The existence of a viscous zone in the region of shock-wave interaction allows a continuous transition from the parameters behind the Mach stem to the parameters behind the reflected shock, which is impossible in the inviscid three-shock theory.
The heat shock response (HSR) in mammals is characterized by the transient activation of the latent transcription factor HSF1, which binds conserved heat shock elements (HSEs) within the regulatory region of heat shock genes (Hsp) and drives their transcription.
We study the evolution of the plasma conditions in the shock front region magnetically connected to each spacecraft, that is the region of the shock front scanned by the "cobpoint" (Heras et al., 1995), as the shock propagates away from the Sun.
Hsf1 and Msn2/4 bind to heat shock elements (HSEs) and stress response elements (STREs), respectively, in the promoter region of heat shock proteins and activate the expression of target gene transcription (Morano et al. [2012]).
In this paper, a 200-mTorr Ar pressure is high enough to form the shock front, and distances of 25 mm and 30 mm may be a region of the shock front.
The increased number of modes may be due to the increased Mach number per se, or the presence of the strong spatial gradients in the region of the shock.
These mutations are insertions of a transposable element, the P-element, into the regulatory region of heat shock genes.
Some studies have demonstrated that EGCG can inhibit the transcriptional activity of aryl hydrocarbon receptor (AhR) through the mechanism that involves direct binding of EGCG to the C-terminal region of heat shock protein 90 (HSP90) [ 12].
All three known HSE motifs (perfect, gap and step type, see additional file 4 for motif consensus sequences) were present in the promoter region of heat-shock induced genes.
The fast response may be related to a fast magnetosonic pulse propagating across the magnetosphere from the region of the IP shock impact on the magnetopause, with a velocity ~103 km/s, whereas a slow intense response is caused by the disturbance propagating along the magnetospheric flanks with a shock velocity in the magnetosheath.
Dubinin et al. (2006) showed an example of an energy-bunched structure in the spectrogram at two distinct energies in the foot region of the bow shock for a quasi-perpendicular shock.
