This document discusses the Bailey Method for aggregate blending to achieve desired volumetrics and compaction in HMA. The key points are:
1) The Bailey Method focuses on aggregate packing and blending aggregates by volume rather than just weight. It evaluates individual aggregates and combined blends.
2) Important factors that influence results are gradation, compactive effort, aggregate shape/texture, and strength.
3) Aggregates are classified as "coarse" or "fine" based on nominal maximum particle size and primary control sieve. Evaluating by loose and rodded unit weights helps understand aggregate packing.
Aggregates blending, blending aggregates by graphical method, concrete mix design, concrete technology, what is aggregates blending, what is blending, methods of blending, how to blend aggregates, civil engineering
Aggregates blending, blending aggregates by graphical method, concrete mix design, concrete technology, what is aggregates blending, what is blending, methods of blending, how to blend aggregates, civil engineering
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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
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In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
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I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
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https://www.hubspot.com/state-of-marketing
· Scaling relationships and proving ROI
· Social media is the place for search, sales, and service
· Authentic influencer partnerships fuel brand growth
· The strongest connections happen via call, click, chat, and camera.
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· Seeking: A single source of truth
· TLDR; Get on social, try AI, and align your systems.
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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.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
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.
Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
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Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
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Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Toxic effects of heavy metals : Lead and Arsenicsanjana502982
Heavy metals are naturally occuring metallic chemical elements that have relatively high density, and are toxic at even low concentrations. All toxic metals are termed as heavy metals irrespective of their atomic mass and density, eg. arsenic, lead, mercury, cadmium, thallium, chromium, etc.
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https://www.hubspot.com/state-of-marketing
· Scaling relationships and proving ROI
· Social media is the place for search, sales, and service
· Authentic influencer partnerships fuel brand growth
· The strongest connections happen via call, click, chat, and camera.
· Time saved with AI leads to more creative work
· Seeking: A single source of truth
· TLDR; Get on social, try AI, and align your systems.
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ChatGPT is a revolutionary addition to the world since its introduction in 2022. A big shift in the sector of information gathering and processing happened because of this chatbot. What is the story of ChatGPT? How is the bot responding to prompts and generating contents? Swipe through these slides prepared by Expeed Software, a web development company regarding the development and technical intricacies of ChatGPT!
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Technology
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Age and Gender
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Race Affects Attitudes
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2. 2
Aggregate Blending
Where do you start?
„ Trial and Error?
„ Specification Bands
„ Coarse
„ Medium
„ Fine
„ Which blend is best?
„ How will it work in the field
during placement?
„ How will it perform?
„ Is there a more
systematical way to find
a starting point?
3. 3
Aggregate Blending
The Bailey Method
„ Originally developed by Robert D. Bailey
(Illinois Department of Transportation)
„ Focus is Aggregate packing!
„ Determine “Coarse” and “Fine”
„ Evaluate individual agg’s and combined blend
by VOLUME as well as by weight
4. 4
Aggregate Packing
What Influences the Results?
„ Gradation
- continuously-graded, gap-graded, etc.
„ Type & Amount of Compactive Effort
- static pressure, impact or shearing
„ Shape
- flat & elongated, cubical, round
„ Surface Texture (micro-texture)
- smooth, rough
„ Strength
- degradation or lack thereof
5. 5
Defining “Coarse” and “Fine”
„ “Coarse” fraction
„ Larger particles that create voids
„ “Fine” fraction
„ Smaller particles that fill voids
„ Estimate void size using Nominal Maximum
Particle Size (NMPS)
„ Break between “Coarse” and “Fine”
„ Primary Control Sieve (PCS)
6. 6
Diameter (d)
= NMPS
Flat face of
aggregate
particle
Round face of
aggregate
particle
Average
Void size
= 0.22*d
for all
four
conditions
Primary Control Sieve = 0.22 x NMPS
7. Primary Control Sieve
Mixture NMPS NMPS x 0.22 Primary Control Sieve
37.5mm 8.250mm 9.5mm
25.0mm 5.500mm 4.75mm
19.0mm 4.180mm 4.75mm
12.5mm 2.750mm 2.36mm
9.5mm 2.090mm 2.36mm
4.75mm 1.045mm 1.18mm
PCS determines the break between Coarse and Fine in the
combined blend and if a given aggregate is a CA or FA
8. 8
Evaluating Aggregates by
Volume
„ Why?
