コーパス検索結果 (1語後でソート)
通し番号をクリックするとPubMedの該当ページを表示します
1 and isotropic (equal in gain for every head rotation axis).
2 of nanoplates that intersect along a 6-fold rotation axis.
3 is is tilted by less than 3 degrees from the rotation axis.
4 ly a small translational component along the rotation axis.
5 on, and the Au(38)S(24) framework has a C(3) rotation axis.
6 ed between 5 degrees and 12 degrees from the rotation axis.
7 ld--is nearly symmetrically aligned with the rotation axis.
8 its strength or its near-alignment with the rotation axis.
9 degrees and a translation of >20 A along the rotation axis.
10 to, instead of nearly parallel to, the Sun's rotation axis.
11 second asymmetric dimer by a local two-fold rotation axis.
12 ffects of asymmetry in close vicinity to the rotation axis.
13 multiple grains that roughly share a common rotation axis.
14 pposite propulsion states along the sphere's rotation axis.
15 y charged surface orthogonal to the internal rotation axis.
17 ules related by a noncrystallographic 2-fold rotation axis approximately parallel to the z-direction.
18 ides with an abrupt lateral shift in Earth's rotation axis at ~50 Ma, independently validated through
19 xplained by reorientation of the satellite's rotation axis because of the presence of a low-density d
21 ted with the smooth halo is aligned with the rotation axis for the plane of dwarf galaxies(14) that e
23 ethod, we demonstrate that by offsetting the rotation axis from the beam axis by 1.25 times the full-
24 f the rotational bulge acts to stabilize the rotation axis, geodynamic models for oscillatory TPW gen
27 rred translational direction and a preferred rotation axis in space, both with cosine tuning function
28 ickness can be reduced, even to zero, if the rotation axis is stabilized by long-term excess elliptic
29 scale and is less invariant parallel to the rotation axis (less geostrophic), and convection transpo
30 -less correspond to rotations about a common rotation axis making it difficult to satisfy this condit
36 rically symmetric oscillating flow about the rotation axis) or a localized Alfven wave in Jupiter's m
38 milar size, rotation rate and inclination of rotation axis, possessing an atmosphere and a solid surf
39 nature, arising in objects without a proper rotation axis, therefore existing as forms with distinct
40 rdless of vertical gaze position, the ocular rotation axis tilted backward 4 degrees farther in abduc
42 diffraction pattern in which the fiber axis (rotation axis) was parallel to the H-bonding direction o
43 basal planes are partially aligned with the rotation axis, we can account for seismological observat
44 cal 6-fold symmetry axis of the P hexon as a rotation axis, we examined the geometrical relationships
45 proximately 30 degrees away from the orbital rotation axis, which avoids both obscuration from the he
46 with its c axis aligned perpendicular to the rotation axis yields anisotropy that is compatible with