From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection     

M. M. Bisi  A. R. Breen  B. V. Jackson  R. A. Fallows  A. P. Walsh  Z. Mikić  P. Riley  C. J. Owen  A. Gonzalez-Esparza  E. Aguilar-Rodriguez  H. Morgan  E. A. Jensen  A. G. Wood  M. J. Owens  M. Tokumaru  P. K. Manoharan  I. V. Chashei  A. S. Giunta  J. A. Linker  V. I. Shishov  S. A. Tyul’bashev  G. Agalya  S. K. Glubokova  M. S. Hamilton  K. Fujiki  P. P. Hick  J. M. Clover  B. Pintér 《Solar physics》2010,265(1-2):49-127

We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environment and upper Earth atmosphere. The interplanetary CME (ICME) impacted the Earth’s magnetosphere and caused the most-intense geomagnetic storm of 2005 with a Disturbed Storm Time (Dst) index reaching ?263 nT at its peak. The terrestrial environment responded to the storm on a global scale. We have combined observations and measurements from coronal and interplanetary remote-sensing instruments, interplanetary and near-Earth in-situ measurements, remote-sensing observations and in-situ measurements of the terrestrial magnetosphere and ionosphere, along with coronal and heliospheric modelling. These analyses are used to trace the origin, development, propagation, terrestrial impact, and subsequent consequences of this event to obtain the most comprehensive view of a geo-effective solar eruption to date. This particular event is also part of a NASA-sponsored Living With a Star (LWS) study and an on-going US NSF-sponsored Solar, Heliospheric, and INterplanetary Environment (SHINE) community investigation.  相似文献   

Relationships between land use and stream invertebrate community structure in a South Island,New Zealand,coastal stream catchment     

Matthew J. Hall  Gerard P. Closs  Ralph H. Riley 《新西兰海洋与淡水研究杂志》2013,47(3):591-603

Macroinvertebrate community composition was compared across streams draining catchments dominated by either native bush, agricultural or urban land uses within the Water of Leith stream catchment near Dunedin, New Zealand. Land use was associated with differences in taxon richness and faunal composition of communities present in each stream. The mean abundance levels of Ephemeroptera, Plecoptera, and Trichoptera were highest in native bush catchments, and lowest in urban catchments. In contrast, the mean abundance of Oligochaeta exhibited the opposite pattern. Increasing dominance of the urban and agricultural streams by pollution tolerant taxa was reflected in the Macroinvertebrate Community Index and Quantitative Macroinvertebrate Community Index scores.  相似文献   

Studying geoengineering with natural and anthropogenic analogs     

Alan Robock  Douglas G. MacMartin  Riley Duren  Matthew W. Christensen 《Climatic change》2013,121(3):445-458

Solar radiation management (SRM) has been proposed as a possible option for offsetting some anthropogenic radiative forcing, with the goal of reducing some of the associated climatic changes. There are clearly significant uncertainties associated with SRM, and even small-scale experiments that might reduce uncertainty would carry some risk. However, there are also natural and anthropogenic analogs to SRM, such as volcanic eruptions in the case of stratospheric aerosol injection and ship tracks in the case of marine cloud albedo modification. It is essential to understand what we can learn from these analogs in order to validate models, particularly because of the problematic nature of outdoor experiments. It is also important to understand what we cannot learn, as this might better focus attention on what risks would need to be solely examined by numerical models. Stratospheric conditions following a major volcanic eruption, for example, are not the same as those to be expected from intentional geoengineering, both because of confounding effects of volcanic ash and the differences between continuous and impulsive injection of material into the stratosphere. Nonetheless, better data would help validate models; we thus recommend an appropriate plan be developed to better monitor the next large volcanic eruption. Similarly, more could be learned about cloud albedo modification from careful study not only of ship tracks, but of ship and other aerosol emission sources in cloud regimes beyond the narrow conditions under which ship tracks form; this would benefit from improved satellite observing capabilities.  相似文献   

