Resolving the Ambiguity of a Magnetic Cloud’s Orientation Caused by Minimum Variance Analysis Comparing it with a Force-Free Model

Solar Physics ◽  
2021 ◽  
Vol 296 (12) ◽  
Author(s):  
Rosemeire Aparecida Rosa Oliveira ◽  
Marcos William da Silva Oliveira ◽  
Arian Ojeda-González ◽  
Valdir Gil Pillat ◽  
Ezequiel Echer ◽  
...  
Solar Physics ◽  
2020 ◽  
Vol 295 (3) ◽  
Author(s):  
Rosemeire Aparecida Rosa Oliveira ◽  
Marcos William da Silva Oliveira ◽  
Arian Ojeda-González ◽  
Victor De La Luz

1996 ◽  
Vol 101 (A3) ◽  
pp. 4961-4965 ◽  
Author(s):  
U. Motschmann ◽  
T. I. Woodward ◽  
K. H. Glassmeier ◽  
D. J. Southwood ◽  
J. L. Pinçon

Author(s):  
Kerry E. Back

The mean‐variance frontier is characterized with and without a risk‐free asset. The global minimum variance portfolio and tangency portfolio are defined, and two‐fund spanning is explained. The frontier is characterized in terms of the return defined from the SDF that is in the span of the assets. This is related to the Hansen‐Jagannathan bound. There is an SDF that is an affine function of a return if and only if the return is on the mean‐variance frontier. Separating distributions are defined and shown to imply two‐fund separation and mean‐variance efficiency of the market portfolio.


2013 ◽  
Vol 31 (5) ◽  
pp. 817-833 ◽  
Author(s):  
M. Volwerk ◽  
N. André ◽  
C. S. Arridge ◽  
C. M. Jackman ◽  
X. Jia ◽  
...  

Abstract. A comparison of magnetotail flapping (the up-and-down wavy motion) between the Earth and the two giant planets Jupiter and Saturn has been performed through investigation of the current sheet normal of the magnetotail. Magnetotail flapping is commonly observed in the Earth's magnetotail. Due to single spacecraft missions at the giant planets, the normal is determined through minimum variance analysis of magnetometer data during multiple intervals when the spacecraft crossed through the current sheet. It is shown that indeed a case can be made that magnetotail flapping also occurs at Jupiter and Saturn. Calculations of the wave period using generic magnetotail models show that the observed periods are much shorter than their theoretical estimates, and that this discrepancy can be caused by unknown input parameters for the tail models (e.g., current sheet thickness) and by possible Doppler shifting of the waves in the spacecraft frame through the fast rotation of the giant planets.


1996 ◽  
Vol 14 (10) ◽  
pp. 1019-1024 ◽  
Author(s):  
H. Kawano ◽  
T. Higuchi

Abstract. In order to determine the normal direction of the magnetopause, the minimum variance analysis technique is frequently used: it is applied to the magnetic field data of a magnetopause crossing observed by a satellite, and provides the direction along which the magnetic field variation is minimum. In this study we propose a method to extend naturally the framework of the minimum variance analysis so that it includes all continuity conditions across a planar magnetopause, so that we could use all physical quantities observed by the spacecraft. We first extend it to the electric field: we discuss how to determine the normal direction and the speed of the magnetopause along the normal by using both the magnetic and electric field data. We next discuss the full extension to all continuity conditions across the magnetopause. Finally, we discuss how to extend our method further so that it can deal with the magnetopause which is accelerating. A discussion of application to observations will appear separately.


Sign in / Sign up

Export Citation Format

Share Document