| Literature DB >> 25055947 |
Hiroki Shishido1, Hiroyuki Takashima, Tsuneo Takebayashi, Yoshihiro Akatsuka, Rui Imamura, Hiroshi Nagahama, Ryuzi Shirase.
Abstract
Identification of the compression factor in cervical disc herniation and cervical spondylotic radioculopathy is often problematic when using two-dimensional magnetic resonance imaging (MRI). This prompted us to compare and examined three-dimensional sequences, coherent oscillatory state acquisition for the manipulation of image contrast (COSMIC), fast imaging employing steady state acquisition (FIESTA) and T2 star weighted MR angiography (SWAN) with 3.0-Tesla (T) MRI to visualize the foramen intervertebral nerve root for the cervical spine. Fat-suppressed COSMIC (FS-COSMIC) sequence gave the highest signal intensity ratio (1.85 ± 0.06) of the nerve root and vertebral arch. A significant difference in signal intensity ratio of the nerve root was found between FS-COSMIC and FIESTA sequences. No significant difference was found between the FS-COSMIC and FIESTA sequences in the cerebrospinal fluid and the spinal cord. The FS-COSMIC sequence proved to be the most suitable sequence for intra and extra dura matter.Entities:
Mesh:
Year: 2014 PMID: 25055947 DOI: 10.6009/jjrt.2014_jsrt_70.7.670
Source DB: PubMed Journal: Nihon Hoshasen Gijutsu Gakkai Zasshi ISSN: 0369-4305