Magnesium Depletion and Impact on Produced Brine Compositions in a Waterflooded Reservoir

2019 ◽  
Author(s):  
Oleg Ishkov ◽  
Eric Mackay ◽  
Myles Jordan ◽  
Sarah Blair
Keyword(s):  
Nutrients ◽  
2021 ◽  
Vol 13 (6) ◽  
pp. 1959
Author(s):  
Flora O. Vanoni ◽  
Gregorio P. Milani ◽  
Carlo Agostoni ◽  
Giorgio Treglia ◽  
Pietro B. Faré ◽  
...  

Chronic alcohol-use disorder has been imputed as a possible cause of dietary magnesium depletion. The purpose of this study was to assess the prevalence of hypomagnesemia in chronic alcohol-use disorder, and to provide information on intracellular magnesium and on its renal handling. We carried out a structured literature search up to November 2020, which returned 2719 potentially relevant records. After excluding non-significant records, 25 were retained for the final analysis. The meta-analysis disclosed that both total and ionized circulating magnesium are markedly reduced in chronic alcohol-use disorder. The funnel plot and the Egger’s test did not disclose significant publication bias. The I2-test demonstrated significant statistical heterogeneity between studies. We also found that the skeletal muscle magnesium content is reduced and the kidney’s normal response to hypomagnesemia is blunted. In conclusion, magnesium depletion is common in chronic alcohol-use disorder. Furthermore, the kidney plays a crucial role in the development of magnesium depletion.


2019 ◽  
Vol 624 ◽  
pp. A21 ◽  
Author(s):  
N. G. Guseva ◽  
Y. I. Izotov ◽  
K. J. Fricke ◽  
C. Henkel

A large sample of Mg II emitting star-forming galaxies with low metallicity [O/H] = log(O/H) – log(O/H)⊙ between –0.2 and –1.2 dex is constructed from Data Release 14 of the Sloan Digital Sky Survey. We selected 4189 galaxies with Mg II λ2797, λ2803 emission lines in the redshift range z ∼ 0.3–1.0 or 35% of the total Sloan Digital Sky Survey star-forming sample with redshift z ≥ 0.3. We study the dependence of the magnesium-to-oxygen and magnesium-to-neon abundance ratios on metallicity. Extrapolating this dependence to [Mg/Ne] = 0 and to solar metallicity we derive a magnesium depletion of [Mg/Ne] ≃ –0.4 (at solar metallicity). We prefer neon instead of oxygen to evaluate the magnesium depletion in the interstellar medium because neon is a noble gas and is not incorporated into dust, contrary to oxygen. Thus, we find that more massive and more metal abundant galaxies have higher magnesium depletion. The global parameters of our sample, such as the mass of the stellar population and star formation rate, are compared with previously obtained results from the literature. These results confirm that Mg II emission has a nebular origin. Our data for interstellar magnesium-to-oxygen abundance ratios relative to the solar value are in good agreement with similar measurements made for Galactic stars, for giant stars in the Milky Way satellite dwarf galaxies, and with low-metallicity damped Lyman-alpha systems.


Metabolism ◽  
1967 ◽  
Vol 16 (4) ◽  
pp. 345-357 ◽  
Author(s):  
Fima Lifshitz ◽  
Helen C. Harrison ◽  
Evelyn C. Bull ◽  
Harold E. Harrison

The Lancet ◽  
1973 ◽  
Vol 301 (7810) ◽  
pp. 1005 ◽  
Author(s):  
MichaelE. Scott
Keyword(s):  

1964 ◽  
Vol 15 (3) ◽  
pp. 133-143 ◽  
Author(s):  
MAURICE E. SHILS
Keyword(s):  

Metabolism ◽  
1966 ◽  
Vol 15 (10) ◽  
pp. 884-895 ◽  
Author(s):  
Michael J. Dunn ◽  
Mackenzie Walser

1981 ◽  
Vol 38 (10) ◽  
pp. 650-652 ◽  
Author(s):  
R. F. Saul ◽  
J. B. Selhorst

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