Lithologic control of debris torrent occurrence   总被引：1，自引：0，他引：1  

Shannon Sterling  Olav Slaymaker 《Geomorphology》2007,86(3-4):307-319

A field-based investigation into the frequency and magnitude of debris torrent systems reveals that lithology controls the spatial and temporal occurrence of debris torrents in the Tsitika Watershed, Vancouver Island, British Columbia. We identified 125 debris torrent systems in the watershed; for half these basins we used dendrochronology, historical air photographs, and field surveys to estimate debris torrent frequency and magnitude for a 30 year period. We find that the volcaniclastic half of the watershed contains more than twice as many debris torrent systems, in which debris torrents occur over seven times more frequently, and the deposits have a higher rate of delivery of sediment to the mainstem river than the intrusive half. Lithologic differences in weathering rates, weathering product grain size, and rock texture can explain the observed differences in debris torrent behaviour. Because debris torrents are the main sediment transport path from hilltop to valley bottom in the region, these results confirm an important lithologic control on regional sediment transport. While the exact numbers are uncertain, we estimate that the sediment flux of volcaniclastic debris torrents in the watershed is five times higher than that of the intrusive debris torrents.  相似文献   

Standardizing catch rates: is logbook information by itself enough?     

Bishop  J.; Venables  W. N.; Dichmont  C. M.; Sterling  D. J. 《ICES Journal of Marine Science》2008,65(2):255-266

  相似文献   

Simple mass distribution for the lunar potential     

Sterling L. Levie Jr. 《Earth, Moon, and Planets》1971,3(3):315-325

A set of twenty-one point masses gravitationally equivalent to the L1 lunar potential model is presented. By construction, the equivalence is valid only in a region of space sampled by Apollo spacecraft. That region is taken to be a finite, torus-shaped shell. When used in place of the L1 model for Apollo 12 lunar orbit determination, the solution set gives spacecraft positions identical to within about 100 m.The solution is developed in two steps: first the L1 potential is examined to determine favorable mass locations, and then the mass values are computed to force an optimum matching of the L1 potential. Therefore the solution set is artificial. It is related to the Moon's actual mass distribution only in its similar gravitational effects in a limited region of space.  相似文献   

The Global Context of Solar Activity During the Whole Heliosphere Interval Campaign     

D. F. Webb  H. Cremades  A. C. Sterling  C. H. Mandrini  S. Dasso  S. E. Gibson  D. A. Haber  R. W. Komm  G. J. D. Petrie  P. S. McIntosh  B. T. Welsch  S. P. Plunkett 《Solar physics》2011,274(1-2):57-86

The Whole Heliosphere Interval (WHI) was an international observing and modeling effort to characterize the 3-D interconnected ??heliophysical?? system during this solar minimum, centered on Carrington Rotation 2068, March 20??C?April 16, 2008. During the latter half of the WHI period, the Sun presented a sunspot-free, deep solar minimum type face. But during the first half of CR 2068 three solar active regions flanked by two opposite-polarity, low-latitude coronal holes were present. These departures from the quiet Sun led to both eruptive activity and solar wind structure. Most of the eruptive activity, i.e., flares, filament eruptions and coronal mass ejections (CMEs), occurred during this first, active half of the interval. We determined the source locations of the CMEs and the type of associated region, such as active region, or quiet sun or active region prominence. To analyze the evolution of the events in the context of the global solar magnetic field and its evolution during the three rotations centered on CR 2068, we plotted the CME source locations onto synoptic maps of the photospheric magnetic field, of the magnetic and chromospheric structure, of the white light corona, and of helioseismological subsurface flows. Most of the CME sources were associated with the three dominant active regions on CR 2068, particularly AR 10989. Most of the other sources on all three CRs appear to have been associated with either isolated filaments or filaments in the north polar crown filament channel. Although calculations of the flux balance and helicity of the surface magnetic features did not clearly identify a dominance of one region over the others, helioseismological subsurface flows beneath these active regions did reveal a pronounced difference among them. These preliminary results suggest that the ??twistedness?? (i.e., vorticity and helicity) of subsurface flows and its temporal variation might be related to the CME productivity of active regions, similar to the relationship between flares and subsurface flows.  相似文献   

Psychological sequels of flood on residents of southeast Caspian region     

Hesam Seyedin  Reza HabibiSaravi  Nasrin sayfouri  Vahid Hoseini Djenab  Fariba Ghasemi Hamedani 《Natural Hazards》2017,88(2):965-975

Flood is the most common disaster in the world and has acute or chronic health consequences including psychological sequels. Post-traumatic stress disorder (PTSD) is one of the main consequences. This study aimed to explore the psychological impacts (PTSD) in two flooded cities of Mazandaran Province, Neka and Behshahr, in the southeastern Caspian region that experienced flooding in 2012. A cross-sectional community-based study was performed on randomly selected samples of 400 individuals using GIS-based sampling from 139931 residents of the two flooded cities. The PTSS-10 questionnaire was used for data collection. The results showed that the overall stress disorder mean score among the participants was 2.59 out of 6. PTSD prevalence in the affected population was 64%. It was also found that stress scores significantly increased in younger people, male gender, the divorced, the widows or the widowers, and those who lost their properties (p < 0.05). Study findings showed that flood is a considerable stressor which develops PTSD. This finding should be taken into account in all four phases of disaster management cycle, and subsequently, specialized post-disaster mental health services must be provided for the afflicted population.  相似文献   

