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Träfflista för sökning "WFRF:(Rosenqvist D.) srt2:(2010-2014)"

Search: WFRF:(Rosenqvist D.) > (2010-2014)

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  • Wallentin, Lars, et al. (author)
  • Efficacy and safety of apixaban compared with warfarin at different levels of predicted international normalized ratio control for stroke prevention in atrial fibrillation
  • 2013
  • In: Circulation. - 0009-7322 .- 1524-4539. ; 127:22, s. 2166-2176
  • Journal article (peer-reviewed)abstract
    • BackgroundIn the Apixaban for Reduction in Stroke and Other Thromboembolic Events in Atrial Fibrillation (ARISTOTLE) trial, apixaban compared with warfarin reduced stroke and systemic embolism, major bleeding, and mortality. We evaluated treatment effects in relation to 2 predictions of time in therapeutic range (TTR).Methods and ResultsThe trial randomized 18 201 patients with atrial fibrillation to apixaban 5 mg twice daily or warfarin for at least 12 months. For each patient, a center average TTR was estimated with the use of a linear mixed model on the basis of the real TTRs in its warfarin-treated patients, with a fixed effect for country and random effect for center. For each patient, an individual TTR was also predicted with the use of a linear mixed effects model including patient characteristics as well. Median center average TTR was 66% (interquartile limits, 61% and 71%). Rates of stroke or systemic embolism, major bleeding, and mortality were consistently lower with apixaban than with warfarin across center average TTR and individual TTR quartiles. In the lowest and highest center average TTR quartiles, hazard ratios for stroke or systemic embolism were 0.73 (95% confidence interval [CI], 0.53–1.00) and 0.88 (95% CI, 0.57–1.35) (Pinteraction=0.078), for mortality were 0.91 (95% CI, 0.74–1.13) and 0.91 (95% CI, 0.71–1.16) (Pinteraction=0.34), and for major bleeding were 0.50 (95% CI, 0.36–0.70) and 0.75 (95% CI, 0.58–0.97) (Pinteraction=0.095), respectively. Similar results were seen for quartiles of individual TTR.ConclusionsThe benefits of apixaban compared with warfarin for stroke or systemic embolism, bleeding, and mortality appear similar across the range of centers’ and patients’ predicted quality of international normalized ratio control.Clinical Trial RegistrationURL: http://www.clinicaltrials.gov. Unique identifier: NCT00412984.
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  • Ågren, Karin, et al. (author)
  • Detection of currents and associated electric fields in Titan's ionosphere from Cassini data
  • 2011
  • In: Journal of Geophysical Research. - 0148-0227 .- 2156-2202. ; 116:4, s. A04313-
  • Journal article (peer-reviewed)abstract
    • We present observations from three Cassini flybys of Titan using data from the radio and plasma wave science, magnetometer and plasma spectrometer instruments. We combine magnetic field and cold plasma measurements with calculated conductivities and conclude that there are currents of the order of 10 to 100 nA m (2) flowing in the ionosphere of Titan. The currents below the exobase (similar to 1400 km) are principally field parallel and Hall in nature, while the Pedersen current is negligible in comparison. Associated with the currents are perpendicular electric fields ranging from 0.5 to 3 mu V m (1).
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  • Easton, J. Donald, et al. (author)
  • Apixaban compared with warfarin in patients with atrial fibrillation and previous stroke or transient ischaemic attack : a subgroup analysis of the ARISTOTLE trial
  • 2012
  • In: Lancet Neurology. - 1474-4422 .- 1474-4465. ; 11:6, s. 503-511
  • Journal article (peer-reviewed)abstract
    • BackgroundIn the ARISTOTLE trial, the rate of stroke or systemic embolism was reduced by apixaban compared with warfarin in patients with atrial fibrillation (AF). Patients with AF and previous stroke or transient ischaemic attack (TIA) have a high risk of stroke. We therefore aimed to assess the efficacy and safety of apixaban compared with warfarin in prespecified subgroups of patients with and without previous stroke or TIA.MethodsBetween Dec 19,2006, and April 2,2010, patients were enrolled in the ARISTOTLE trial at 1034 clinical sites in 39 countries. 