Topographic analysis of esophageal double-peaked waves

被引:48
|
作者
Clouse, RE [1 ]
Staiano, A [1 ]
Alrakawi, A [1 ]
机构
[1] Washington Univ, Sch Med, Div Gastroenterol, St Louis, MO 63110 USA
关键词
D O I
10.1016/S0016-5085(00)70252-6
中图分类号
R57 [消化系及腹部疾病];
学科分类号
摘要
Background & Aims: Esophageal double-peaked waves occur with increased frequency in patients with functional esophageal symptoms. This study was undertaken to further understand the mechanisms responsible for their production. Methods: Topographic methods that consider temporal and spatial relationships of pressure data were used to examine 74 double-peaked waves detected in 18 subjects referred for manometric evaluation of unexplained symptoms. The studies were performed with a computerized data acquisition and analysis system designed for topographic plotting. Results: The second peak appeared to represent muscle contraction that merged with an unusually strong pressure site in the third topographic segment and covered 6.3 +/- 1.6 cm (33.5% +/- 8.5% esophageal length) proximal to this site. In 50 swallows (67.6%), the peak itself progressed in a retrograde direction at 13.2 +/- 10.8 cm/s, suggesting cephalad extension of a strong distal motor event. Analysis of wave onsets and movement: of the peristaltic trailing edge detected retrograde propagation in up to 33.8% of waves, antegrade propagation in 2.7%, and simultaneous contraction in the remainder. Conclusions: In symptomatic patients, the second peak in a double-peaked wave is typically a short, simultaneous, or retrograde pressure event in the region of and merging with the third topographic segment in the distal esophageal body. Topographic methods help explain the common association of these waveforms with other features of exaggerated contraction in the distal esophagus and suggest their relationship to inadequate inhibitory nerve function.
引用
收藏
页码:469 / 476
页数:8
相关论文
共 50 条
  • [31] DISCOVERY OF THE MOST DISTANT DOUBLE-PEAKED EMITTER AT z=1.369
    Luo, B.
    Brandt, W. N.
    Silverman, J. D.
    Strateva, I. V.
    Bauer, F. E.
    Capak, P.
    Kartaltepe, J.
    Lehmer, B. D.
    Mainieri, V.
    Salvato, M.
    Szokoly, G.
    Schneider, D. P.
    Vignali, C.
    ASTROPHYSICAL JOURNAL, 2009, 695 (02): : 1227 - 1232
  • [32] The spectral energy distributions of AGN with double-peaked Balmer lines
    Strateva, I.
    Brandt, W. N.
    Eracleous, M.
    Garmire, C.
    Komossa, S.
    CENTRAL ENGINE OF ACTIVE GALACTIC NUCLEI, 2007, 373 : 399 - 402
  • [33] Double-peaked emission lines in radio-loud AGNs
    Eracleous, M
    Halpern, JP
    ACCRETION PROCESSES IN ASTROPHYSICAL SYSTEMS: SOME LIKE IT HOT!, 1998, (431): : 257 - 260
  • [34] Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies
    Meng-Xin Wang
    A-Li Luo
    Research in Astronomy and Astrophysics, 2019, 19 (09) : 37 - 54
  • [35] Approximation of a double-peaked lightning channel-base current
    Javor, Vesna
    COMPEL-THE INTERNATIONAL JOURNAL FOR COMPUTATION AND MATHEMATICS IN ELECTRICAL AND ELECTRONIC ENGINEERING, 2012, 31 (03) : 1007 - 1017
  • [36] Double-peaked impact force of very soft gel balls
    Tanaka, Y
    PHYSICAL REVIEW E, 2006, 73 (03):
  • [37] Stability of double-peaked solitons in Bragg gratings with the quadratic nonlinearity
    Leitner, Y
    Malomed, BA
    PHYSICAL REVIEW E, 2005, 71 (05):
  • [38] The ultraviolet spectra of active galaxies with double-peaked emission lines
    Eracleous, M
    Halpern, JP
    Storchi- Bergmann, T
    Filippenko, AV
    Wilson, AS
    Livio, M
    INTERPLAY AMONG BLACK HOLES, STARS AND ISM IN GALACTIC NUCLEI, 2004, (222): : 29 - 32
  • [39] Models and ideas for the interpretation of the variability of double-peaked emission lines
    Eracleous, Michael
    Lewis, Karen T.
    Bogdanovic, Tamara
    Gezari, Suvi
    Halpern, Jules P.
    AGN VARIABILITY FROM X-RAYS TO RADIO WAVES, 2006, 360 : 227 - +
  • [40] Discovery of a quasar with double-peaked broad balmer emission lines
    Terwel, Jacco H.
    Jonker, Peter G.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 512 (01) : L80 - L84