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THe kit looks wrong, unfortunaley the fix will be incredibly difficult, as the whole nose of the car is too long, too flat, and alerady painted...
Bis 1864 gehörte Flensburg zu Dänemark. An den Gebäuden und Straßen dieser Zeit lassen sich auch heute noch Einflüsse dänischer Lebensart erkennen.
Leider vergaß ich bei der Abreise die Tasche mit meiner neuen Kamera. So entstanden diese Aufnahmen notgedrungen mit meiner alten Ersatzkamera. Das hat aber auch nicht viel schlechter funktioniert.
I improved my IDL routine which is used for generating syndynes and synchrones for comets and now it is capable of plotting the grids in J2000 equatorial coordinates. Please note the scale is different in these three graphics. The letter \alpha stands for right ascension and the letter \delta denotes for declination. All in Mercator projection.
Advanced simulation capabilities can model reactors, such as INL's Advanced Test Reactor shown here, from atomic scales to full-sized reactor assemblies.
For more information about INL's research projects and career opportunities, visit the lab's facebook site.
It came out in the usual M9 Kodachrome colours and saturation which does get tedious after a while so I had a go at getting it to a Portra 400 overexposed a stop look.
Advanced simulation capabilities can model reactors, such as INL's Advanced Test Reactor shown here, from atomic scales to full-sized reactor assemblies.
For more information about INL's research projects and career opportunities, visit the lab's facebook site.
Researchers from Michigan State University are using Mira to perform 3-D simulations of the final moments of a core-collapse supernova’s life cycle. This visualization is a volume rendering of a massive star's radial velocity. In comparison to previous 1-D simulations, none of the structure seen here would be present.
Image Credit: Sean Couch, Michigan State University
These simulated CTAO images illustrate the TeV-bright supernova remnant RX J1713 3946 for different emission scenarios. Source: Nakamori T. & et. al (2015). Prospects for CTA Observations of RX J1713.73946. Astroparticle Physics.
Credit: CTAO Consortium
صوره بسيطه عباره عن Ù…Øاكاة الواقع بالخيال
مجسم لقارب وسط ماتبقى من مياه الأمطار ÙŠØاكي
ذلك القارب الØقيقي وسط مياه البØر
اتمنى ان تØوز على رضاكم
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/
A simulation shows what the grocery store aisle looks like to someone with age-related macular degeneration (AMD). AMD damages the macula, a small spot near the center of the eye’s light-sensing retina. The macula lets us see objects that are straight ahead — it’s the part of the eye used for sharp, central vision.
NIH researchers from the National Eye Institute (NEI) profiling epigenomic changes in light-sensing mouse photoreceptors have a clearer picture of how age-related eye diseases may be linked to age-related changes in the regulation of gene expression. The findings, published online April 21, 2020 in Cell Reports, suggest that the epigenome could be targeted as a therapeutic strategy to prevent leading causes of vision loss, such as AMD.
Learn more: www.nih.gov/news-events/news-releases/nei-researchers-lin...
Credit: National Eye Institute, NIH
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
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.
Participants of the 14th World Scout Moot visit the parlament of Canada to have an active role as ambasadors on a UN simulation experience
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
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)
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/
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/
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/
A crude 3D simulation created using StereoPhoto Maker Pro - stereo.jpn.org/eng/stphmkr/ - and Depthy - depthy.stamina.pl/
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