽  
...  

<p>A quick and effective technique is developed to diagnose the geomagnetic dipole field based on an unstrained single circular current loop model. In comparsion with previous studies, this technique is able to separate and solve the loop parameters successively. With this technique, one can search the optimum full loop parameters quickly, including the location of loop center, the loop orientation, the loop radius, and the electric current carried by the loop, which can roughly indicate the locations, sizes, orientations of the interior current sources. The technique tests and applications demonstrate that this technique is effective and applicable. This technique could be applied widely in the fields of geomagnetism, planetary magnetism and palaeomagnetism. The further applications and constrains are discussed and cautioned.</p>


Energies ◽  
2020 ◽  
Vol 13 (19) ◽  
pp. 5218
Author(s):  
Xiaoyong Zhang ◽  
Jiaxuan Lei ◽  
Heng Li ◽  
Hongtao Liao ◽  
Jun Peng

Ultracapacitors have recently received great attention for energy storage due to their small pollution, high power density, and long lifetime. In many applications, ultracapacitors need to be charged with a high current, where a multi-module charging system is typically adopted. Although the classical decentralized control method can control the charging process of ultracapacitors, there exists a problem that the charging current may be imbalanced among charging modules. In this paper, a cooperative cascade charging method is proposed for the multi-module charging system to reduce the current imbalance among charging modules. First, the state-space averaging method and graph theory are used to model the multiple-module charging system. Second, an effective cooperative cascade control is proposed, where the outer voltage loop stabilizes the output voltage to the desired voltage and the inner current loop guarantees the current of each charger to follow the target current. The block diagram is used to establish the closed-loop model of the charging system. In order to evaluate the proposed charging method, a laboratory prototype was established. Compared with the classical decentralized method, this method can effectively suppress the current imbalance, which is proved by simulation and experimental results.


1981 ◽  
Vol 59 (1) ◽  
pp. 1-14 ◽  
Author(s):  
D. G. Lahoz ◽  
G. M. Graham

The "current loop" model for a magnetic dipole is thoroughly examined in connection with the electromagnetic force density in material media. An updated and theoretically consistent expression for that force density is presented which differs from the Livens' and Page–Adams' proposals in minor details. The notation in our updated formula gives precise information about the volume elements within the material medium which are the seats where the different force density terms are localized. The corresponding tensor theory is also developed and, using the concept of localized Poynting vector, a new interpretation of the "Lorentz diffraction" phenomenology is suggested which would seem to explain the observed small deviations from the mean deflection.


2009 ◽  
Vol 23 (24) ◽  
pp. 4977-4985 ◽  
Author(s):  
M. SAGLAM ◽  
G. SAHIN

We show that the electron–positron annihilation process ending with the creation of two gamma photons (with right- and left-hand circular helicity) can be explained in terms of the current loop model. We first show that both electron and positron (which are spin 1/2 particles) carry an intrinsic flux quantum of ±Φ0/2 even in the absence of an external magnetic field. By using the conservation of the magnetic flux quanta for collisions, we then argue that photon also carries a magnetic flux quantum of ±Φ0 = ±(hc/e) with itself along the propagation direction, where the (+) sign corresponds to the right-hand helicity and (-) one to the left-hand one.


2015 ◽  
Vol 33 (4) ◽  
pp. 505-517 ◽  
Author(s):  
A. V. Nikolaev ◽  
V. A. Sergeev ◽  
N. A. Tsyganenko ◽  
M. V. Kubyshkina ◽  
H. Opgenoorth ◽  
...  

Abstract. Substorm current wedge (SCW) formation is associated with global magnetic field reconfiguration during substorm expansion. We combine a two-loop model SCW (SCW2L) with a background magnetic field model to investigate distortion of the ionospheric footpoint pattern in response to changes of different SCW2L parameters. The SCW-related plasma sheet footprint shift results in formation of a pattern resembling an auroral bulge, the poleward expansion of which is controlled primarily by the total current in the region 1 sense current loop (I1). The magnitude of the footprint latitudinal shift may reach ∼ 10° corrected geomagnetic latitude (CGLat) during strong substorms (I1= 2 MA). A strong helical magnetic field around the field-aligned current generates a surge-like region with embedded spiral structures, associated with a westward traveling surge (WTS) at the western end of the SCW. The helical field may also contribute to rotation of the ionospheric projection of narrow plasma streams (auroral streamers). Other parameters, including the total current in the second (region 2 sense) loop, were found to be of secondary importance. Analyzing two consecutive dipolarizations on 17 March 2010, we used magnetic variation data obtained from a dense midlatitude ground network and several magnetospheric spacecraft, as well as the adaptive AM03 model, to specify SCW2L parameters, which allowed us to predict the magnitude of poleward auroral expansion. Auroral observations made during the two substorm activations demonstrate that the SCW2L combined with the AM03 model nicely describes the azimuthal progression and the observed magnitude of the auroral expansion. This finding indicates that the SCW-related distortions are responsible for much of the observed global development of bright auroras.


2013 ◽  
Vol 771 (2) ◽  
pp. 125 ◽  
Author(s):  
Oscar Olmedo ◽  
Jie Zhang ◽  
Valbona Kunkel
Keyword(s):  

1996 ◽  
Vol 76 (20) ◽  
pp. 3818-3821 ◽  
Author(s):  
Raymond E. Goldstein ◽  
David P. Jackson ◽  
Alan T. Dorsey

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