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- Reveiz, Ludovic, et al.
(författare)
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Stress ulcer, gastritis, and gastrointestinal bleeding prophylaxis in critically ill pediatric patients : a systematic review
- 2010
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Ingår i: Pediatric Critical Care Medicine. - : Lippincott Williams & Wilkins. - 1529-7535 .- 1947-3893. ; 11:1, s. 124-132
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Tidskriftsartikel (refereegranskat)abstract
- OBJECTIVE: To identify and evaluate the quality of evidence supporting prophylactic use of treatments for stress ulcers and upper gastrointestinal bleeding. Stress ulcers, erosions of the stomach and duodenum, and upper gastrointestinal bleeding are well-known complications of critical illness in children admitted to the pediatric intensive care unit.DATA SOURCES: Studies were identified from the Cochrane Central Register of Controlled Trials, PUBMED; LILACS; Scirus. We also scanned bibliographies of relevant studies.STUDY SELECTION: This systematic review of randomized controlled trials assessed the effects of drugs for stress-related ulcers, gastritis, and upper gastrointestinal bleeding in critically ill children admitted to the pediatric intensive care unit.DATA EXTRACTION AND SYNTHESIS: Two reviewers independently extracted the relevant data. Most randomized controlled trials were judged as having unclear risk of bias. When pooling two randomized controlled trials, treatment was significantly more effective in preventing upper gastrointestinal bleeding (macroscopic or important bleeding) compared with no treatment (two studies = 300 participants; relative risk, 0.41; 95% confidence interval, 0.19-0.91; I = 12%). Meta-analysis of two studies found no significant difference in death rates among groups (two randomized controlled trials = 132 participants; relative risk, 1.39; 95% confidence interval, 0.70-2.79; I = 4%). The rate of pneumonia was not significantly different when comparing treatment and no treatment in one study. When comparing ranitidine with no treatment, significant differences were found in the proportion of mechanically ventilated children with normal gastric mucosal endoscopic findings by histologic specimens (one randomized controlled trial = 48 participants; relative risk, 3.53; 95% confidence interval, 1.34-9.29). No significant differences were found when comparing different drugs (omeprazole, ranitidine, sucralfate, famotidine, amalgate), doses, or regimens for main outcomes (deaths, endoscopic findings of erosion or ulcers, upper gastrointestinal bleeding, or pneumonia).CONCLUSIONS: Although pooled data of two studies suggested that critically ill pediatric patients may benefit from receiving prophylactic treatment to prevent upper gastrointestinal bleeding, we found that high-quality evidence to guide clinical practice is still limited.
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| 2. |
- Telloni, Daniele, et al.
(författare)
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Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations
- 2022
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Ingår i: Astrophysical Journal. - : IOP Publishing Ltd. - 0004-637X .- 1538-4357. ; 935:2
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Tidskriftsartikel (refereegranskat)abstract
- The solar wind measured in situ by Parker Solar Probe in the very inner heliosphere is studied in combination with the remote-sensing observation of the coronal source region provided by the METIS coronagraph aboard Solar Orbiter. The coronal outflows observed near the ecliptic by Metis on 2021 January 17 at 16:30 UT, between 3.5 and 6.3 R (circle dot) above the eastern solar limb, can be associated with the streams sampled by PSP at 0.11 and 0.26 au from the Sun, in two time intervals almost 5 days apart. The two plasma flows come from two distinct source regions, characterized by different magnetic field polarity and intensity at the coronal base. It follows that both the global and local properties of the two streams are different. Specifically, the solar wind emanating from the stronger magnetic field region has a lower bulk flux density, as expected, and is in a state of well-developed Alfvenic turbulence, with low intermittency. This is interpreted in terms of slab turbulence in the context of nearly incompressible magnetohydrodynamics. Conversely, the highly intermittent and poorly developed turbulent behavior of the solar wind from the weaker magnetic field region is presumably due to large magnetic deflections most likely attributed to the presence of switchbacks of interchange reconnection origin.
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