This document provides specifications for various standard H-beam, wide flange, lip channel, and equal angle steel sections. It includes dimensions such as height, width, thickness, area, weight, moments of inertia, radii of gyration, and other geometric properties. Sections range in size from 100x100 mm to 588x300 mm for H-beams, 148x100 mm to 500x200 mm for wide flanges, 100x50x20 mm to 200x75x20 mm for lip channels, and 40x40 mm to 120x120 mm for equal angles. Properties are specified in metric units.
Fantastic tutorial, shared with us by Dario Ilardi, of Grafica2d3d.com, I recommend to see.
The website is in Italian, but it is full of excellent tutorials, understandable in any language.
This great tutorial, explain, step by step, how to obtain, by using vray 2.0 for sketchup, a render, clear and clean as what we see in the picture below.
Dario say : " I'm experimenting with the use of brute force as a substitute of irradiance map and I must say that in terms of speed and quality impressed me positively "
Thanks so much Dario for this one, the result is really good !
Fantastic tutorial, shared with us by Dario Ilardi, of Grafica2d3d.com, I recommend to see.
The website is in Italian, but it is full of excellent tutorials, understandable in any language.
This great tutorial, explain, step by step, how to obtain, by using vray 2.0 for sketchup, a render, clear and clean as what we see in the picture below.
Dario say : " I'm experimenting with the use of brute force as a substitute of irradiance map and I must say that in terms of speed and quality impressed me positively "
Thanks so much Dario for this one, the result is really good !
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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.
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.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
1. H-BEAM
Standard Sectional Dimension
Section
Informativ e Reference
A rea Unit Geometrical Radius O f Modulus O f
Nominal H x B t1 t2 r A Weight Moment O f Inertia Gy ration O f A rea Section
Dimensional
mm
mm mm mm mm cm2 kg/m
lx cm4 ly cm4 ix cm iy cm Zx cm3 Zy cm3
100 x 100
100 x
100
6 8 10 21.90 17.20 383 134 4.18 2.47 76.50 26.7
* 125 x 125
125 x
125
6.5 9 10 30.31 23.80 847 293 5.29 3.11 136 47.00
150 x 150
150 x
150
7 10 11 40.14 31.50 1,640 563 6.39 3.75 219.00 75.10
* 175 x 175
175 x
175
7.5 11 12 51.21 40.20 2,880 984 7.50 4.38 330.00 112.00
200 x 200
200 x
200
8 12 13 63.53 49.90 4,720 1,600 8.62 5.02 472.00 160.00
250 x 250
250 x
250
9 14 16 92.18 72.40 10,800 3,650 10.80 6.29 867.00 292.00
300 x 300
300 x
300
10 15 18 119.80 94.00 20,400 6,750 13.10 7.51 1,360.00 450.00
350 x 350
350 x
350
12 19 20 173.9 137.00 40,300 13,600 15.20 8.84 2,300.00 776.00
2. Wide Flange Shape - According JIS G3192
Standard SectionalDimension
Section Informative Reference
Area Unit Geometrical Radius Of Modulus Of
H x B t1 t2 r A Weight Moment Of Inertia Gyration Of Area Section
mm mm mm mm cm2 kg/m Kg/12m
lx cm4 ly cm4 ix cm iy cm Zx cm3 Zy cm3
150 x
75
5 7 8 17.85 14.00 168 666 49.5 6.11 1.66 88.8 13.2
* 148 x
100
6 9 11 26.84 21.10 253.2 1,020 151 6.17 2.37 138 30.1
198 x
99
4.5 7 11 23.18 18.20 218.4 1,580 114 8.26 2.21 160 23.0
200 x
100
5.5 8 11 27.16 21.30 255.6 1,840 134 8.24 2.22 184 26.8
* 194 x
150
6 9 8 38.11 29.9 - 2,630 507 8.30 3.65 271 67.6
248 x
124
5 8 12 32.68 25.70 308.4 3,540 255 10.4 2.79 285 41.1
3.29 481 67.79 12 37.66 29.60 355.2 4,050 294 10.4 2.79 324 47.0
298 x
149
5.5 8 13 40.80 32.0 384 6,320 442 12.4 3.29 424 59.3
300 x
150
6.5 9 13 52.68 36.70 440.4 7,210 508 12.4 3.29 481 67.7
346 x
174
6 9 13 52.68 41.40 469.8
11,100 792
14.5 3.88 641 91.0
350 x
175
7 11 14 72.16 49.60 595.2 13,600 984 14.7 3.95 775 112
396 x
199
7 11 16 84.1 56.60 679.2 20,000 1,450 16.7 4.48 1,010 145
400 x
200 8 13 16 96.8 66.0 792 23,700 1,740 16.8 4.54 1,190 174
450 x
200
9 14 8 96.8 76.0 912 33,500 1,870 18.6 4.40 1,490 187
500 x
200 10 16 20 114.2 89.6 1075.2 47,800 2,140 20.5 4.43 1,910 214
600 x
200
11 17 22 134.4 106 1272 77,600 2,280 24.0 4.12 2,590 228
588 x
300
12 20 28 192.5 151 1812 181,000 9,020 24.80 6.85 4,020 601