„ Better understand
aggregate packing
„ Control VOLUME of Coarse
and Fine for Mix “Type”
„ How?
„ Test the individual Coarse
and Fine aggregates
9. 9
Loose Unit Weight - CA
„ NO compactive effort
applied
„ Start of particle-to-
particle contact
„ Use shoveling
procedure
„ Strike off ~ level
„ Careful not to compact
„ Determine LUW
„ Kg/m3 or lbs./ft3
„ Determine volume of
voids
10. 10
Rodded Unit Weight - CA
„ With compactive effort
applied
„ Increased particle-to-
particle contact
„ Three equal lifts using
shoveling procedure
„ Rod 25 times per lift
„ Strike off ~ level
„ Careful not to compact
„ Determine RUW
„ Kg/m3 or lbs./ft3
„ Determine volume of
voids
11. 11
Chosen Unit Weight - CA(s)
LUW RUW
Coarse-Graded SMA
Fine-Graded
< LUW
< 90% 95-105% 110-125%
12. 12
Chosen Unit Weight - FA(s)
100%
LUW
100%
RUW
Dense-graded
FA CUW
“SET”
According To
Mix Type
SMA
13. 13
Developing the Combined
Blend
1. Determine Mix Type & NMPS
2. Choose the VOLUME of CA
3. Blend the CA’s by VOLUME
4. Blend the FA’s by VOLUME
5. Choose the desired % Minus 0.075mm
Convert the Individual aggregate %’s
from VOLUME to weight
14. 14
Combined Blend Evaluation
„ Evaluation method
depends on which
fraction (Coarse or
Fine) is in control:
„ Coarse-graded, SMA
„ Fine-graded
15. K J I H G F E
K J I H G F E D C B A
D C B A
Sieve Size (mm) Raised to 0.45 Power
Sieve Size (mm) Raised to 0.45 Power
100
100
0
0
%
Pass
ing
%
Pass
ing
Combined Blend Gradation
Combined Blend Gradation
50
50
20
20
80
80
Sieve % Passing
A 100
B 97
C 76
D 63
E 39
F 25
G 17
H 11
I 7
J 5
K 4.2
10
10
30
30
40
40
60
60
70
70
90
90
Coarse
Fine
1
2
3
4
16. 16
Combined Blend Evaluation
Coarse-Graded Mixes
Half Sieve = 0.5 x NMPS
PCS = 0.22 x NMPS
Coarse
Fraction
Fine
Fraction
SCS = 0.22 x PCS
TCS = 0.22 x SCS
1 CA CUW (% PCS)
CA Ratio =
% Half Sieve - % PCS
100 - % Half Sieve
FAf Ratio =
% TCS
% SCS
2
3
4
FAc Ratio =
% SCS
% PCS
17. 17
Combined Blend Evaluation
Coarse-Graded Mixes
1. CA CUW increase = VMA increase
„ 4% change in PCS ≅ 1% change in VMA or
Voids
2. CA Ratio increase = VMA increase
„ 0.20 change ≅ 1% change in VMA or Voids
3. FAc Ratio increase = VMA decrease
„ 0.05 change ≅ 1% change in VMA or Voids
4. FAf Ratio increase = VMA decrease
„ 0.05 change ≅ 1% change in VMA or Voids
Has the
most
influence
on VMA
or Voids
18. K J I H G F E
K J I H G F E D C B A
D C B A
Sieve Size (mm) Raised to 0.45 Power
Sieve Size (mm) Raised to 0.45 Power
100
100
0
0
%
Pass
ing
%
Pass
ing
Combined Blend Gradation
Combined Blend Gradation
50
50
20
20
80
80
Sieve % Passing
A 100
