Study of an Extended EUV Filament Using SoHO/SUMER Observations of the Hydrogen Lyman Lines

A?filament and its channel close to the solar disk were observed in the complete hydrogen Lyman spectrum, and in several EUV lines by the SUMER (Solar Ultraviolet Measurement of Emitted Radiation) and CDS (Coronal Diagnostic Spectrometer) spectrographs on the SoHO satellite, and in H?? by ground-based telescopes during a multi-instrument campaign in May 2005. It was a good opportunity to get an overview of the volume and the density of the cold plasma in the filament channel; these are essential parameters for coronal mass ejections. We found that the width of the filament depends on the wavelength in which the filament is observed (around 15?arcsec in H??, 30?arcsec in L??, and 60?arcsec in EUV). In L?? the filament is wider than in H?? because cool plasma, not visible in H??, is optically thick at the L?? line center, and its presence blocks the coronal emission. We have derived physical plasma properties of this filament fitting the Lyman spectra and H?? profiles by using a 1D isobaric NLTE model. The vertical temperature profile of the filament slab is flat (T??7000?K) with an increase to ???20?000?K at the top and the bottom of the slab. From an analysis of the L?? and H?? source functions we have concluded that these lines are formed over the whole filament slab. We have estimated the geometrical filling factor in the filament channel. Its low value indicates the presence of multi-threads.     

The 10Be deglaciation chronology of the Göschenertal,central Swiss Alps,and new insights into the Göschenen Cold Phases

The Göschenertal (Göschenen valley) is the type locality of the so‐called Göschenen Cold Phases I (~3–2.3 ka) and II (~1.8–1.1 ka). According to earlier studies, these Late Holocene climatic cooling periods were characterized by changes in vegetation and pronounced glacier advances. As a peculiarity, the Göschenen Cold Phase I was thought to be connected to a local surge‐type advance of the Chelengletscher (Chelen glacier) – an exceptional event of unparalleled dimension in the European Alps. Based on cosmogenic ¹⁰Be exposure ages from moraine boulders, we investigated the local glacier chronology. In contrast to former research, moraines at different positions within the Göschenen valley (central Swiss Alps) have been dated to the Younger Dryas and the Early Holocene. This questions the applicability of palaeo‐Equilibrium Line Altitude (ELA) calculations for stadial attributions without additional numerical age constraints. Furthermore, we have found compelling evidence that the proposed non‐climatic glacier advance attributed to the Göschenen Cold Phase I did not occur. The present results, along with a reappraisal of the original study, question the scientific reliability and the glaciological definition of the Göschenen Cold Phases as glacier advances that clearly exceeded the Little Ice Age positions. While our data do not exclude potential changes in climate and vegetation, we nonetheless show that the Göschenen Cold Phases are not suitable as reference stadials in the system of Alpine Holocene glacier fluctuations.     

Measurement of Mass-Independent Perturbations of Cadmium in Nuclear Debris Samples

The isotopic composition of cadmium in nuclear debris was measured by multi-collector inductively coupled plasma-mass spectrometry (MC-ICP-MS). Mass-independent perturbations due to fission product decay on the isotopes of Cd were observed. Relative fission yields for masses 111, 112, 114 and 116 were determined in each sample of nuclear debris and compared with reported values found in irradiated plutonium and uranium fuels. Mass spectrometry measurements of the valley fission product endpoints are extremely challenging due to the low cumulative fission yields and small amounts of each isotope that are produced. To overcome these challenges, a new purification method for Cd was developed and validated by examination of a number of geological reference materials.     

Major Breakthroughs in Geological Theory,Key Techniques and Exploration of Tight Oil in China

正In recent years,U.S.tight oil exploration and development have achieved significant progress,with rapidly increasing production,which has significantly changed the U.S.A.energy supply pattern(Fig.1).Compared with the North American marine to marginal marine-continental transitional facies,China’s tight oil(Fig.1)     

CZChemDB and EarthChem: Advancing management and access of critical zone geochemical data

Multiple Critical Zone Observatories (CZO) have been established in recent years in the USA and other international settings to conduct collaborative research on processes that occur at and near Earth’s surface, also known as the Critical Zone (CZ). Data documentation and data sharing are two persistent problems facing the CZOs that impede the ability for cross-site comparisons and integrated analysis. In this study, a relational database was developed for CZ rock and regolith geochemical data – CZChemDB. There are a total of 24 interrelated tables in the database, each representing different aspects of CZ features. The main data group includes tables of locations, sites, samples, subsamples, preparation/treatments, laboratory-analysis and data values. The meta-data group includes tables of methods, references, and data quality. Lookup tables (variables, units, etc.) contain lists of “controlled” vocabularies. The CZChemDB is currently implemented in the MS Access database management system. It is expected to be integrated into the EarthChem portal by summer of 2011 for broader online accessibility and usability. This integration also complements the EarthChem’s global geochemistry database with CZ regolith data. The structure of the CZChemDB is simple, straightforward, and flexible so that it has potential to accommodate other chemical data collected from CZOs, such as pore fluid data. Furthermore, the development of CZChemDB represents the first attempt toward the standardization of geochemical data documentation and data sharing among CZOs. This effort will establish a model to bridge the connections between data acquisition, data management, data sharing, and data searching/discovering that are all essential but weak in terms of linkages within most geoscience research projects.     

