Poster I produced for the Synthesis of a core drilled by ConocoPhillips in the Southern North Sea. I achieved a 1st class grade (A4) for the Poster and accompanying report.
Aggregate Used in Concrete & Building Purposes; صخورالصوان (Chert)
درنات او عقيدات الشيرت(Nodular or Concretion Cherts)
زلط الطواحين (Mill chert)
الشيرت الطبقى (Bedded Cherts )
رواسب الكالسيوم الكربونات (Calcium Carbonate Deposits)
الحجر الجيري (Limestone)
الدولوميت (Dolomite/ Dolostone)
الفرق بين الحجر الجيري (Limestone) و الدولوميت (Dolomite/ Dolostone)
استخدمات الحجر الجيري
السن المستخدم فى الاغراض المدنية
سن الأسفلت (Road or Asphalt Aggregates):
سن جابرو (Gabbro Aggregates)
سن بازالت (Basalt Aggregates)
سن الدولوميت (Dolomite/Dolostone Aggregates)
سن الشيرت (Chert Aggregates)
السن المستخدم فى الخرسانة وأغراض البناء (Aggregate Used in Concrete & Building Purposes)
الفرق بين الزلط (Flint/Chert) و السن (Aggregate)...!
الأقضلية بين استخدام الزلط (Flint/Chert) و السن (Aggregate) فى الخرسانة وأغراض البناء
How can minerals deposits be formed; GEOLOGICAL PROCESSES; Ore Fluids; Ore Forming Processes; Concentrating Processes; Magmatic mineral deposits; Residual mineral deposits ; Placer deposits; Sedimentary mineral deposits; Metamorhogenic mineral deposits; Hydrothermal mineral deposits ; Magmatic Deposits
Cumulate deposits: fractional crystallization processes can concentrate metals (Cr, Fe, PGE, Pt, Ni, Ti, Diamond ))
Pegmatites : late staged crystallization forms pegmatites and many residual elements are concentrated (Li, Ce, Be, Sn, U, Rare Earths (REE), Feldspar, Mica, Gems).
magmatic deposits; Mode of Formation of Magmatic Ores Deposits; Mode of Formation of Orthomagmatic Ores ; Fractional Crystallization (or Crystal fractionation ); Magmatic (or Liquid ) Immiscibility; Simple crystallization without concentration (Dissemination); Segregation of early formed crystals; (Layer Types); Injection of material concentrated elsewhere by differentiation Residual liquid segregation; Residual liquid injection; Immiscible liquid segregation; Immiscible-liquid-injection; Early magmatic deposit; Late magmatic deposit; Types of Magmatic Ore Deposits:Chromite; Fe-Ti (± V) oxides; Ni – Cu – Fe (± Pt) sulfides; Platinum Group Elements (PGEs); REE, and Zr in Carbonatites; Diamond in kimberlites.
Most evaporites are derived from bodies of Sea-water, but under special conditions, Inland lakes may also give rise to evaporite deposits, particularly in regions of low rainfall and high temperature.
Evaporite deposits are excellent indicators of paleoclimate (need a hot and arid climate for major evaporite deposits to form)
Igneous rocks formaion through chemical weatheringrita martin
Igneous rocks are generally termed as fire rocks formed either underground or above ground there are two types Intrusive, Extrusive igneous rocks mainly containing high silica content
Aggregate Used in Concrete & Building Purposes; صخورالصوان (Chert)
درنات او عقيدات الشيرت(Nodular or Concretion Cherts)
زلط الطواحين (Mill chert)
الشيرت الطبقى (Bedded Cherts )
رواسب الكالسيوم الكربونات (Calcium Carbonate Deposits)
الحجر الجيري (Limestone)
الدولوميت (Dolomite/ Dolostone)
الفرق بين الحجر الجيري (Limestone) و الدولوميت (Dolomite/ Dolostone)
استخدمات الحجر الجيري
السن المستخدم فى الاغراض المدنية
سن الأسفلت (Road or Asphalt Aggregates):
سن جابرو (Gabbro Aggregates)
سن بازالت (Basalt Aggregates)
سن الدولوميت (Dolomite/Dolostone Aggregates)
سن الشيرت (Chert Aggregates)
السن المستخدم فى الخرسانة وأغراض البناء (Aggregate Used in Concrete & Building Purposes)
الفرق بين الزلط (Flint/Chert) و السن (Aggregate)...!
