Magdas Dana Alina, Cuna Stela, Cristea Gabriela, Ionete Roxana Elena, Costinel Diana
Department of Mass Spectrometry, Chromatography and Applied Physics, National Institute for Research and Development of Isotopic and Molecular Technologies, Cluj-Napoca, Romania.
Isotopes Environ Health Stud. 2012 Jun;48(2):345-53. doi: 10.1080/10256016.2012.661731. Epub 2012 Mar 7.
This paper presents a study concerning the isotopic fingerprint ((18)O and (13)C) of some wines prepared from relevant Romanian grape varieties (e.g. Feteasca Alba (FA), Feteasca Regala (FR) and Cabernet Sauvignon (CS)) obtained in different vintage years (2002, 2003, 2004, 2007 and 2008). These wines were obtained from different vineyards having a significant role in the wine market: Cotesti, Tohani, Stefanesti, Aiud, Cotnari, Bucium, Murfatlar, Bujoru, Dragasani and Valea Calugareasca. Several observations related to the dependence of isotope ratios on geographical origin and climatic conditions were drawn. The authentic wines obtained from the FA grape variety from six different vineyards showed δ(18)O values in the range of+3.28 (Cotesti region - 45 °38'N/27 °04'E) to-2.60 ‰ (Aiud region - 46 °19'N/23 °45'E). The δ(13)C values were very similar for all the samples with an average of about-26 ‰. The difference between the δ(18)O values was due to the different climatic zones, which have an influence on the δ(18)O values of wine water. For the wine variety CS obtained from the Dealu Mare-Tohani vineyard, production years 2003 and 2004, a greater difference in the δ(18)O values of wine water ranging from 1.89 (in 2004) to 5.35 ‰ (in 2003) was noted. This difference is explained by the different mean annual temperatures in 2003 and 2004.
本文介绍了一项关于罗马尼亚一些相关葡萄品种(如白妃蒂亚斯卡(FA)、皇家妃蒂亚斯卡(FR)和赤霞珠(CS))在不同年份(2002年、2003年、2004年、2007年和2008年)所酿葡萄酒的同位素指纹(氧-18和碳-13)的研究。这些葡萄酒产自对葡萄酒市场有重要影响的不同葡萄园:科泰斯蒂、托哈尼、斯特凡内斯蒂、阿尤德、科特纳里、布丘姆、穆尔法特拉尔、布约鲁、德拉格萨尼和卡卢加雷亚斯卡谷。得出了一些关于同位素比率与地理来源和气候条件相关性的观察结果。从六个不同葡萄园的FA葡萄品种获得的正宗葡萄酒显示,氧-18值在+3.28(科泰斯蒂地区 - 北纬45°38′/东经27°04′)至-2.60‰(阿尤德地区 - 北纬46°19′/东经23°45′)范围内。所有样品的碳-13值非常相似,平均约为-26‰。氧-18值的差异是由于不同的气候带,其对葡萄酒中水的氧-18值有影响。对于从马勒-托哈尼葡萄园获得的2003年和2004年生产年份的CS葡萄酒品种,葡萄酒中水的氧-18值差异更大,范围从1.89(2004年)至5.35‰(2003年)。这种差异可以用2003年和2004年不同的年平均温度来解释。