Sentence examples for angle field from inspiring English sources

Implementations of magic angle field rotation are extremely demanding due to power requirements or an inaccessible geometry.

High-resolution T2* images were acquired using a gradient echo sequence, TR 10 ms, TE 4.5 ms, 6° flip angle, field of view (FOV) 4 cm, and a voxel size of 0.098 × 0.098 × 0.30 mm.

Moreover, the parameter Θ denotes the steering vector of the angle field [17] and is independent of the space location: varTheta =left[begin{array}{cc}hfill -sin varphi hfill & hfill cos theta cos varphi hfill hfill cos varphi hfill & hfill cos theta sin varphi hfill hfill 0hfill & hfill -sin theta hfill end{array}right] (26).

The fifth of the technology milestones required the demonstration of the Microarcsecond Metrology Testbed at a performance of 3,200 picometers over its wide angle field of regard.

The narrow angle field will be used by SIM to detect terrestrial planets; the team applied the same criteria to both the narrow and wide angle measurements.

Scoring was carried out using an Olympus CH2 light microscope (Tokyo, Japan) with a wide angle (field size of 0.274 mm and field diameter of 0.59 mm).

The physicochemical properties of polymerized phospholipid monolayer on the substrate were evaluated using water contact angle, field-emission scanning electron micrograph (FE-SEM), atomic force microscopy (AFM) and X-ray photoelectron spectroscopy (XPS).

Treatment plans were developed by applying tangential photon fields set up isocentrically, with or without individually weighted segmental fields superimposed on the tangential fields and 1-2 coplanar, different gantry angle fields.

The key ingredients appear to be three cameras that capture a 120-degree wide-angle field of view from the front, an even wider 180 degree span from the back, a depth sensing camera that captures images at the relatively modest 320×180 resolution, and a 4MP color camera sensor for snapping regular pics.

The current instrument design consists of five coded aperture γ-ray telescopes: a central telescope with 1892 cmb of detector area, 1.9′ angular resolution, and 8.3° half-angle field of view (FOV); and four side-looking telescopes, each with 1945 cmb detector area, 3.8′ resolution, and 26.1° FOV.

Additionally, the high-magnification probe can be optically scanned toward and engaged at any subfield within the wide-angle field [ 12].