الأقضلية بين استخدام الزلط (Flint/Chert) و السن (Aggregate) فى الخرسانة وأغراض البناء
How can minerals deposits be formed; GEOLOGICAL PROCESSES; Ore Fluids; Ore Forming Processes; Concentrating Processes; Magmatic mineral deposits; Residual mineral deposits ; Placer deposits; Sedimentary mineral deposits; Metamorhogenic mineral deposits; Hydrothermal mineral deposits ; Magmatic Deposits
Cumulate deposits: fractional crystallization processes can concentrate metals (Cr, Fe, PGE, Pt, Ni, Ti, Diamond ))
Pegmatites : late staged crystallization forms pegmatites and many residual elements are concentrated (Li, Ce, Be, Sn, U, Rare Earths (REE), Feldspar, Mica, Gems).
magmatic deposits; Mode of Formation of Magmatic Ores Deposits; Mode of Formation of Orthomagmatic Ores ; Fractional Crystallization (or Crystal fractionation ); Magmatic (or Liquid ) Immiscibility; Simple crystallization without concentration (Dissemination); Segregation of early formed crystals; (Layer Types); Injection of material concentrated elsewhere by differentiation Residual liquid segregation; Residual liquid injection; Immiscible liquid segregation; Immiscible-liquid-injection; Early magmatic deposit; Late magmatic deposit; Types of Magmatic Ore Deposits:Chromite; Fe-Ti (± V) oxides; Ni – Cu – Fe (± Pt) sulfides; Platinum Group Elements (PGEs); REE, and Zr in Carbonatites; Diamond in kimberlites.
Most evaporites are derived from bodies of Sea-water, but under special conditions, Inland lakes may also give rise to evaporite deposits, particularly in regions of low rainfall and high temperature.
Evaporite deposits are excellent indicators of paleoclimate (need a hot and arid climate for major evaporite deposits to form)
Igneous rocks formaion through chemical weatheringrita martin
Igneous rocks are generally termed as fire rocks formed either underground or above ground there are two types Intrusive, Extrusive igneous rocks mainly containing high silica content
SUPERGENE ENRICHMENT; Definition; Zones; Morphology of Zoning; Oxidized zone ; Supergene zone ; Gossans and Cappings; Chemical Changes Involved; Electrowinning; Formation of Copper Oxides
In this presentation we discuss cobalt crusts, its classification, Occurrence and Distribution, Formation, Texture, Mineralogy, Scope for future mining and exploration.
Residual mineral deposits; Laterites; Laterite Profile; Laterisation system; Laterite/Bauxite Conditions; Laterite-type Bauxite, Constitution of Bauxite, Types of deposits; Origin and Mode of formation; Clay (Kaolinite) Deposits; Nickel Laterite Deposits; Mineralogy and Types of lateritic nickel ore deposits; World Nickel Laterite Deposits; Processing of Ni Laterites; Example: Ni-laterites, Ni in soils in east Albania
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
2. Accompanying Information Leaflet for Well 41/15-1
Geological Context:
The core represents Well 41/15-1 drilled by ConocoPhilips in the Southern North Sea off the Yorkshire
coast. This section of core can be correlated to the Zechstein group which is of Permian age.
Diagenetic Processes: The relative timing of these events is shown on Figure 3.
