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1 ge satellite Charon is its dark red northern polar cap.
2 temporal patches of water frost in the north polar cap.
3 ular depressions commonly found on the south polar cap.
4 ed near the edge of Mars' southern perennial polar cap.
5 a thick CO2 layer, as is the residual south polar cap.
6 , with stronger westerly flow encircling the polar cap.
7 n-based transport resulted in unstable Cdc42 polar caps.
8 e sources reach all latitudes, including the polar caps.
9 ringtime sublimation of Mars' CO(2) seasonal polar caps.
10 ed correctly, septins promote turning of the polar cap and proper tracking of a pheromone gradient.
11 re, we investigate the dynamic nature of the polar cap and the regulation of the GTPase Cdc42 in the
12 und that Cdc42 exchanged rapidly between the polar caps and cytosol and that this rapid exchange requ
13 oscillations near 32 degrees S, a warm south polar cap, and a compact hot point within 3 degrees of t
16 ggest lower-latitude aurora and increases in polar cap area, as well as heating, expansion, and volat
17 plume from a source centered near the south polar cap, as distinct from a separately measured more u
18 ther that the septin structure surrounds the polar cap, ensuring that cell growth is directed toward
19 ation, stronger actin polymerization, higher polar cap formation, and enhanced adhesion and chemotact
22 distribution of surface IcsA, such that the polar cap is maintained and some IcsA is distributed alo
23 tion infrastructure, and analog to a Martian polar cap, it is an ideal place to test a sterile drill
26 e nuclear periphery that segregated into two polar caps, perpendicular to the PPB, before nuclear env
28 the planet provide synoptic observations of polar cap retreat, condensate clouds, and the lifecycle
29 the evolution of sublimation from the north polar cap, revealing that the released water has a repre
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