COMMUNITY GARDENS AND POLITICS OF SCALE IN NEW YORK CITY*

ABSTRACT. New York City community gardens have been the subject of political contestation over the course of their thirty‐year existence. In 1999, 114 gardens were slated for public auction and redevelopment. This article examines the controversy over the garden auction as a politics of scale in which garden advocates successively raised the scope of the controversy beyond the scale of individual gardens, and ultimately beyond that of the city. Analysis of this land‐use conflict highlights the significance of politics of scale for grassroots organizations within a market‐centric, neoliberal economic framework.     

The phosphates of IIIAB iron meteorites

Abstract— Thirteen phosphate minerals are found in IIIAB iron meteorites. Four of these (sarcopside, graftonite, johnsomervilleite, and galileiite) constitute the majority of occurrences. The IIIB iron meteorites are confined to occurrences of only these four phosphates. The IIIA iron meteorites may contain one or more of these four phases; they may also contain other rarer phosphates, and silica (in two instances) and a silicate rock (in one instance). Thus, the IIIA lithophile chemistry is more varied than that of the IIIB meteorites. Based on petrographic relations, sarcopside appears to be the first phosphate to form. Graftonite is probably formed by recrystallization of sarcopside. Johnsomervilleite and galileiite exsolved as enclaves in sarcopside or graftonite at lower temperatures, although some of these also nucleated as separate crystals. The IIIAB phosphates are carriers of a group of incompatible lithophile elements: Fe, Mn, Na, Ca, and K, and, rarely, Mg as well as Pb. These elements (and O) were concentrated in a residual, S-rich liquid during igneous fractional crystallization of the IIIAB core mass. The phosphates formed by oxidation of P as the core solidified and excluded O, which increased its partial pressure in the residual liquid. The trace siderophile trends in bulk IIIAB metal are paralleled by a mineralogical trend of the phosphate minerals that formed. For IIIAB meteorites with low-Ir contents in the metal, the phosphates are mainly Fe-Mn phases; at intermediate Ir values, more Na-bearing phosphates appear; at the highest Ir values, the rarer Na-, K-, Mg-, Cr-, and Pb-bearing phosphates appear. The absence of significant amounts of Mg, Si, Al, and Ti suggest depletion of these elements in the core by the overlying mantle.     

WILDLIFE CONSERVATION AND BAMBOO MANAGEMENT IN CHINA'S SOUTHEAST UPLANDS*

ABSTRACT. The subtropical forests, grasslands, and wetlands of Southeast China's Wuyi‐Daiyun Mountain Range provide essential habitats for diverse wildlife, including a dwindling population of tigers. Three primary protected areas, the Meihuashan, Wuyishan, and Longxishan Nature Reserves, contain varied wildlife habitats and also provide natural resources for 7,000 people in several dozen villages. A field‐based study of land use and habitat quality in these reserves shows that anthropogenic bamboo forests are among the least valuable habitats for wildlife but that, as the primary source of household income, bamboo monoculture is spreading rapidly and replacing habitats of greater ecological value. Although authorities in Meihuashan have demarcated the many broadleaf forest patches for strict protection, household income and bamboo‐management research in all three reserves suggests that successful habitat conservation may ultimately depend on more equitable systems of land tenure, improved cooperative cottage industries, and greater local economic diversification.     

对逆冲断层一些普遍观念的质疑──以美国西部科迪勒拉及中国华北的野外研究为例(英文)

在过去的25年里,由于许多原因,作为最常见、分布也最广泛的地质构造形迹之一,逆冲断层成为倍受关注的科学研究主题。文中指出,关于逆冲断层及其几何学特征的许多普遍认识（或观念）,并不像以往文献中所阐述的那样简单。其中之一的"薄皮"冲断构造是受地层控制的,极少有或者没有结晶基底物的卷入。文中主张,"薄皮"一词只有逆冲板片的几何学形态含义,而不应包含地层意义,并列举了一些完全由结晶岩石所构成的薄皮逆冲构造的例子来说明这一主张。近来,逆冲双重构造成为构造文献中的热点。关于逆冲双重构造的成因,引用得最多的是1982年Boyer和Elliot在其重要论文"逆冲断层系统"中所作的解释。他们认为,双重道冲构造是通过在冲断坡底部发生下盘破裂。新生断裂不断向前扩展并进入先存断层下盘的一系列变形过程中逐渐形成的。根据Boyer和Elliot提出的这种变形过程,将形成一个具有平面状顶板断层的边冲双重构造,这个顶板断层只在活动断坡的顶部是主动向前扩展的。依笔者之见,在实际的构造变形当中,是不可能具备形成平顶过冲双重构造的地质条件的。而能对平顶过冲双重构造形成作出最好解释的是反序（out－of－sequence,OOS）边冲断层的发育,即断层向着主冲断层的后方发展,在先存道冲构造的上部?     

