scholarly journals TWINS energetic neutral atom observations of local-time-dependent ring current anisotropy

2012 ◽  
Vol 117 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
J. Goldstein ◽  
P. Valek ◽  
D. J. McComas ◽  
J. Redfern
1987 ◽  
Vol 14 (6) ◽  
pp. 652-655 ◽  
Author(s):  
Edmond C. Roelof

2002 ◽  
Vol 107 (A12) ◽  
pp. SMP 21-1-SMP 21-13 ◽  
Author(s):  
P. Cson Brandt ◽  
R. Demajistre ◽  
E. C. Roelof ◽  
S. Ohtani ◽  
D. G. Mitchell ◽  
...  

2005 ◽  
Vol 23 (8) ◽  
pp. 2825-2849 ◽  
Author(s):  
S. McKenna-Lawlor ◽  
L. Li ◽  
S. Barabash ◽  
K. Kudela ◽  
J. Balaz ◽  
...  

Abstract. The Earth’s ring current and how it responds to varying interplanetary conditions is described and an account provided of the production of Energetic Neutral Atoms (ENAs) in the geo-corona. Also, the potential to remotely monitor, on a global scale, the temporal and spatial evolution of magnetospheric plasma populations through analysing ENA images recorded during magnetic storms/substorms is indicated. A technical account of the Energetic NeUtral Atom Detector Unit NUADU aboard China’s TC-2 mission (measurement range 45–>158 keV) follows, together with an account of the scientific objectives of NUADU, both in stand-alone mode and in the context of multi-point imaging. Low altitude ENA emissions recorded by NUADU during south polar passages of TC-2 at the time of a moderate magnetic storm in September 2004, as well as bright ring current emissions recorded in November 2004 during a major geomagnetic storm, are presented and discussed in the context of various, accompanying, terrestrial disturbances. Also, ENA observations of the November 2004 ring current imaged simultaneously by TC-2/NUADU and by IMAGE/ HENA (viewing, respectively, from the Northern and Southern Hemispheres), are compared.


2006 ◽  
Vol 2 (S239) ◽  
pp. 314-316 ◽  
Author(s):  
Achim Weiss ◽  
Martin Flaskamp

AbstractThe non-local, time-dependent convection theory of Kuhfuß (1986) in both its one- and three-equation form has been implemented in the Garching stellar evolution code. We present details of the implementation and the difficulties encountered. Specific test cases have been calculated, among them a 5 M⊙ star and the Sun. These cases point out deficits of the theory. In particular, the assumption of an isotropic velocity field leads to too extensive overshooting and has to be modified at convective boundaries. Some encouraging aspects are indicated as well.


2021 ◽  
Vol 254 (2) ◽  
pp. 32
Author(s):  
Bishwas L. Shrestha ◽  
Eric J. Zirnstein ◽  
Jacob Heerikhuisen ◽  
Gary P. Zank

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