A Multi-Observatory Inter-Comparison of Line-of-Sight Synoptic Solar Magnetograms     

P. Riley  M. Ben-Nun  J. A. Linker  Z. Mikic  L. Svalgaard  J. Harvey  L. Bertello  T. Hoeksema  Y. Liu  R. Ulrich 《Solar physics》2014,289(3):769-792

The observed photospheric magnetic field is a crucial parameter for understanding a range of fundamental solar and heliospheric phenomena. Synoptic maps, in particular, which are derived from the observed line-of-sight photospheric magnetic field and built up over a period of 27 days, are the main driver for global numerical models of the solar corona and inner heliosphere. Yet, in spite of 60 years of measurements, quantitative estimates remain elusive. In this study, we compare maps from seven solar observatories (Stanford/WSO, NSO/KPVT, NSO/SOLIS, NSO/GONG, SOHO/MDI, UCLA/MWO, and SDO /HMI) to identify consistencies and differences among them. We find that while there is a general qualitative consensus, there are also some significant differences. We compute conversion factors that relate measurements made by one observatory to another using both synoptic map pixel-by-pixel and histogram-equating techniques, and we also estimate the correlation between datasets. For example, Wilcox Solar Observatory (WSO) synoptic maps must be multiplied by a factor of 3?–?4 to match Mount Wilson Observatory (MWO) estimates. Additionally, we find no evidence that the MWO saturation correction factor should be applied to WSO data, as has been done in previous studies. Finally, we explore the relationship between these datasets over more than a solar cycle, demonstrating that, with a few notable exceptions, the conversion factors remain relatively constant. While our study was able to quantitatively describe the relationship between the datasets, it did not uncover any obvious “ground truth.” We offer several suggestions for how this may be addressed in the future.  相似文献   

The radio source population at high frequency: follow-up of the 15-GHz 9C survey     

R. C. Bolton  G. Cotter  G. G. Pooley  J. M. Riley  E. M. Waldram  C. J. Chandler  B. S. Mason  T. J. Pearson  A. C. S. Readhead 《Monthly notices of the Royal Astronomical Society》2004,354(2):485-521

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An ion-exchange technique for concentrating ammonia from small volumes of seawater     

Ronald T. Riley  Michael C. Mix 《Marine Chemistry》1981,10(2):159-164

An ion-exchange technique was used to concentrate ammonia from seawater. Precipitation of bivalent cations, prior to concentration, reduced the variability of ammonia recovery from the ion-exchange column and lengthened column life. Analysis of the eluate was by the phenolhypochlorite reaction. The method was designed for use with small seawater samples (>10ml) and has the advantage that it can be adapted for use with small volumes of seawater with no loss in sensitivity. In a 10 ml seawater example NH₃-N concentrations of 10–150 μg l^?1 were accurately determined.  相似文献   

The relationship between star formation rate and radio synchrotron luminosity at 0 < z < 2     

Timothy Garn  David A. Green  Julia M. Riley  Paul Alexander 《Monthly notices of the Royal Astronomical Society》2009,397(2):1101-1112

We probe the relationship between star formation rate (SFR) and radio synchrotron luminosity in galaxies at  0 < z < 2  within the northern Spitzer Wide-area Infrared Extragalactic survey (SWIRE) fields, in order to investigate some of the assumptions that go into calculating the star formation history of the Universe from deep radio observations. We present new 610-MHz Giant Metrewave Radio Telescope (GMRT) observations of the European Large-Area ISO Survey-North 2 (ELAIS-N2) field, and using this data, along with previous GMRT surveys carried out in the ELAIS-N1 (North 1) and Lockman Hole regions, we construct a sample of galaxies which have redshift and SFR information available from the SWIRE survey. We test whether the local relationship between SFR and radio luminosity is applicable to   z = 2  galaxies, and look for evolution in this relationship with both redshift and SFR in order to examine whether the physical processes which lead to synchrotron radiation have remained the same since the peak of star formation in the Universe. We find that the local calibration between radio luminosity and star formation can be successfully applied to radio-selected high-redshift, high-SFR galaxies, although we identify a small number of sources where this may not be the case; these sources show evidence for inaccurate estimations of their SFR, but there may also be some contribution from physical effects such as the recent onset of starburst activity, or suppression of the radio luminosity within these galaxies.  相似文献   