Pyrite formation requires the presence of organic matter in the sediment, sulfate dissolved in aqueous
solution in the pore water and, locally anaerobic (reducing) conditions. It is the presence of decaying
organic matter in the sediment that creates the reducing chemical environment (Bacterial Sulfate
Reduction). The bacteria reduce the sulfate ions (SO42-) in pore water to sulfide ions (S2-) and if iron is
present it will react with it to form pyrite (FeS2). CH2O + SO4
2- -> H2S + CO2. These sulfate reducing
bacteria require other nutrients to survive which is provided by the organic matter (sugars). The
pyrite-sulfur content of the rock correlates directly with TOC content of the rock (a measure of source
rock richness).
Stylolites are formed due to the compaction of the micrite. It involves a large-scale loss of material.
During compaction, the micrite dissolves along horizontal planes on which insoluble residue
accumulates to form stylolites. The insoluble residue, consists largely of clay minerals, accumulates on
these planes and produces a dark foliation/band. They form by pressure dissolution, which is a
dissolution process that reduces pore space under pressure during diagenesis (Klein and Philpotts,
2017). This results in the micrite having a very low porosity and this has a knock-on effect on
permeability, reducing it also. This nature of the rock makes it a good seal. Stylolites are present
throughout the whole core, highlighting the fact that, the whole section previously consisted of Micrite.
Quartz nodules suspected to be Chert were present in the core. Chert consists almost entirely of Silica
that forms when the Siliceous skeletons of marine plankton are dissolved during diagenesis, with Silica
being precipitated from pore water into fractures/pores within the rock.
Dolomite forms from the post-depositional alteration of the lime mud by magnesium rich groundwater.
The groundwater has a meteoric origin. The available Mg facilitates the conversion of calcite to
dolomite. Only the upper core (Box 1-9) has experienced significant dolomitisation. Evidence for this is
through the weak reaction with dilute HCl. This is most likely the extent to which Mg rich groundwater
could penetrate and had enough Mg2+ to replace Ca2+.
Anhydrite was identified throughout the core, SEM and thin section images (Figures 4-7). It was present
in the section of dolomitic lime mud. It is an evaporite deposit that likely precipitated as gypsum but
upon burial and compaction, has been dehydrated to Anhydrite. The gypsum was likely deposited on
the edges of the lagoon (the intertidal zone).
Depositional Environment:
The depositional environment of the whole unit is a stratified lagoonal environment. The upper core
consists of dolomitised lime mud with thin sections of anhydrite and traces of pyrite and chert. This
represents a depositional environment with partial terrestrial exposure whilst also having anoxic,
reducing conditions. The micrite was deposited in a lagoon. A regression likely occurred after, allowing
for evaporite precipitation in the upper core. Block diagram illustrating this (Figure 1.) A basinal
environment was also considered but due to being unable to explain the presence of evaporites in a
short transition (i.e. going from basinal facies to intertidal facies in 20m) this option was ruled out.
In Figures 4-5 the rocks are stained with Alizarin Red solution (a surface precipitate) that reacts with
carbonates to highlight calcite (pink) and doesn’t react with dolomite (unstained). (J. A. D. Dickson,
1966).
3. References:
Cameron, T. (1992). The Geology of the Southern North Sea. HMSO, London.
Data-ogauthority.opendata.arcgis.com. (2020). OGA - Oil & Gas Activity - SNS. [online] Available at:
https://data-ogauthority.opendata.arcgis.com/datasets/1e557a10142a467ca53d8b664d9c5a65
[Accessed 26 Jan. 2020].
J. A. D. Dickson (1966). Carbonate Identification and Genesis as Revealed by Staining. Journal of
Sedimentary Research, 36, 491-505.
Klein, C. and Philpotts, A. (2017). Earth materials. 2nd ed. Cambridge University Press, St Ives.
Underhill, J. and Hunter, K. (2008). Effect of Zechstein Supergroup (Z1 cycle) Werrahalit pods on
prospectivity in the southern North Sea. AAPG Bulletin, 92(7), 827-851.