恒山中元古代早期基性岩墙群的单颗粒锆石U—Pb年龄及其克拉通构造演化意义

华北克拉通中北部变质基底发育大规模的前寒武纪基性岩墙群,由于基性岩墙同位素定年技术存在问题,因此一直未获得岩墙群的确切年龄数据。本文利用单颗粒锆石U-Pb化学法,首次获得恒山地区北西向基性岩墙群的U-Pb年龄为1769.1±2.5Ma,并证明它代表基性岩墙群的侵位年龄,这一年龄数据也是华北克拉通大规模分布的未变质基性岩墙群已知的最古老年龄。综合分析同期岩浆活动的同位素年龄记录,本文提出中元古代早期华北的岩浆侵位发生于伸展构造背景下。     

Monazite-Xenotime Thermochronometry and Al2SiO5 Reaction Textures in the Picuris Range, Northern New Mexico, USA: New Evidence for a 1450-1400 Ma Orogenic Event

Al₂SiO₅ reaction textures in aluminous schist and quartziteof the northern Picuris range, north-central New Mexico, recorda paragenetic sequence of kyanite to sillimanite to andalusite,consistent with a clockwise P–T loop, with minor decompressionnear the Al₂SiO₅ triple-point. Peak metamorphic temperaturesare estimated at 510–525°C, at 4·0–4·2kbar. Kyanite and fibrolite are strongly deformed; some prismaticsillimanite, and all andalusite are relatively undeformed. Monaziteoccurs as inclusions within kyanite, mats of sillimanite andcentimetre-scale porphyroblasts of andalusite, and is typicallyaligned subparallel to the dominant regional foliation (S₀/S₁or S₂) and extension lineation (L₁). Back-scatter electron imagesand X-ray maps of monazite reveal distinct core, intermediateand rim compositional domains. Monazite–xenotime thermometryfrom the intermediate and rim domains yields temperatures of405–470°C (±50°C) and 500–520°C(±50°C), respectively, consistent with the progradeto peak metamorphic growth of monazite. In situ, ion microprobeanalyses from five monazites yield an upper intercept age of1417 ± 9 Ma. Near-concordant to concordant analyses yield²⁰⁷Pb–²⁰⁶Pb ages from 1434 ± 12 Ma (core) to 1390± 20 Ma (rim). We find no evidence of older regionalmetamorphism related to the 1650 Ma Mazatzal Orogeny. KEY WORDS: Al₂SiO₅; metamorphism; monazite; thermochronometry; triple-point     

Multiple generations of hibonite in spinel-hibonite inclusions from Murchison

Abstract— Through freeze-thaw disaggregation of the Murchison meteorite, we have recovered, in addition to many spinel-hibonite spherules, several hibonite-rich inclusion fragments in which the hibonite has wider ranges in TiO₂ contents (e.g., 0.07–8.6 wt% in one inclusion and 2–10 wt% in another) than previously observed within single inclusions. In these inclusions, there are sharp contacts between texturally early, Ti-poor hibonite and relatively late, Ti-rich hibonite, and the two types occur in complex intergrowth textures that are not consistent with crystallization from a melt in a single-stage cooling event. One inclusion has, in addition to relatively TiO₂-rich hibonite, some that is virtually TiO₂-free but contains ～1 wt% MgO and ～1.5 wt% SiO₂. Instead of the common substitution of Mg + Ti for 2Al, Mg coupled with Si in this case, probably reflecting crystallization from an unusual, Ti-free silicate liquid. Ion microprobe analyses of Ti-rich and Ti-poor hibonite from this inclusion yield quite similar trace-element patterns and Mg-isotopic compositions. The results are most consistent with formation of Ti-rich hibonite from Ti-poor hibonite by addition of Mg and Ti to the latter by exchange with a hot, Ti-rich liquid. That this occurred without a resolvable change in the Mg-isotopic composition requires that the Ti-rich, second generation of hibonite formed <2.5 times 10⁵ yr later than the Ti-poor hibonite. Observations of spinel-hibonite spherules and spherule fragments in our sample suite provide additional evidence that, despite the claims by Greenwood et al. (1994), spinel-hibonite spherules crystallized from individual, molten droplets, as earlier suggested by Macdougall (1981) and MacPherson et al. (1983).