Carbon monoxide levels along roadway     

F. W. L. Kho B.Sc.  P. L. Law B.SCE.  M.SCE.  M.Sc.  Sc.D.  S. H. Ibrahim M.S.c  Ph.D.  J. Sentian B.Sc.  M.Sc. 《International Journal of Environmental Science and Technology》2007,4(1):27-34

This paper predicts and compares the carbon monoxide (CO) concentration levels along Sembulan Road for years 2004 and 2014 using CAL3QHC air dispersion model at two major locations, i.e., at Sembulan Roundabout and Sutera Harbour Intersection, Kota Kinabalu, Sabah, Malaysia. The CO concentration “hot-spots” were also identified at Sutera Harbour Intersection, and the highest maximum 1-hr average ground level concentrations of CO modeled for Kpg. Air Sembulan located in the northeast of idling road was 9.33 ppm for year 2004. This study showed that there would be no extreme changes in CO concentration trends for year 2014 although a substantial increase in the number of vehicles is assumed to affect the level of CO concentrations. It was also found that the CO levels would be well below the Malaysian Ambient Air Quality Guidelines of 30 ppm for 1-hour Time-Weighted Average (TWA). Comparisons between the modeled and observed outputs using quantitative data analysis technique and statistical methods indicated that the CAL3QHC predicted results correlated well with measured data. It was predicted that receptors located near to the major intersection, in the long-term would be potentially exposed to relatively higher CO levels.  相似文献   

Geothermal energy prospects in Brazil: A preliminary analysis     

V. M. Hamza  S. M. Eston  R. L. C. Araujo 《Pure and Applied Geophysics》1978,117(1-2):180-195

Results of geothermal gradient measurements in 44 localities in Brazil are presented. The Precambrian shield areas are found to be characterized by relatively low temperature gradients in the range 6 to 20°C/km while younger sedimentary basins are characterized by gradients in the range 15 to 35°C/km. An inverse correlation between geothermal gradient and tectonic age has been observed. This as well as the favourable hydrological conditions suggest that the best sites for extraction of geothermal energy in Brazil are the younger sedimentary basins. The Parana Basin is found to offer at present the best site for extraction of geothermal energy in Brazil. Preliminary examination of the temperature distributions in the major aquifer (Botucatu sandstone) suggest that this aquifer contains substantial quantities of warm waters in the temperature range 40 to 90°C. The water layer in this confined aquifer is in convective motion and can be considered as a low enthalphy geothermal system. Many of the routine uses to which geothermal waters are put, such as space heating and soil warming, are not applicable in Brazil mainly because of the favourable climatic conditions. Conversion of this geothermal energy into electrical energy is also unlikely to be economical. Hence we do not consider the Parana Basin geothermal system as an independent ec9nomically exploitable energy resource. However, a few other applications are pointed out where geothermal waters can be used as a supplementary or supporting energy source in increasing the efficiency of economically viable systems utilizing hot waters.  相似文献   

Petrography and geochemistry of carbonate void-filling cements in fossil reefs     

Dr. Ibrahim A. Mirsal  Prof. Dr. Heinrich Zankl 《International Journal of Earth Sciences》1979,68(3):920-951

An Investigation of the distribution of Ca²⁺, Mg²⁺, Na⁺, Sr²⁺ and K⁺ as well as O¹⁸ and C¹³ in void-filling cements out of three fossil reefs — of Devonian and Triassic ages — shows a rhythmic fluctuation of these parameters in the successive layers. This reflects a similar change in the salinity conditions during cementation. It also leads to the presumption that the void filling process starts in early stages with a semi-closed system and later passes into a relatively closed one. Results obtained from factor analysis support this hypothesis.The original mineralogic constitution of the cements must have followed the rhythmic fluctuation of salinity with the result of forming alternative layers of aragonite and calcite. These lead, through inversion and grain growth, in later diagenetic stages to the formation of fibrous calcite.Blocky calcite represents the last stage of cementation. It crystallises out of exhausted solutions and shows no signs of inversion.Multivariate analysis of all investigated parameters reveals three factors. These were interpreted as representing Salinity, Temperature and original Mineralogy.

