ライフサイエンスコーパス: polar cap

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 was etched and removed, returning it to the polar cap.

8 e variations during the establishment of the polar cap.

9 d two-dimensional turbulence on an idealized polar cap.

10 n-based transport resulted in unstable Cdc42 polar caps.

11 e sources reach all latitudes, including the polar caps.

12 ringtime sublimation of Mars' CO(2) seasonal polar caps.

13 larities between irregularities found in the polar cap and in the auroral region in that context.

14 ed correctly, septins promote turning of the polar cap and proper tracking of a pheromone gradient.

15 re, we investigate the dynamic nature of the polar cap and the regulation of the GTPase Cdc42 in the

16 und that Cdc42 exchanged rapidly between the polar caps and cytosol and that this rapid exchange requ

17 oscillations near 32 degrees S, a warm south polar cap, and a compact hot point within 3 degrees of t

18 he polar wind, a low energy outflow from the polar cap, and then transitions to the accelerated outfl

19 Clouds observed over the polar cap are likely composed of CO2 that condensed out

20 The martian polar caps are among the most dynamic regions on Mars, g

21 ggest lower-latitude aurora and increases in polar cap area, as well as heating, expansion, and volat

22 plume from a source centered near the south polar cap, as distinct from a separately measured more u

23 ectly implies radiolytic modification of the polar caps by precipitation of Jovian charged particles

24 volution of water released from the southern polar cap during southern summer, the equinox phases, an

25 ther that the septin structure surrounds the polar cap, ensuring that cell growth is directed toward

26 ation, stronger actin polymerization, higher polar cap formation, and enhanced adhesion and chemotact

27 Our models show that the north polar cap formed over the last 1.7-12.0 Myr and that gla

28 Revealing the origins of aurorae in Earth's polar cap has long been a challenge since direct precipi

29 The nature of the martian south polar cap has remained enigmatic since the first spacecr

30 The central portion of the north polar cap is covered by a thick CO2 layer, as is the res

31 distribution of surface IcsA, such that the polar cap is maintained and some IcsA is distributed alo

32 Most of the jovian polar cap is threaded by helical magnetic flux that clos

33 tion infrastructure, and analog to a Martian polar cap, it is an ideal place to test a sterile drill

34 The north polar cap of Mars is the only millions-of-years-old surf

35 to generate a magnetically open, Earth-like polar cap on the time scale of planetary rotation, resul

36 ng the approach phase that show the northern polar cap over a range of longitudes.

37 Staining of the septal or polar cap peptidoglycan by a fluorescent lectin was unaf

38 e nuclear periphery that segregated into two polar caps, perpendicular to the PPB, before nuclear env

39 ptionally gigantic aurora filling the entire polar cap region on a day when the solar wind had almost

40 The south polar cap retreat was similar to that observed by Viking

41 the planet provide synoptic observations of polar cap retreat, condensate clouds, and the lifecycle

42 the evolution of sublimation from the north polar cap, revealing that the released water has a repre

43 tent with the negligible flexure beneath the polar cap seen by radars.

44 These observations are consistent with polar cap stratigraphy(1,7), but lower- to mid-latitude

45 These polar caps then marked the spindle poles upon NEBD.

46 Polar cap topography displays evidence of modification b

47 Under these circumstances, the polar cap travels toward septin structures and away from

48 The two polar cap volumes yield an upper limit of the present su