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صوره بسيطه عباره عن محاكاة الواقع بالخيال
مجسم لقارب وسط ماتبقى من مياه الأمطار يحاكي
ذلك القارب الحقيقي وسط مياه البحر
اتمنى ان تحوز على رضاكم
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
Film Simulation Kodak Panatomic X
Film Simulation = Acros + Y
Sharpness = +2
Shadows = +3
Highlights = +3
Grain = Off
Noise Reduction = 0
Dynamic Range = DR100
White Balance = Auto
Color = n/a
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The Fuji X-Pro1 has a very useful film simulation feature. With it, a user is able to produce images that look like they were taken with Fuji color negative films such as Fujicolor NPS and Fuji color slide films such as Provia, Velvia, and Astia.
Stacie Sicher, a registered nurse educator at Penn State Health St. Joseph Medical Center, right, looks on as Melissa Klimowicz, a nursing student from Drexel University College of Nursing and Health Professions, performs chest compressions during a code blue simulation on Thursday, Feb. 24, 2022.
Magnetohydrodynamic turbulence powered by neutrino-driven convection behind the stalled shock of a core-collapse supernova simulation. This simulation shows that the presence of rotation and weak magnetic fields dramatically impacts the development of the supernova mechanism as compared to nonrotating, nonmagnetic stars. The nascent neutron star is just barely visible in the center below the turbulent convection.
Image Credit: Sean M. Couch, Michigan State University
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
These are reference images I'm using to test my new Velvia 100 RVP Film Simulation presets.
It's pretty well nailed down. With DMAX increases to Greens and Reds, and careful attention to how Velvia F used to make Reds orange and Yellows green, I made the adjustsments to reflect with known parameters of Velvia 100 RVP.
Like RVP, lighting conditions, exposures and subjects work differently with this simulation, but I used this reference set of 16 images to really stress test the preset.
In some cases, only two of the sliders need to be adjusted to suit the shooting conditions which are Exposure and White settings.
White balance needs to be adjusted manually. RVP tends to have a coolish tendency to it's images (which kind of makes sense because projector lights tended to be warmer.
White balancing with this preset requires you find your optimal results and then pull back towards cool just a little bit.
Read more about this on my blog:
frontallobbings.blogspot.ca/2013/02/fujifilm-velvia-100-r...
Participants of the 14th World Scout Moot visit the parlament of Canada to have an active role as ambasadors on a UN simulation experience
Film Simulation Agfa Color
Film Simulation = Classic Chrome
Sharpness = 0
Shadows = +1
Highlights = +2
Grain = Strong
Noise Reduction = -3
Dynamic Range = Auto
White Balance = Auto
Color = -4
ISO = Auto (6400)
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The Pagani Zonda Revolucion is coming to Project CARS' Game of the Year Edition, available this spring!
More info:
www.projectcarsgame.com/home/announcing-project-cars-game...
During the week of 19 June 2017, 50 scientists and computing experts came together on the DESY campus in Zeuthen, Germany to discuss new analysis and simulation methods for CTA. The talks covered simulation tools, reconstruction algorithms and tools, instrument response functions, high-level science tools and grid tools.
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
Film Simulation Kodak Panatomic X
Film Simulation = Acros + Y
Sharpness = +2
Shadows = +3
Highlights = +3
Grain = Off
Noise Reduction = 0
Dynamic Range = DR100
White Balance = Auto
Color = n/a
Website | Google + | Facebook | Twitter | Visual Ohio Blog | Best Light Photo Blog | Tumblr
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
This image shows a simulated sky map showing the inner region (-90° < l < 90°) of the galactic plane that will be obtained during the CTAO galactic plane survey. The image shows expected populations of galactic supernova remnants and pulsar wind nebulae as well as diffuse emission that will be detected during the 1,600 hours of observing time planned for the survey.
Learn more: www.cta-observatory.org/ctas-galactic-plane-survey-will-p...
Credit: CTA Collaboration
Had some fun making an Aerochrome-esque photo edit in affinity photo. The real deal would have been fun to mess with if it was still available!
The Sentinel 2a Mission Control Team in simulation training at ESOC on 28 April 2015. Liftoff is set for June 2015.
The ‘Poverty Trap’ simulation took the entire year group into a school-based simulation of a slum in a developing country.
The Sentinel 2a Mission Control Team in simulation training at ESOC on 28 April 2015. Liftoff is set for June 2015.
The Sentinel 2a Mission Control Team in simulation training at ESOC on 28 April 2015. Liftoff is set for June 2015. Credit: ESA/J. Mai
Film Simulation Kodak Panatomic X
Film Simulation = Acros + Y
Sharpness = +2
Shadows = +3
Highlights = +3
Grain = Off
Noise Reduction = 0
Dynamic Range = DR100
White Balance = Auto
Color = n/a
Website | Google + | Facebook | Twitter | Visual Ohio Blog | Best Light Photo Blog | Tumblr
The precise conditions inside a white dwarf star in the hours leading up to its explosive end as a Type Ia supernova are one of the mysteries confronting astrophysicists studying these massive stellar explosions. But now, a team of researchers, composed of three applied mathematicians at the U.S. Department of Energy's (DOE) Lawrence Berkeley National Laboratory and two astrophysicists, has created the first full-star simulation of the hours preceding the largest thermonuclear explosions in the universe. www.lbl.gov/cs/Archive/news091509.html