---

Zusammenfassung Die Untersuchung der Verteilung von Ca²⁺, Mg²⁺, Na⁺, Sr²⁺ und K⁺, sowie O¹⁸ und C¹³ in Hohlraumzementen aus drei fossilen Riffen von devonischem und triadischem Alter zeigt eine rhythmische Schwankung in den sukzessiven Zementschalen. Die Schwankung der geochemischen Parameter reflektiert eine änderung der Salinitätsbedingungen. Dies wird unter der Annahme erklärt, daß die Ausfüllung der Hohlräume zuerst in einem halbgeschlossenen, später dann in einem relativ geschlossenen System stattfindet. Die Faktorenanalyse bestätigt diese Hypothese.Die Mineralogie der gebildeten Zemente folgt der rhythmischen Salinitätsschwankung und daraus entstand zunächst eine Wechsellagerung von calcitischen und aragonitischen Zementen.über Inversion und Sammelkristallisation bildet sich während der späteren Diagenese der fibröse Calcit, dessen rhythmische Gefügeabfolge von der ursprünglichen Mineralogie der Zemente diktiert wird. Als letzte Zementgeneration folgt blockiger Calcit aus ionenarmen Lösungen, wobei keine Umwandlung dieser Zementphase mehr erfolgt.Aus der Faktorenanalyse aller geochemischen Parameter ergeben sich drei Faktorengruppen, die die Salinität, Temperatur und ursprüngliche Bildungsmineralogie charakterisieren.

---

Résumé L'examen de la répartition du Ca₂₊, Mg₂₊, Na₊, Sr₂₊ et K₊, ainsi que O¹⁸ et C¹³ dans le ciment de remplissage des vides de 3 récifs fossiles d'âge dévonien à triasique, montre une variation rythmique dans les couches successives du ciment. La variation des paramètres chimiques reflète un changement dans les conditions de la salinité. Ceci s'explique si l'on accepte que le remplissage des vides a eu lieu dans un milieu d'abord à moitié fermé, et plus tard relativement fermé. L'analyse des facteurs confirme cette hypothèse. La minéralogie du ciment formé est conforme à la variation rythmique de la salinité, d'où résulta une alternance de ciment calcitique et aragonitique.Après l'inversion et la recristallisation coalescente, il s'est formé, durant la diagenèse ultérieure de la calcite fibreuse, dont la succession structurale rythmique est dictée par la minéralogie originelle du ciment. Comme dernière génération de ciment, vient de la calcite en bloc provenant d'une solution pauvre en ions, sans qu'il s'en suive une transformation decette phase de cimentation.L'analyse des facteurs de tous les paramètres chimiques fait apparaÎtre trois groupes de facteurs qui caractérisent la salinité, la température et la minéralogie originelle de formation.

---

, : Sa²⁺, Mg²⁺, Na²⁺, Sr²⁺ K⁺, ¹⁸O ¹³S . . , , , . . , . , . , , - . 3 , , .

  相似文献   

Short note: A simple nomogram for interpretation due to magnetic horizontal cylinders     

Ibrahim Kara  Davut Aydogan  F. Ahmet Yüksel 《Geophysical Prospecting》1998,46(6):659-663

The magnetic anomaly ΔF due to a long horizontal cylinder yields three points related to its extrema. A nomogram is presented for the determination of some source parameters of the causative body.  相似文献   

Comments on “Correlation analysis of geothermal data for the sedimentary basins of India” by J.G. Negi et al.     

V.M. Hamza 《Earth and Planetary Science Letters》1974,24(2):336

  相似文献   

On the iron interpretation of the 6.4 keV emission line from SGR 1900+14     

Alaa I. Ibrahim  Hisham Anwer  Mohamed H. Soliman  Nicholas Mackie-Jones  Kalvir S. Dhuga  William C. Parke  Jean H. Swank  Tilan Ukwatta  M. T. Hussein  T. El-Sherbini 《Astrophysics and Space Science》2007,308(1-4):535-539

A 6.4 keV emission line was discovered in an unusual burst from the soft gamma repeater SGR 1900+14 with the Rossi X-ray Timing Explorer (RXTE). The line was detected in part of a complex multipeak precursor that preceded the unusual burst of 1998 August 29, i.e. two days after the giant flare of August 27 from the source. The origin of the line was not firmly identified and two possible interpretations were equally plausible including (a) Kα fluorescence from a small iron rich material that was ejected to the magnetosphere during the August 27 flare, and (b) proton or α-particle cyclotron resonance. If the iron scenario was correct, we expect to find evidence for the line during the intervening interval between the flare and the August 29 burst, i.e. on August 28. Here we present the results of the August 28 burst observation, taken with RXTE. We detect a total of seven bursts whose individual and joint spectra do not show evidence for spectral lines. We also investigated a sample of nine bursts before and after the August 29 burst (from 1998 June to December) that do not reveal evidence for a spectral line near 6.4 keV or elsewhere. These results disfavor the iron scenario and make the proton/α-particle cyclotron resonance interpretation more plausible. The appearance of the emission line in part of a complex burst and its absence from the studied sample indicate that the line is likely due to a transient phenomenon that may depend on the burst morphology, energetics and the properties of the emission region.   相似文献   