B 92
C 60
D 32
E 25
F 19
G 17
H 15
I 13
J 11
K 9.5
10
10
30
30
40
40
60
60
70
70
90
90
Coarse
Fine
1
2
3
4
19. 19
Combined Blend Evaluation
SMA Mixes
1. CA CUW increase = VMA increase
„ 2% change in PCS ≅ 1% change in VMA or
Voids
2. CA Ratio increase = VMA increase
„ 0.20 change ≅ 1% change in VMA or Voids
3. FAc Ratio increase = VMA decrease
„ 0.10 change ≅ 1% change in VMA or Voids
4. FAf Ratio increase = VMA decrease
„ 0.10 change ≅ 1% change in VMA or Voids
Has the most
influence on
VMA or
Voids
Has the
2nd most
influence
on VMA
or Voids
20. K J I H G F E
K J I H G F E D C B A
D C B A
Sieve Size (mm) Raised to 0.45 Power
Sieve Size (mm) Raised to 0.45 Power
100
100
0
0
%
Pass
ing
%
Pass
ing
Combined Blend Gradation
Combined Blend Gradation
50
50
20
20
80
80
Sieve % Passing
A 100
B 98
C 85
D 72
E 58
F 40
G 32
H 21
I 12
J 7
K 4.4
10
10
30
30
40
40
60
60
70
70
90
90
1
2
3
4
Coarse
Fine
21. 21
Combined Blend Evaluation
Fine-Graded Mixes
Original Half Sieve
Original PCS
New PCS
New Half Sieve
New SCS
New TCS
New
Coarse
Fraction
New Fine
Fraction
Original
Coarse
Fraction
1
2
3
4
% CA LUW
New CA Ratio
New FAc Ratio
New FAf Ratio
22. 22
Combined Blend Evaluation
Fine-Graded Mixes
1. CA CUW decrease = VMA increase
„ 6% change original PCS ≅ 1% change in VMA or
Voids
2. New CA Ratio increase = VMA increase
„ 0.35 change ≅ 1% change in VMA or Voids
3. New FAc Ratio increase = VMA decrease
„ 0.05 change ≅ 1% change in VMA or Voids
4. New FAf Ratio increase = VMA decrease
„ 0.05 change ≅ 1% change in VMA or Voids
„ Old CA Ratio still relates to segregation
susceptibility
Has the
most
influence
on VMA
or Voids
26. 26
Predicting Performance
„ We can relate to
volumetric changes
well
„ We can relate blend
gradations and the
four main principles
to compactibility and
segregation
„ But…….performance
includes much more!
27. R2
= 0.0649
2.5
3.0
3.5
4.0
4.5
5.0
5.5
6.0
36 37 38 39 40 41 42 43 44 45 46 47
PCS
Rutting
(mm)
R2
= 0.0283
2.5
3.0
3.5
4.0
4.5
5.0
5.5
6.0
0.900 0.920 0.940 0.960 0.980 1.000
New CA Ratio
Rutting
(mm)
R2
= 0.0088
2.5
3.0
3.5
4.0
4.5
5.0
5.5
6.0
0.280 0.290 0.300 0.310 0.320 0.330 0.340
New FAc Ratio
Rutting
(mm)
Rutting
vs. PCS
Rutting vs.
New CA Ratio
Rutting vs.
New FAc Ratio
28. 28
So How Does the Method
Help?
„ In Developing New Blends:
„ Field Compactibility
„ Segregation Susceptibility
„ In Evaluating Existing Blends:
„ What’s worked and what hasn’t?
„ More clearly define principle ranges
„ In Estimating VMA/Void
changes between:
„ Design trials
„ QC samples
„ Saves Time and Reduces Risk!