Geochemical and quality assessment of groundwater of Marand Basin, East Azarbaijan Province, northwestern Iran   总被引：2，自引：2，他引：0  

Kaveh Pazand  Ardeshir Hezarkhani  Yousef Ghanbari  Nasrin Aghavali 《Environmental Earth Sciences》2012,67(4):1131-1143

The chemical analysis of 83 water wells in the Marand area, Azarbaijan Province NW of Iran was evaluated to determine the hydrogeochemical processes and ion concentration background in the region. Over the entire area, the dominated hydrochemical types are Ca? +?Mg?+?SO₄?+?Cl, Ca?+?SO₄, Na?+?Cl and Ca?+?Mg?+?HCO₃. Based on the total hardness, the softness of the groundwater is determined. According to electrical conductivity (EC) and sodium adsorption ratio (SAR), the most dominant classes are C3?CS1, C3?CS2, C4?CS2 and C2?CS1. The major ion concentrations are below the acceptable level for drinking water. The groundwater salinity hazard is medium to high, but the Na hazard is low to medium; with regard to irrigation water, the quality is low to medium. So, a drainage system is necessary to avoid the increase of toxic salt concentrations.  相似文献   

Visibility and Origin of Compact Interplanetary Radio Type IV Bursts     

Nasrin Talebpour Sheshvan  Silja Pohjolainen 《Solar physics》2018,293(11):148

We have analyzed radio type IV bursts in the interplanetary (IP) space at decameter–hectometer (DH) wavelengths to determine their source origin and a reason for the observed directivity. We used radio dynamic spectra from the instruments on three different spacecraft, STEREO-A, Wind, and STEREO-B, which were located approximately 90 degrees apart from each other in 2011?–?2012, and thus gave a 360 degree view of the Sun. The radio data were compared to white-light and extreme ultraviolet (EUV) observations of flares, EUV waves, and coronal mass ejections (CMEs) in five solar events. We find that the reason that compact and intense DH type IV burst emission is observed from only one spacecraft at a time is the absorption of emission in one direction and that the emission is blocked by the solar disk and dense corona in the other direction. The geometry also makes it possible to observe metric type IV bursts in the low corona from a direction where the higher-located DH type IV emission is not detectable. In the absorbed direction we found streamers, and they were estimated to be the locations of type II bursts, caused by shocks at the CME flanks. The high-density plasma was therefore most probably formed by shock–streamer interaction. In some cases, the type II-emitting region was also capable of stopping later-accelerated electron beams, which were visible as type III bursts that ended near the type II burst lanes.  相似文献   

Predictive value of Keetch-Byram Drought Index for cereal yields in a semi-arid environment     

Nasrin?Salehnia  Hossein?ZareEmail authorView author&#;s OrcID profile  Sohrab?Kolsoumi  Mohammad?Bannayan 《Theoretical and Applied Climatology》2018,131(3-4):1005-1018

The study examines the potential of urban roofs to reduce the urban heat island (UHI) effect by changing their reflectivity and implementing vegetation (green roofs) using the example of the City of Vienna. The urban modelling simulations are performed based on high-resolution orography and land use data, climatological observations, surface albedo values from satellite imagery and registry of the green roof potential in Vienna. The modelling results show that a moderate increase in reflectivity of roofs (up to 0.45) reduces the mean summer temperatures in the densely built-up environment by approximately 0.25 °C. Applying high reflectivity materials (roof albedo up to 0.7) leads to average cooling in densely built-up area of approximately 0.5 °C. The green roofs yield a heat load reduction in similar order of magnitude as the high reflectivity materials. However, only 45 % of roof area in Vienna is suitable for greening and the green roof potential mostly applies to industrial areas in city outskirts and is therefore not sufficient for substantial reduction of the UHI effect, particularly in the city centre which has the highest heat load. The strongest cooling effect can be achieved by combining the green roofs with high reflectivity materials. In this case, using 50 or 100 % of the green roof potential and applying high reflectivity materials on the remaining surfaces have a similar cooling effect.  相似文献   

Quantifying the reliability of four global datasets for drought monitoring over a semiarid region     

Pari-Sima Katiraie-Boroujerdy  Nasrin Nasrollahi  Kuo-lin Hsu  Soroosh Sorooshian 《Theoretical and Applied Climatology》2016,123(1-2):387-398

  相似文献   

Notes on the Cambrian Area of Comley     

Edgar Sterling Cobbold 《Proceedings of the Geologists' Association. Geologists' Association》1925,36(4):367-376

  相似文献