The only one certified organic in the Philippines. Go Organic is a healhy way of living. It is also a good Organic Farming Business Model to make a living. We're looking for growers from Mindanao, Visayas and Calabarzon area who are willing to partner with us through franchising system. It is Built, Operate and Transfer technology; our company will assist franchisee until they can grow organic produce. Our company also be the one to buy produce from growers to market it to target market.
Para matricularte en nuestra escuela de negocios online MUNDO MARKETING solo pulsa clic en www.enelmundodelmarketing.com y paso seguido pulsa clic en la opción únete
Energy storage phosphors @ Phosphor Global Summit 2019Philippe Smet
Presentation on opportunities and limitations of energy storage phosphors, which can be used for glow-in-the-dark roads or safety illumination. Loss mechanisms in phosphors. Presented at the Phosphor Global Summit and Quantum Dot Forum 2019 in San Diego, La Jolla, California. March 19-21.
Talk presented at the ICIQ seminar in Tarragona, June 10 2022.
Abstract:
Persistent phosphors are typically impurity doped luminescent materials that feature an energy storage step between the excitation (e.g. by exposure to daylight or UV) and the emission of light. This energy storage, which can last from seconds to days, is rooted in charge carriers being trapped at particular defects in the material. Thermal energy is then required to release the charge carriers, after which recombination and light emission occurs. In this seminar, I will highlight the state-of-the-art in the field, by showing the unique characteristics of current applications (like in safety signage or bioimaging) and the remaining challenges. The physico-chemical mechanisms of the trapping and detrapping processes are discussed, along with the key analytical and spectroscopic techniques applied to those materials.
In the second part, starting from those recent insights, persistent phosphors are turned into a versatile sensing platform for mechanical pressure, ultrasound, temperature, or optical and X-ray dosimetry. For each application, the relevant mechanisms are highlighted, as well as the remaining hurdles.
Understanding of light sensing organs in biology creates opportunities for the development of novel optic systems that cannot be available with existing technologies. The insect's eyes, i.e., compound eyes, are particularly notable for their exceptional interesting optical characteristics, such as wide fields of view and infinite depth-of-field. While the construction of man-made imaging systems with these characteristics is of interest due to potential for applications in micro air vehicles (MVAs) and clinical endoscopes, currently available devices offer only limited capabilities due to their use of compound lens systems in planar geometries. In this presentation, I discuss a complete set of materials, design layouts and integration schemes for digital cameras that mimic fully hemispherical compound eyes. Certain of the concepts extend recent advances in ‘stretchable electronics’ that provide previously unavailable options in design. I also discuss another interesting hierarchical micro- and nanostructures that can be found in eyes of night-active insects such as moth and mosquito. I present research trends on fabrication methods, optical characteristics, and various applications for artificial micro-/nanostructures that resemble ‘moth eye’ structure.
GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096Sérgio Sacani
We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first
spatially resolved, mid-infrared images of IIZw096, a merging luminous infrared galaxy (LIRG) at z = 0.036.
Previous observations with the Spitzer Space Telescope suggested that the vast majority of the total IR luminosity
(LIR) of the system originated from a small region outside of the two merging nuclei. New observations with
JWST/MIRI now allow an accurate measurement of the location and luminosity density of the source that is
responsible for the bulk of the IR emission. We estimate that 40%–70% of the IR bolometric luminosity, or
3–5 × 1011 Le, arises from a source no larger than 175 pc in radius, suggesting a luminosity density of at least
3–5 × 1012 Le kpc−2
. In addition, we detect 11 other star-forming sources, five of which were previously
unknown. The MIRI F1500W/F560W colors of most of these sources, including the source responsible for the
bulk of the far-IR emission, are much redder than the nuclei of local LIRGs. These observations reveal the power
of JWST to disentangle the complex regions at the hearts of merging, dusty galaxies.
The only one certified organic in the Philippines. Go Organic is a healhy way of living. It is also a good Organic Farming Business Model to make a living. We're looking for growers from Mindanao, Visayas and Calabarzon area who are willing to partner with us through franchising system. It is Built, Operate and Transfer technology; our company will assist franchisee until they can grow organic produce. Our company also be the one to buy produce from growers to market it to target market.
