scholarly journals High-latitudes magnetic substorms under different types of the solar wind large-scale structure

Author(s):  
Irina Despirak ◽  
Andris Lubchich ◽  
Natalia Kleimenova
1992 ◽  
Vol 9 ◽  
pp. 671-680
Author(s):  
Neta A. Bahcall

AbstractA consistent picture of large-scale structure appears to be emerging from different types of observations including the spatial distribution of galaxies, clusters of galaxies, narrow pencil-beam surveys, and quasars. I describe these observations below. A network of large-scale superclusters, up to ~ 150 Mpc in scale, is suggested. The supercluster network surrounds low-density regions of similar scales, suggesting a “cellular” structure of the universe. (Ho = 100 km /s/ Mpc is used).


1974 ◽  
Vol 60 ◽  
pp. 625-630 ◽  
Author(s):  
Carl E. Heiles ◽  
Carl Heiles

The correlation of Hiand dust at high latitudes gives different results depending on whether one uses galaxy or reddening data for the dust distribution. It is not certain to what extent this depends on differences in the gas to dust ratio or on difficulties in determining the amount of dust from the optical data. The correlation of Hiand continuum radiation shows Histructures associated with the large-scale loops. There is also a coincidence of a hole in both the Hiand continuum.


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