Temporal and spatial zonation of macroepiphytes on Posidonia oceanica (L.) Delile leaves in a meadow off Tunisia          下载免费PDF全文

Lotfi Mabrouk  Mounir Ben Brahim  Asma Hamza  Med‐Najmeddine Bradai 《Marine Ecology》2015,36(1):77-92

The aim of this survey was to study the cover and the composition of macroepiphytic species on the leaves of Posidonia oceanica in the east of Tunisia. Surveys were conducted in December 2009 (winter period), March (spring period) and August 2010 (summer period) in a fringing reef located in Chebba. At each sampling date, 15 adult leaves were randomly collected and divided into basal and apical parts. The inner face of each part was examined with ocular glasses and microscope to estimate species cover by orthogonal projection. PERMANOVA and ANOSIM were used to test for differences of cover between sampling dates and leaf parts. SIMPER, cluster analysis, and PCA were used to ordinate species assemblages. Comparison of epiphytic cover along leaf blades showed significant differences for all groups, except cyanophycea, with high cover of hydrozoans and bryozoans in the basal part and high cover of algae in the apical part. The species composition and cover also vary with sampling date; minimum values were detected in December and the epiphytic community was composed of a few pioneer species, whereas maximum epiphytic cover values were registered in August, with the epiphytic community being composed of a more mature and more diverse community, termed ‘climax’. The main regulatory factors for this distribution are discussed.  相似文献   

Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24   总被引：1，自引：0，他引：1  

M. Bendict Lawrance  A. Shanmugaraju  Y.-J. Moon  M. Syed Ibrahim  S. Umapathy 《Solar physics》2016,291(5):1547-1560

  相似文献   

Diversity and temporal fluctuations of epiphytes and sessile invertebrates on the rhizomes Posidonia oceanica in a seagrass meadow off Tunisia     

Lotfi Mabrouk  Mounir Ben Brahim  Asma Hamza  Med‐Najmeddine Bradai 《Marine Ecology》2014,35(2):212-220

The aim of this work is to study the temporal dynamics of rhizome epiphytes and sessile animals living on the rhizomes of the seagrass Posidonia oceanica in the east of Tunisia. Surveys were conducted in October 2009, and in January, April and August 2010 on a fringing reef located in Chebba. Rhizomes were sampled by SCUBA diving at three stations. Samples were examined with a microscope to estimate the cover of macroinvertebrate and macroalgal organisms on the top 10 cm of each rhizome. Results revealed a high diversity of epiphytes on P. oceanica rhizomes with a dominance of red and brown algae, ascidians, and bryozoans. Distinct temporal changes were observed in Oued Lafrann, with a high January cover (winter period) for all groups. These winter increases can be attributed to: (i) the low phenological parameters of P. oceanica in winter that reduce the effects of shading, (ii) life cycles of the epiphytes and invertebrates, (iii) water motion and (iv) grazing.  相似文献   

Potential use of faujasite–phillipsite and phillipsite–chabazite tuff in purification of treated effluent from domestic wastewater treatment plants     

Reyad A. Al Dwairi  Khalil M. Ibrahim  Hani N. Khoury 《Environmental Earth Sciences》2014,71(12):5071-5078

Characterization of zeolitic tuff from Jabal Hannoun (HN) and Mukawir (MR) was carried out to examine the ability of using low-cost natural materials in domestic wastewater treatment. The grain size between 0.3 and 1 mm (0.3–1 mm) of the HN and MR has the highest total zeolite grade (faujasite–phillipsite and phillipsite–chabazite) and suitable cation exchange capacity. They were used as fixed-bed ion exchangers and adsorbents. The zeolitic tuff efficiently removed the organic and nitrogen compounds, Pb and Zn from the effluent. One bed volume (1 BV) of the zeolitic tuff is capable to remove up to 95 % of total organic carbon form 500 BV of the effluent. The removal percent of total nitrogen by HN and MR is close to 95 and 90 %, respectively. The zeolitic tuff has an excellent efficiency to remove Pb and Zn from the effluent. 1 BV of HN completely cleans Zn and Pb from 680 and 730 BV of the effluent, respectively, whereas 1 BV of MR is able to clean completely Zn and Pb from 500 and 685 BV of the effluent, respectively. The greater performance of the HN compared with the MR may be explained by its higher zeolites grade and presence of faujasite.  相似文献