Para matricularte en nuestra escuela de negocios online MUNDO MARKETING solo pulsa clic en www.enelmundodelmarketing.com y paso seguido pulsa clic en la opción únete
Energy storage phosphors @ Phosphor Global Summit 2019Philippe Smet
Presentation on opportunities and limitations of energy storage phosphors, which can be used for glow-in-the-dark roads or safety illumination. Loss mechanisms in phosphors. Presented at the Phosphor Global Summit and Quantum Dot Forum 2019 in San Diego, La Jolla, California. March 19-21.
Talk presented at the ICIQ seminar in Tarragona, June 10 2022.
Abstract:
Persistent phosphors are typically impurity doped luminescent materials that feature an energy storage step between the excitation (e.g. by exposure to daylight or UV) and the emission of light. This energy storage, which can last from seconds to days, is rooted in charge carriers being trapped at particular defects in the material. Thermal energy is then required to release the charge carriers, after which recombination and light emission occurs. In this seminar, I will highlight the state-of-the-art in the field, by showing the unique characteristics of current applications (like in safety signage or bioimaging) and the remaining challenges. The physico-chemical mechanisms of the trapping and detrapping processes are discussed, along with the key analytical and spectroscopic techniques applied to those materials.
In the second part, starting from those recent insights, persistent phosphors are turned into a versatile sensing platform for mechanical pressure, ultrasound, temperature, or optical and X-ray dosimetry. For each application, the relevant mechanisms are highlighted, as well as the remaining hurdles.
Understanding of light sensing organs in biology creates opportunities for the development of novel optic systems that cannot be available with existing technologies. The insect's eyes, i.e., compound eyes, are particularly notable for their exceptional interesting optical characteristics, such as wide fields of view and infinite depth-of-field. While the construction of man-made imaging systems with these characteristics is of interest due to potential for applications in micro air vehicles (MVAs) and clinical endoscopes, currently available devices offer only limited capabilities due to their use of compound lens systems in planar geometries. In this presentation, I discuss a complete set of materials, design layouts and integration schemes for digital cameras that mimic fully hemispherical compound eyes. Certain of the concepts extend recent advances in ‘stretchable electronics’ that provide previously unavailable options in design. I also discuss another interesting hierarchical micro- and nanostructures that can be found in eyes of night-active insects such as moth and mosquito. I present research trends on fabrication methods, optical characteristics, and various applications for artificial micro-/nanostructures that resemble ‘moth eye’ structure.
GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096Sérgio Sacani
We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first
spatially resolved, mid-infrared images of IIZw096, a merging luminous infrared galaxy (LIRG) at z = 0.036.
Previous observations with the Spitzer Space Telescope suggested that the vast majority of the total IR luminosity
(LIR) of the system originated from a small region outside of the two merging nuclei. New observations with
JWST/MIRI now allow an accurate measurement of the location and luminosity density of the source that is
responsible for the bulk of the IR emission. We estimate that 40%–70% of the IR bolometric luminosity, or
3–5 × 1011 Le, arises from a source no larger than 175 pc in radius, suggesting a luminosity density of at least
3–5 × 1012 Le kpc−2
. In addition, we detect 11 other star-forming sources, five of which were previously
unknown. The MIRI F1500W/F560W colors of most of these sources, including the source responsible for the
bulk of the far-IR emission, are much redder than the nuclei of local LIRGs. These observations reveal the power
of JWST to disentangle the complex regions at the hearts of merging, dusty galaxies.
A giant galaxy in the young Universe with a massive ringSérgio Sacani
In the local (redshift z ≈ 0) Universe, collisional ring galaxies make up only ~0.01% of galaxies1 and are formed by head-on galactic collisions that trigger radially propagating density waves2–4. These striking systems provide key snapshots for dissecting galactic disks and are studied extensively in the local Universe5–9. However, not much is known about distant (z > 0.1) collisional rings10–14. Here we present a detailed study of a ring galaxy at a look-back time of 10.8 Gyr (z = 2.19). Compared with our Milky Way, this galaxy has a similar stellar mass, but has a stellar half-light radius that is 1.5–2.2 times larger and is forming stars 50 times faster. The extended, dif- fuse stellar light outside the star-forming ring, combined with a radial velocity on the ring and an intruder galaxy nearby, provides evidence for this galaxy hosting a collisional ring. If the ring is secularly evolved15,16, the implied large bar in a giant disk would be inconsistent with the current understand- ing of the earliest formation of barred spirals17–21. Contrary to previous predictions10–12, this work suggests that massive col- lisional rings were as rare 11 Gyr ago as they are today. Our discovery offers a unique pathway for studying density waves in young galaxies, as well as constraining the cosmic evolution of spiral disks and galaxy groups.
