CHEMISTRY INVESTIGATORY PROJECT ON -
AIM:-
MEASURING THE AMOUNT OF ACETIC ACID IN VINEGAR BY TITRATION WITH AN INDICATOR SOLUTION
PURPOSE:-
THE GOAL OF THIS PROJECT IS TO DETERMINE THE AMOUNT OF ACETIC ACID IN DIFFERENT TYPES OF VINEGAR USING TITRATION WITH A COLORED pH INDICATOR TO DETERMINE THE ENDPOINT
Physics investigatory project for class 12 on the topic " to estimate charge induced on two styro foam / pith balls separated by a distance "
Just change the name and cover page.
CHEMISTRY INVESTIGATORY PROJECT ON -
AIM:-
MEASURING THE AMOUNT OF ACETIC ACID IN VINEGAR BY TITRATION WITH AN INDICATOR SOLUTION
PURPOSE:-
THE GOAL OF THIS PROJECT IS TO DETERMINE THE AMOUNT OF ACETIC ACID IN DIFFERENT TYPES OF VINEGAR USING TITRATION WITH A COLORED pH INDICATOR TO DETERMINE THE ENDPOINT
Physics investigatory project for class 12 on the topic " to estimate charge induced on two styro foam / pith balls separated by a distance "
Just change the name and cover page.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
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 .
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
1. NAME - AYUSHMAAN PANDEY
CLASS- XII 'A'
ROLL NO.
Saraswati vidya mandir sr.
sec. school
2.
3. of coil depend
Objective
To study the factors on which the Self Inductance
of a coil depends by observing the effect of this coil,
4. when put in series with a resistor (bulb) in a circuit
fed up by an A.C. source of adjustable frequency.
5.
6. I would like to express my special thanks of gratitude to my
teacher Mrs.Shailendra sir who have given me the golden
opportunity to do this wonderful project on the topic which
also helped me in doing a lot of Research and I came to
know about so many new things. I am really thankful to
them.
Secondly I would also like to thank my parents and friends
who helped me a lot in finalizing this project within the limited
time frame.
10. There are four basic factors of inductor
construction determining the amount of inductance
created. These factors all indicate inductance by
affecting how much magnetic field flux will develop
11. for a given amount of magnetic field force (current
through the inductor’s wire coil.
The factors are:-
• NUMBER OF WIRE WRAPS, OR “TURNS” IN
THE COIL.
• COIL AREA.
14. Aim
To study the factor on which the Self Inductance of
a coil depends by observing the effect of this coil,
15. when put in series with a resistor (bulb) in a circuit
fed up by an A.C. source of adjustable frequency.
Apparatus Required
16. A coil of large turns, A.C. source of adjustable
frequency, an electric bulb, (6 V) A.C. ammeter of
suitable range, rheostat, a soft iron rod, one way
key, connecting wires etc.
17. Theory
Self Inductance is the property of a coil which
opposes the change in current through it. The Self
Inductance of a coil (long solenoid) is
18. L =μ0μr N2 A
Where μr= Relative magnetic permeability of
magnetic material,
μr = μμμ°
19. N= Total number of turns in solenoid
A= Area of cross section of solenoid
l= Length of solenoid
Hence, the Self Inductance depends upon
20. • No. of turns (N), L α N2
• Geometry of coil, L=A , L α 1/l
• Nature of core material, L= μ
21. When an inductor is connected in series with a
resistor (bulb) with a variable source of frequency,
then current flowing in the bulb is
I rms=E rms
22. Z
Where Z= (R2 + ω2L2)½=Impedance of the A.C.
Circuit
R= Resistance of bulb
L= Self Inductance of coil
23. ω = 2πf = Angular frequency of A.C. source.
The brightness of bulb i.e. Heat generated in bulb
is
H= I2rmsZt
24. The brightness of bulb i.e. Heat generated in bulb
is
H= I2rmsZt
Or,
P=H/t= I2rmsZ
28. Switch on the A.C. supply and adjust the
constant current in the circuit by using the
variable resistor (R1) (let frequency of source is
60 Hz and voltage is 6V).
29. Record the current in A.C. ammeter and see the
brightness of bulb.
Now, put the soft iron rod inside the inductor core
and record the current in A.C. ammeter and
30. again check the brightness of bulb. The current
and brightness both decreases.
Now, switch off the supply and decrease the
frequency of A.C. source (say 50 Hz).
31. Again switch on the supply and adjust the current
in circuit at same constant voltage 6V by using
the rheostat. Note the current in ammeter and
brightness of bulb. The current and brightness
both will increases.
32. Again insert the iron in the core of coil and note
the current and brightness. The current and
brightness both decreases.
33. Repeat the steps 5, 6 and 7 for different
frequency of A.C. source (say 40 Hz,30 Hz and
20 Hz).
38. • The current in the circuit decrease on inserting
the iron rod in the core of coil at constant
frequency of applied voltage and brightness of
bulb decreases and vice-versa.
39. • The current in the circuit increases on decreasing
the frequency of applied voltage and vice-versa.
Therefore, the brightness of bulb increases.
Precautions
40. • The coil should have large number of turns.
• Current should be passed for a small time to
avoid the heating effect.
• There should not be parallax in taking the
reading of ammeter.
41. Sources of Error
• The resistance of circuit may increases slightly
due to heating effect of current.
42. • There may be eddy current in soft iron coil.
Bibliography
https://www.google.com/url?sa=t&source=web&rct=j&url=https
://en.wikipedia.org/wiki/Inductance&ved=2ahUKEwj08Iniro7lAh
UJqI8KHTf0AnYQFjADegQIBBAB&usg=AOvVaw2P7iDjtFkUu
M4sVZ3Xvuee