The behaviour of the midlatitude F-region at the time of four magnetospheric substorms during the night of 29/30 October 1973

1976 ◽  
Vol 24 (3) ◽  
pp. 293-298
Author(s):  
M.M. Gogoshev ◽  
K.B. Serafimov ◽  
Ts.N. Gogosheva ◽  
K.M. Kazakov
1986 ◽  
Author(s):  
Bodo W. Reinisch ◽  
Jurgen Buchau ◽  
Edward J. Weber ◽  
Claude G. Dozois ◽  
Klaus Bibl
Keyword(s):  

1999 ◽  
Vol 19 (11) ◽  
pp. 7751-7758 ◽  
Author(s):  
Wei Yan ◽  
Elizabeth A. Craig

ABSTRACT Hsp40s are ubiquitous, conserved proteins which function with molecular chaperones of the Hsp70 class. Sis1 is an essential Hsp40 of the cytosol of Saccharomyces cerevisiae, thought to be required for initiation of translation. We carried out a genetic analysis to determine the regions of Sis1 required to perform its key function(s). A C-terminal truncation of Sis1, removing 231 amino acids but retaining the N-terminal 121 amino acids encompassing the J domain and the glycine-phenylalanine-rich (G-F) region, was able to rescue the inviability of a Δsis1 strain. The yeast cytosol contains other Hsp40s, including Ydj1. To determine which regions carried the critical determinants of Sis1 function, we constructed chimeric genes containing portions of SIS1 and YDJ1. A chimera containing the J domain of Sis1 and the G-F region of Ydj1 could not rescue the lethality of the Δsis1 strain. However, a chimera with the J domain of Ydj1 and the G/F region of Sis1 could rescue the strain’s lethality, indicating that the G-F region is a unique region required for the essential function of Sis1. However, a J domain is also required, as mutants expected to cause a disruption of the interaction of the J domain with Hsp70 are inviable. We conclude that the G-F region, previously thought only to be a linker or spacer region between the J domain and C-terminal regions of Hsp40s, is a critical determinant of Sis1 function.


2006 ◽  
Vol 37 (5) ◽  
pp. 1007-1017 ◽  
Author(s):  
M.A. Abdu ◽  
I.S. Batista ◽  
B.W. Reinisch ◽  
J.H.A. Sobral ◽  
A.J. Carrasco

Entropy ◽  
2021 ◽  
Vol 23 (4) ◽  
pp. 390
Author(s):  
Pouya Manshour ◽  
Georgios Balasis ◽  
Giuseppe Consolini ◽  
Constantinos Papadimitriou ◽  
Milan Paluš

An information-theoretic approach for detecting causality and information transfer is used to identify interactions of solar activity and interplanetary medium conditions with the Earth’s magnetosphere–ionosphere systems. A causal information transfer from the solar wind parameters to geomagnetic indices is detected. The vertical component of the interplanetary magnetic field (Bz) influences the auroral electrojet (AE) index with an information transfer delay of 10 min and the geomagnetic disturbances at mid-latitudes measured by the symmetric field in the H component (SYM-H) index with a delay of about 30 min. Using a properly conditioned causality measure, no causal link between AE and SYM-H, or between magnetospheric substorms and magnetic storms can be detected. The observed causal relations can be described as linear time-delayed information transfer.


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