Prospecting in Ostia Antica (Italy) and the Discovery of the Basilica of Constantinus I. in 1996

H. Becker
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引用次数: 1

Abstract

Cooperation of Bavarian State Conservation Office. Department Archaeological Prospection and Aerial Archaeology (H. Becker). German Archaeological Institute Rome ( P. Zanker. M. Heinzelmann). Institute for Photogrametry and Remote Sensing Technical University Munich (M. Stephani. K. Eder. R. Brandt). Bayerische Akademie der Wissenschaften (Kommission zur Erforschung des antiken Stadtewesens) Munchen, Soprintendenza Archaeologica di Ostia (A. Galina Zevi). After the huge excavations in 1938 to 1942 in Ostia Antica. the ancient habour of Rome for the World Exhibition 1942 in Rome, there remained about 40 hectare of the area of the ancient city untouched. This is about 50 to 60% of the original built up area. On one hand the untouched area would be a chance for future research work in Ostia. at the other hand this was always a handicap for urbanistic research. The ideas about the building structure in some quarters of the city (regiones) as well as about the distribution and type of various buildings will be almost hypothetical. Even the location of some important buildings like the amphitheatre and the temple of Volcano are still unknown. Therefore the department Rome of the German Archaeological Institute began to organize a experimental project testing modern methods for archaeological prospecting for urbanistic research. The combination of aerial photo interpretation of several sources, digital terrain modelling and geophysical prospecting (caesium magnetometry and resistivity surveying) were applied on the base of the same coordinate system. An area of about 15 ha. the biggest untouched area, in regio V in the southeast of the ancient city was selected for a first test for geophysical prospecting in August 1996. The limits of this test area were chosen very close to the excavated parts of this regio. to the south and east it was spread far beyond the ancient city wall reaching the modern fence of the archaeological area. Hopefully in this area used as ploughed field for agriculture the archaeological structures should remained untouched and buried not very deeply. Considering the time of ten days only for this first test in August 1996 caesium magnetometry was applied only, because resistivity surveying seemed to slow for vast areas. The summer in 1996 was also very dry with temperatures sometimes above 36° Celsius (in the non-existing shadow), which would have caused severe electrical contact problems to the ground. After a very limited test for resistivity surveying in area where the basilica was found in 1997 there was a bigger area surveyed by resistivity methods in June 1998. which gave almost no additional information about the archaeology in the ground that could be seen already in the magnetograms. This was also the first test for a quadro-sensor caesium magnetometer system mounted on a non magnetic chariot ( the socalled "Magneto-Scanner"(Fig. 1). This new system consists of 4 caesium magnetometers Scintrex SMARTMAG SM4G-Special with quadro-sensor configuration. 2 gradiometcr consoles, data loggers, power supply (4 batteries 12V/6Ah). interface electronics and automatic distance trigger mounted on a nonmagnetic chariot, total weight about 50 kg. A fifth magnetometer can be used for compensating the daily magnetic variation synchronised in a variometer mode. The whole system (5 magnetometers and the chariot) can be packed into any normal personal car (there is no van necessary). The "Magneto-Scanner" had to be built up rather quickly to be ready for the test in Ostia within some weeks. Several persons and companies helped for this fast construction: The main part of this system was sponsered by the Bayerische Motorenwerke AG BMW. the nonmagnetic chariot was built by my brother Dr. Thomas Becker the construction was made during manufacturing and Scintrex (Canada) succeeded in fast delivery even for the modified sensor-systems SM4G-Special. Jorg Fassbinder helped solving many problems due to the interface electronics and the distance triggering and Rainer Appel succeeded finishing a software
1996年在奥斯蒂亚安蒂卡(意大利)的勘探和君士坦丁努斯大教堂的发现
巴伐利亚州自然保护办公室的合作。考古勘探和航空考古学系(H. Becker)。罗马德国考古研究所(P. Zanker)。m . Heinzelmann)。慕尼黑工业大学摄影与遥感研究所。k·埃德尔。r·勃兰特)。慕尼黑巴伐利亚科学研究院,奥地利奥地利考古研究所(A. Galina Zevi)。1938年到1942年在奥斯蒂亚安蒂卡进行了大规模的挖掘。为了1942年在罗马举行的世界博览会,罗马的古港口保留了大约40公顷的古城区域。这大约是原来建筑面积的50%到60%。一方面,这片未受破坏的地区将为奥斯蒂亚未来的研究工作提供机会。另一方面,这一直是城市研究的障碍。关于城市(地区)某些地区的建筑结构以及各种建筑的分布和类型的想法几乎是假设的。甚至一些重要的建筑,如圆形剧场和火山神庙的位置仍然未知。因此,德国考古研究所罗马部开始组织一个实验项目,测试城市研究中考古勘探的现代方法。在同一坐标系下,将多源航空照片解译、数字地形模拟和物探(铯磁、电阻率测量)相结合。面积约15公顷。1996年8月,在古城东南的V区选定了最大的未开发地区进行第一次地球物理勘探试验。这个试验区的边界选择得非常接近这个地区的挖掘部分。在南部和东部,它远远超出了古城墙,到达了考古区域的现代围栏。希望在这个被用作农业耕地的地区,考古结构应该保持原封不动,埋得不要很深。考虑到1996年8月的第一次测试只有10天的时间,只使用了铯磁强计,因为电阻率测量在广大地区似乎很慢。1996年的夏天也非常干燥,温度有时超过36摄氏度(在不存在的阴影中),这将导致严重的地面电接触问题。1997年在发现教堂的地区进行了非常有限的电阻率测量试验后,1998年6月又用电阻率法对更大的区域进行了测量。这几乎没有提供更多的关于地下考古的信息,这些信息可以从磁图中看到。这也是安装在非磁性战车上的四传感器铯磁力计系统的第一次测试(所谓的“磁扫描仪”)。1).该新系统由4个带有四轴传感器配置的Scintrex SMARTMAG SM4G-Special铯磁力计组成。2个梯度仪控制台,数据记录仪,电源(4节12V/6Ah电池)。接口电子和自动距离触发器安装在一个非磁性战车上,总重量约50公斤。第五磁力计可用于补偿以变差计模式同步的每日磁变化。整个系统(5个磁力计和战车)可以装进任何普通的个人汽车(没有必要的货车)。为了在几周内为奥斯蒂亚的测试做好准备,“磁扫描仪”必须相当快地组装起来。几个人和公司为这个快速建设提供了帮助:这个系统的主要部分是由巴伐利亚汽车公司宝马赞助的。非磁性战车是由我的兄弟托马斯·贝克尔博士建造的,建筑是在制造过程中制造的,Scintrex(加拿大)成功地快速交付,甚至修改了传感器系统SM4G-Special。Jorg Fassbinder帮助解决了接口电子和距离触发的许多问题,Rainer Appel成功地完成了一个软件
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