scholarly journals Effect of stationary longitudinal structures on the growth of Tollmin-Schlichting waves

2019 ◽  
Vol 1404 ◽  
pp. 012080
Author(s):  
S A Gaponov ◽  
N M Terehkova
Author(s):  
Yangkun Liu ◽  
Jiyao Xu ◽  
Chao Xiong ◽  
Xiao Liu ◽  
Bing Guo

2001 ◽  
Vol 203 ◽  
pp. 251-253
Author(s):  
E. E. Benevolenskaya ◽  
A. G. Kosovichev ◽  
P. H. Scherrer

We present results of investigation of the large-scale structure of the solar corona during the transition period between solar cycles 22 and 23 and at the beginning of the current cycle 23 using the SOHO/EIT EUV data obtained in 171 Å, 195 Å, 284 Å and 304 Å lines. For this analysis the data were transformed into synoptic maps for each of the spectral lines, and for the 195/171 line ratio which is an index of the coronal temperature. The synoptic maps reveal stable longitudinal structures in the coronal intensities and temperature, which are related to large-scale magnetic field structures. We discuss the relation between the coronal and photospheric magnetic structures obtained from the SOHO/MDI data, and compare the rotation rates of these structures with the rotation profile of the solar interior in order to determine the possible origin of the coronal structures.


2011 ◽  
Vol 29 (1) ◽  
pp. 81-89 ◽  
Author(s):  
P. S. Brahmanandam ◽  
Y.-H. Chu ◽  
K.-H. Wu ◽  
H.-P. Hsia ◽  
C.-L. Su ◽  
...  

Abstract. From global soundings of ionospheric electron density made with FORMOSAT 3/COSMIC satellites for September 2006–August 2009, day-night variations in vertical and longitudinal structures of the electron densities in equatorial E- and F-regions for different seasons are investigated for the first time. The results reveal that the wavenumber-3 and wavenumber-4 patterns dominated the nighttime (22:00–04:00 LT) F-region longitudinal structures in solstice and in equinox seasons, respectively. In daytime (08:00–18:00 LT) F-region, the wavenumber-4 patterns governed the longitudinal structures in the September equinox and December solstice, and wavenumber-3 in March equinox and June solstice respectively. A comparison of the daytime and nighttime longitudinal electron density structures indicates that they are approximately 180° out of phase with each other. It is believed that this out of phase relation is very likely the result of the opposite phase relation between daytime and nighttime nonmigrating diurnal tidal winds that modulate background E-region dynamo electric field at different places, leading to the day-night change in the locations of the equatorial plasma fountains that are responsible for the formation of the F-region longitudinal structures. Further, a good consistency between the locations of the density structures in the same seasons of the different years for both daytime and nighttime epochs has been noticed indicating that the source mechanism for these structures could be the same.


2011 ◽  
Vol 56 (5) ◽  
pp. 690-696 ◽  
Author(s):  
E. D. Donets ◽  
E. E. Donets ◽  
E. M. Syresin ◽  
A. E. Dubinov ◽  
I. V. Makarov ◽  
...  

1975 ◽  
Vol 17 (1) ◽  
pp. 129-131 ◽  
Author(s):  
W. Scheid ◽  
H. Traut

Anaphase chromosomes exhibit two longitudinal structures which are connected at their ends in a U-shaped closed configuration. The U-shaped ends might be part of the chromosome characterized by a relatively dense condensation of chromosomal material or part of the loop-like structure of the chromosome per se.


Sign in / Sign up

Export Citation Format

Share Document