File:Inversion Recovery Attenuation (expand the description below for a detailed explanation).webm

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Inversion_Recovery_Attenuation_(expand_the_description_below_for_a_detailed_explanation).webm(WebM audio/video file, VP8/Vorbis, length 54 s, 256 × 240 pixels, 165 kbps overall, file size: 1.06 MB)

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English: Inversion recovery is primarily concerned with T1 relaxation and is used to nullify signal from a subpopulation of protons. By starting with a 180 degree pulse, the rotated protons have practically zero XY-component; they experience only T1 decay along the Z-axis. The individual protons do indeed precess with an XY-component, but the 180 degree pulse does not necessarily align them. They point in multiple random directions, and so they cancel each other out.

If another 90 degree pulse is delivered just as net magnetic dipole of the targeted subpopulation crosses through the XY-plane, the protons will all rotate into the XY-plane, but they will have an XY-component that will continue to experience T1 decay without producing any measurable signal. Meanwhile, tissues with greater or lesser T1 values will rotate into the XY-plane with a magnitude greater than one, and will precess normally and produce a measurable signal. The result is that the same image can be produced, but the targeted subpopulation will show up as hypointense on the final image. The graphic shows the following three individual sequences: 1. The 90 degree pulse occurs before the Z-component crosses zero. It thus rotates out into the XY-plane and creates a measurable signal. 2. The 90 degree pulse occurse right when the Z-component crosses zero. It thus has no net XY-component after the rotation and creates no signal. 3. The 90 degree pulse occurs after the Z-component crosses zero. It thus rotates back out into the XY-plane and produces measurable signal.

Examples of IR sequences include FLuid Attenuation Inversion Recovery (FLAIR) and Short T1 Inversion recovery (STIR).
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Source YouTube: Inversion Recovery Attenuation (expand the description below for a detailed explanation) – View/save archived versions on archive.org and archive.today
Author Tyler Moore

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This file is licensed under the Creative Commons Attribution 3.0 Unported license.
Attribution: Tyler Moore
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Date/TimeThumbnailDimensionsUserComment
current12:27, 19 June 201854 s, 256 × 240 (1.06 MB)Vislupus (talk | contribs)Imported media from https://www.youtube.com/watch?v=MnlG51a4sLE

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Format Bitrate Download Status Encode time
VP9 240P 135 kbps Completed 17:18, 24 June 2023 37 s
Streaming 240p (VP9) 131 kbps Completed 06:15, 6 December 2023 1.0 s
WebM 360P 453 kbps Completed 15:57, 30 November 2023 4.0 s
Streaming 144p (MJPEG) 459 kbps Completed 21:36, 15 November 2023 2.0 s
Stereo (Opus) 2 kbps Completed 16:34, 24 November 2023 1.0 s
Stereo (MP3) 128 kbps Completed 13:29, 10 November 2023 2.0 s

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