18 201 patients with AF or atrial flutter were randomly assigned to receive apixaban 5 mg twice daily or warfarin (target international normalised ratio 2.0-3.0). The median duration of follow-up was 1.8 years (IQR 1.4-2.3). The primary efficacy outcome was stroke or systemic embolism, analysed by intention to treat. The primary safety outcome was major bleeding in the on-treatment population. All participants, investigators, and sponsors were masked to treatment assignments. In this subgroup analysis, we estimated event rates and used Cox models to compare outcomes in patients with and without previous stroke or TIA. The ARISTOTLE trial is registered with ClinicalTrials.gov, number NTC00412984.FindingsOf the trial population, 3436 (19%) had a previous stroke or TIA. In the subgroup of patients with previous stroke or TIA, the rate of stroke or systemic embolism was 2.46 per 100 patient-years of follow-up in the apixaban group and 3.24 in the warfarin group (hazard ratio [HR] 0.76, 95% CI 0.56 to 1.03); in the subgroup of patients without previous stroke or TLA, the rate of stroke or systemic embolism was 1.01 per 100 patient-years of follow-up with apixaban and 1.23 with warfarin (HR 0.82, 95% CI 0.65 to 1.03; p for interaction=0.71). The absolute reduction in the rate of stroke and systemic embolism with apixaban versus warfarin was 0.77 per 100 patient-years of follow-up (95% CI -0.08 to 1.63) in patients with and 0.22 (-0.03 to 0.47) in those without previous stroke or TIA. The difference in major bleeding with apixaban compared with warfarin was 1.07 per 100 patient-years (95% CI 0.09-2.04) in patients with and 0.93 (0.54-1.32) in those without previous stroke or TIA.InterpretationThe effects of apixaban versus warfarin were consistent in patients with AF with and without previous stroke or TIA. Owing to the higher risk of these outcomes in patients with previous stroke or TIA, the absolute benefits of apixaban might be greater in this population.FundingBristol-Myers Squibb and Pfizer.
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  • Hollenberg, J, et al. (author)
  • replik till Bengt Fagrell : Fler hjärtstartare behövs i samhället
  • 2013
  • In: Läkartidningen. - : Läkartidningen Förlag AB. - 0023-7205 .- 1652-7518. ; 110:19-20, s. 959-
  • Journal article (pop. science, debate, etc.)abstract
    • Fler hjärtstartare behövs, men konceptet behöver utvecklas. Vi måste dessutom finna nya sätt att mobilisera hjärtstartare till platsen för hjärtstoppet.
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  • Opgenoorth, Hermann J., et al. (author)
  • Day-side ionospheric conductivities at Mars
  • 2010
  • In: Planetary and Space Science. - : Elsevier BV. - 0032-0633 .- 1873-5088. ; 58:10, s. 1139-1151
  • Journal article (peer-reviewed)abstract
    • We present estimates of the day-side ionospheric conductivities at Mars based on magnetic field measurements by Mars Global Surveyor (MGS) at altitudes down to similar to 100 km during aerobraking orbits early in the mission. At Mars, the so-called ionospheric dynamo region, where plasma/neutral collisions permit electric currents perpendicular to the magnetic field, lies between 100 and 250 km altitude. We find that the ionosphere is highly conductive in this region, as expected, with peak Pedersen and Hall conductivities of 0.1-1.5 S/m depending on the solar illumination and induced magnetospheric conditions. Furthermore, we find a consistent double peak pattern in the altitude profile of the day-side Pedersen conductivity, similar to that on Titan found by Rosenqvist et al. (2009). A high altitude peak, located between 180 and 200 km, is equivalent to the terrestrial peak in the lower F-layer. A second and typically much stronger layer of Pedersen conductivity is observed between 120 and 130 km, which is below the Hall conductivity peak at about 130-140 km. In this altitude region, MGS finds a sharp decrease in induced magnetic field strength at the inner magnetospheric boundary, while the day-side electron density is known to remain high as far down as 100 km. We find that such Titan-like behaviour of the Pedersen conductivity is only observed under regions of strongly draped magnetospheric field-lines, and negligible crustal magnetic anomalies below the spacecraft. Above regions of strong crustal magnetic anomalies, the Pedersen conductivity profile becomes more Earth-like with one strong Pedersen peak above the Hall conductivity peak. Here, both conductivities are 1-2 orders of magnitude smaller than the above only weakly magnetised crustal regions, depending on the strength of the crustal anomaly field at ionospheric altitudes. This nature of the Pedersen conductivity together with the structured distribution of crustal anomalies all over the planet should give rise to strong conductivity gradients around such anomalies. Day-side ionospheric conductivities on Mars (in regions away from the crustal magnetic anomalies) and Titan seem to behave in a very similar manner when horizontally draped magnetic field-lines partially magnetise a sunlit ionosphere. Therefore, it appears that a similar double peak structure of strong Pedersen conductivity could be a more general feature of non-magnetised bodies with ionised upper atmospheres, and thus should be expected to occur also at other non-magnetised terrestrial planets like Venus or other planetary bodies within the host planet magnetospheres.
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