Csil presents a list of Lighting market research
-World Trade of Lighting Fixtures and Lamps
-LEDS and the Worldwide Market for Lighting Fixtures
-World Market for Retrofit LED Lamps
-E-Commerce for the Lighting Fixtures Industry
-The European Market for Lighting Fixtures, Part I
-The European Market for Lighting Fixtures, Part II
The Lighting Fixtures market in Russia
...
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The solution to promote research and development of new solutions is to invest in new forms of "modus operandi" with strategy and awareness; for example, to invest in new financing instruments, such as European funding programs direct and indirect, the bank funds European investment Bank (EIB); or as the formula of public-private partnerships (PPP); or as other forms, such as crowdfunding or venture capital.
Responda 113 Linux-ympäristö hallinnoidaan SUSE Managerin avullaFinceptum Oy
Responda 113 on käyttänyt SLESia ja SUSE Manageria omassa it-ympäristössään vuoden 2015 alusta lähtien. Niiden käyttöönotto sujui suunnitelmien mukaan.
”SUSEn järjestämä koulutus auttoi oivaltamaan SUSEn tavan tehdä asioita. Käyttöönoton ja asennuksen teimme yhdessä heidän asiantuntijoiden kanssa hyvänä tiimityönä, sisältäen ratkaisun toimivuuteen liittyvät työpajat”, painottaa Jousimaa. ”Uskon SUSEn soveltuvan hyvin myös myöhemmin alkavaan erittäin kriittiseen tuotantokäyttöön. Koko operatiivinen toimintamme hyödyntää Linux ja SUSE ympäristöjä. ”
”Linuxin osuus tulee edelleen kasvamaan. SUSE Manager on osoittautunut todella hyväksi työkaluksi Linux-ympäristön hallinnointiin. Päivitykset sujuvat ja voimme kontrolloida sekä valvoa ympäristöä tehokkaasti. Näemme yhdellä silmäyksellä koneiden tilan, ja voimme helposti auditoida ovatko palvelimet turvassa myös tunnetuimmilta tietoturvauhkilta. Päivityksiä voidaan toteuttaa yhdellä kerralla useille järjestelmille ja voimme olla varmoja siitä, että kriittiset palvelinkonfiguraatiot on tehty samalla tavalla”, sanoo Jousimaa.
”SUSEn ratkaisut ovat toimineet ongelmitta, emmekä ole tarvinneet niihin liittyvää tukipalvelua. Tukea ja asiantuntemusta on tarjolla SUSElta tarpeen vaatiessa. Ympäristömme kuormittaa it-yksikköämme vähemmän, ja aikaa on vapautunut ylläpidosta kehitystyöhön. Ilman SUSE Manageria emme kykenisi hallinnoimaan tehokkaasti kymmeniä virtuaalipalvelimia”, korostaa Jousimaa.
”Linux-palvelinten hallinta on helpompaa verrattuna Windowsiin
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A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
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.
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.
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.
2. Description of Stellar Sea Lions
A comparison of a baby Steller Sea Lion
to an adult Steller Sea Lion.
A Steller Sea Lions face up close.
3. Where can I find a Steller Sea Lion?
Here we have a haulouts or rookery
with Steller Sea Lions on it.
This is a map showing red dots for
the populations of Steller Sea Lions
being known to live.
6. Movement & Migration
From this map, we can see the migration patterns of Steller Sea Lions in different
seasons. The summer is typically when mating occurs so they are found bundled up
by each other in few areas. Then we winter comes around they all usually disperse to
find better foraging sites; males will go farther than females.
http://www.sararegistry.gc.ca/6F4F012C-8D22-46C0-A95F-
AA05524EF18B/fig04_eng.jpg
7. Natural Enemies & Defensive Behavior
Many factors that influence Steller Sea Lions threats are that of:
1. environmental changes (warming of Pacific Ocean)
2. Diseases (pneumonia, a bacterial infection called
Leptospirosis, which affects their kidneys and livers, and San
Miguel sea lion virus)
3. Predation (killer whales and sharks)
4. acoustic disturbances (noise chips, aircraft, research boats, or
military activities can affect vibrations in the water)
5. intentional take (fishermen shooting or capturing Sea Lions)
https://www.youtube.com/watch?v=s56PEYP0D1E
In this video we see a shark attacking a Steller Sea Lion. We can see that a Sea
Lions only real defense mechanism is to swim away. They do not have any special
piece on their body that helps them fight away predators.
8. Social And Solitary Behavior
Here is a picture of Steller Sea
Lions on a refugee. On a
refugee it is common that you
will find more females than
males, due to the fact that
males are out traveling and
running into other animals
where they have to
communicate with one
another to stay safe.
9. Reproductive Behavior/Life Cycle
Females give birth
to their first pup
when they are 4 to 6
years old. They are
able to give birth
once a tear there
after.
Pups are born late May
through early July, most
during second or third
week of June.
Females stay
with pups for 9
days before
beginning a
regular routine
of foraging trips
to sea
Mother leaves to
feed at sea,
beginning a cycle 1-3
days at sea & 1-2 days
feeding her pup
Nursing period can last up
to 3 years, but in just 11-14
days females begin
breeding process again.
A Steller Sea Lions life
span is about 30 years for
females and 20 years for
males.
10. Conservation Status
1990- Steller Sea Lions were put on the Endangered Species List
1997- It was later recognized that there were 2 other populations of Steller
Sea Lions taking them off of the “Depleted” list and uplifted to the
Endangered Status under the ESA
2012- Eastern population was delisted by designing a Steller Sea Lion
Recover Plan
2013- Eastern population was removed from the ESA, but still holds its
depleted status under MMPA
As far as the Western population of Steller Sea Lion’s goes the Alaska Sea
Otter and Steller Sea Lion Commission will continue to keep a close eye on
Steller Sea Lions over the next few years to make sure that there is only a
positive change in the condition so that the population does not become
more endangered.
11. Current Research
We, the people, must keep our eye out for any suspicious behavior that
may be harming Steller Sea Lions to help keep their population growing!
They’re growling for your help.
http://www.marinemammal.org//wp-content/uploads/2012/10/haulout.jpg
Map is found at: http://www.adfg.alaska.gov/static/research/programs/marinemammals/images/steller_haulouts_rangemap.jpg