Community Development Approaches to Heart Health Promotion: A Geographical Perspective

This paper reports results of a qualitative study of community development approaches to heart health promotion in Ontario. Cardiovascular disease (CVD) represents a substantial proportion of the burden of illness experienced by western industrialized countries. Biomedical research has implicated lifestyle choices and socioeconomic conditions as primary determinants of CVD. There has been a resultant shift from curative to preventive/health promoting strategies to reduce this burden of illness. The Canadian Heart Health Initiative-Ontario Project (CHHIOP), a two-stage (quantitative and qualitative) longitudinal study, was designed to address issues of heart health promotion through the investigation and strengthening of community-based heart health activities in both the formal and informal public health systems. The study reported on in this paper forms one part of the qualitative stage and focuses on how community relationships and community development approaches play out in local contexts to shape the reality of (heart) health promotion practice. Analysis of key informant interviews using Ethnograph illustrates the centrality of community context, the lack of a common understanding of key concepts (e.g., community development), and the emergence of a shift in health agencies' ways of doing business characterized by increased partnering and collaboration in the delivery of (heart) health promotion programs. Local perspectives and the dynamics of intra-community relations were allowed to emerge through the use of qualitative approaches implying a need for place-sensitive (heart) health promotion strategies.     

1300 micron continuum and C18O line mapping of the giant molecular cloud cores in Orion, W49, and W51

We present observations of the 1300 micron continuum emission and the C18O spectral-line emission from three well-studied giant molecular cloud cores: Orion, W49, and W51. The observations were obtained at the Five College Radio Astronomy Observatory, and they provide a means to examine the consistency of these two methods to trace the column density structure of molecular clouds. We find a good general correlation between the 1300 micron continuum, which traces the column density of dust, and the C18O J = 2 --> 1 line emission, which traces the column density of molecular gas, when the effects of source temperature are taken into consideration. Moreover, nominal values for the gas and dust abundances and the dust properties reproduce the observed continuum-to-line ratios. Thus, no strong C18O abundance gradients within sources has been found, and it appears that either the C18O emission lines or the submillimeter dust emission may be used to derive the mass column density within molecular clouds accurately.     

Use of multi-point analysis and modelling to address cross-scale coupling in space plasmas: Lessons from Cluster

The properties of plasmas (in space) are fundamentally governed by both ‘cross-scale’ coupling and comparative temporal behaviour operating over the micro-, meso-, and (MHD-) fluid regimes: for example, under conditions of turbulence, during magnetic reconnection and in shocks and other plasma boundaries. These themes map to a number of related and overlapping, phenomena, where known phenomena play different roles in each theme. Detailed understanding of fundamental plasma processes therefore requires analysis of both theoretical models (to distinguish the collisionless from the collisional regimes) and multi-scale measurements (suitable to address issues of stationarity). In particular, the investigation of phenomena requires analysis techniques which can distinguish and quantify temporal behaviour and the multi-scale spatial behaviour. The analysis of existing, multi-point data sets has led to a number of data co-ordination methods, such as the four spacecraft analysis tools developed for cluster, and we consider examples here. Advanced analysis concepts may be investigated with suitable considerations of measurement quality:adequate sampling of phenomena (for example, to extract the necessary information on the mechanisms operating) requires suitable spacecraft configurations and directly relates to the measurement quality achievable. A particular issue is how to resolve temporal behaviour across the spatial regimes, so that the data set is suitably coordinated. With the addition of theoretical modelling (in the context of particular phenomena) both the space and laboratory plasma regimes may be compared and we give an example of nonlinear wave coupling across spatial scales in this context.     

RHESSI Data Analysis Software: Rationale and Methods

The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) performs imaging spectroscopy of the Sun with high spatial and spectral resolution from 3 keV to 17 MeV using indirect Fourier-transform techniques. We review the rationale behind the RHESSI data analysis software, and explain the underlying structure of the software tools. Our goal was to make the large data set available within weeks after the RHESSI launch, and to make it possible for any member of the scientific community to analyze it easily. This paper describes the requirements for the software and explores our decisions to use the SolarSoftWare and Interactive Data Language programming packages, to support both Windows and Unix platforms, and to use object-oriented programming. We also describe how the data are rapidly disseminated and how ancillary data sets are used to enhance the RHESSI science. Finally, we give a schematic overview of some of the data flow through the high-level analysis tools. More information on the data and analysis procedures can be found at the RHESSI Data Center website, http://hesperia.gsfc.nasa.gov/rhessidatacenter. Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1022444531435     

“Where is home?” Here and there: transnational experiences of home among Canadian migrants in the United States

Using structured telephone interviews this research focuses on how Canadian migrants living in the United States experience and describe home. We argue that the globalisation of peoples’ lives, transnationalism and the concomitant creation of transnational social spaces have greatly affected the meaning of home for migrants. The understandings of home that result reflect the reality of living in social worlds that span two countries and the development of decentred multiple attachments and feelings of belonging in more than one place. In response to these circumstances Canadian migrants experience home as multi-dimensional, pluri-local, and characterized by regular movement across the U.S.–Canada border. When asked specifically about feeling at home upon re-entry to the U.S. many respondents answered yes. However, many interviewees qualified their answers by describing home in different ways and associating different aspects of their lives with each country. Canada as home was most often described in terms of family, while home in the U.S. was associated with work. Respondents also differentiated between feeling at home once they reached their residence as opposed to feeling unwelcome at the U.S. border.