Local responses to changed circumstances: Coalmining in the market economy in Upper Silesia, Poland     

Ray Riley  Maria Tkocz 《GeoJournal》1999,48(4):279-290

It is argued that the emphasis of much recent research into coalmining has been placed on international and national scale influences which affect coalfields as a whole; change at the intra-coalfield scale has received less attention. After providing a background to events in Poland during communism, attention focuses on developments since 1989, commencing with coalfield-wide influences. There follows an examination of the work of the state body Państwowa Agencja Węgla Kamiennego, which executes government policy at the local level, and whose membership is drawn from the coalfield region. This agency recommends the closure and amalgamation of mines, but otherwise rationalisation measures are left to the seven mining companies and the colliery managers. The restructuring which has been carried out is considered under five heads: organisational change within the collieries, employment, production and technical change, and ecological adjustment. While recognising the importance of the socioeconomic and political environment and geology, there is much evidence to suggest that intra-coalfield patterns are strongly determined by local decision-makers. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

A Snapshot of the Sun Near Solar Minimum: The Whole Heliosphere Interval     

Barbara J. Thompson  Sarah E. Gibson  Peter C. Schroeder  David F. Webb  Charles N. Arge  Mario M. Bisi  Giuliana de Toma  Barbara A. Emery  Antoinette B. Galvin  Deborah A. Haber  Bernard V. Jackson  Elizabeth A. Jensen  Robert J. Leamon  Jiuhou Lei  Periasamy K. Manoharan  M. Leila Mays  Patrick S. McIntosh  Gordon J. D. Petrie  Simon P. Plunkett  Liying Qian  Peter Riley  Steven T. Suess  Munetoshi Tokumaru  Brian T. Welsch  Thomas N. Woods 《Solar physics》2011,274(1-2):29-56

We present an overview of the data and models collected for the Whole Heliosphere Interval, an international campaign to study the three-dimensional solar?Cheliospheric?Cplanetary connected system near solar minimum. The data and models correspond to solar Carrington Rotation 2068 (20 March??C?16 April 2008) extending from below the solar photosphere, through interplanetary space, and down to Earth??s mesosphere. Nearly 200 people participated in aspects of WHI studies, analyzing and interpreting data from nearly 100 instruments and models in order to elucidate the physics of fundamental heliophysical processes. The solar and inner heliospheric data showed structure consistent with the declining phase of the solar cycle. A closely spaced cluster of low-latitude active regions was responsible for an increased level of magnetic activity, while a highly warped current sheet dominated heliospheric structure. The geospace data revealed an unusually high level of activity, driven primarily by the periodic impingement of high-speed streams. The WHI studies traced the solar activity and structure into the heliosphere and geospace, and provided new insight into the nature of the interconnected heliophysical system near solar minimum.  相似文献   

A new device for use in crushing rigid biomass and geological materials prior to compositional analysis     

Lance W. Riley  Shirley M. Baker  Edward J. Phlips 《Journal of Paleolimnology》2010,44(2):737-739

Traditional preparation of rigid material for compositional analysis has involved time-consuming and physically demanding grinding processes, such as the use of mortar and pestle. This paper describes a simple and relatively inexpensive new device capable of quickly, safely, and efficiently pulverizing rigid and brittle biomass material, or geologic materials, such as rock and sediment. The high sample recovery obtained with this device is comparable to that achieved by much more expensive analytical equipment.  相似文献