Defects in energy storage phosphors: friends or enemies? (PRE19 workshop)Philippe Smet
Plenary talk presented at the PRE19 workshop (Photoluminescence in Rare Earths: Photonic Materials and Devices) in Nice, France, on September 4. Dealing with persistent luminescence, afterglow, mechanoluminescence, traps, defects and thermoluminescence. Overview of the activities of the LumiLab research in the past 10 years.
Dr. Riq Parra presents an overview of his program, Ultrashort Pulse (USP) Laser -- Matter Interactions, at the AFOSR 2013 Spring Review. At this review, Program Officers from AFOSR Technical Divisions will present briefings that highlight basic research programs beneficial to the Air Force.
A population of_fast_radio_bursts_ar_cosmological_distances
atri 2
1. UEF // University of Eastern FinlandUEF // University of Eastern Finland
Under graduate seminar, 03/10/2016
Atri Halder
LIMITS PROVIDED BY DIFFRACTION TO OPTICAL SYSTEMS
AND PROBABLE WAY TO GET RID OF IT
2. UEF // University of Eastern Finland 03/10/2016Atri Halder 2
0th order
z
x
+ 1st order
- 1st order
Transmission
function
Diffraction by a sinusoidal grating
T.F. =
1
2
1 + cos 𝑢𝑥
=
1
2
+
1
4
𝑒 𝑖𝑢𝑥
+
1
4
𝑒−𝑖𝑢𝑥
15˚
3. UEF // University of Eastern Finland
0th order
+ 1st order
- 1st order
x
z
Transmission
function
Diffraction by a sinusoidal grating
4
35˚
Atri Halder 03/10/2016
4. UEF // University of Eastern Finland 503/10/2016Atri Halder
0th order
x
+ 1st order
- 1st order
z
Diffraction by a sinusoidal grating
-2nd order
+ 2nd order
5. UEF // University of Eastern Finland
Imaging by optical system
503/10/2016Atri Halder
L1
L2
Image plane intensity
distribution
z
6. UEF // University of Eastern Finland
Diffraction pattern of a circuler aperture
3.10.2016Atri Halder 6
Normalizedintensity
X axis
Radious(R)
The diffraction pattern
of a circular aperture is
known as Airy Disc or
Point Spread Function
7. UEF // University of Eastern Finland
Diffraction pattern of a circuler aperture
3.10.2016Atri Halder 7
U V
L
1. Focal Length
2. Aperture
3. Wavelength
4. Source
10. UEF // University of Eastern Finland 3.10.2016Atri Halder 10
𝐿 =
1.22 𝜆
2 ݊ ߠ݊݅ݏ
11. UEF // University of Eastern Finland
Super-resolution
•Toraldo phase filter (The idea was first
developed by G. Toraldo di Francia in 1947)
•Genetic algorithem or Particle swarm
optimization
•Changing the shape of the Point Spread
Function
3.10.2016Atri Halder 11
12. UEF // University of Eastern Finland
Synthesis of phase filters:
123.10.2016Atri Halder
13. Refference:
1) Joseph W. Goodman, Introduction to Fourier Optics, 2nd edition
(McGraw-Hills Series).
2) Born, Max; Wolf, Emil (October 1999). Principles of Optics. Cambridge:
Cambridge University Press. p. 461. ISBN 0-521-64222-1.
3) G. Toraldo di Francia, “Modern trends in the evaluation of optical
images,” J. Opt. Soc. Am. 47, 507 (1957).
4) H. Hyv¨arinen, S. Rehman, J. Tervo, J. Turunen, and C. J. R. Sheppard,
“Limitations of superoscillation filters in microscopy applications,” Opt.
Lett. 37, 903–905 (2012).
3.10.2016Atri Halder 13