Retroreflectors, or corner-cube prisms, are optical devices that return any incident light back in exactly the direction from which it came. The central design concept is a trio of mutually perpendicular surfaces such as is found at the corner of a cube (look up into the corner of the room where the ceiling hits the walls). If these three surfaces are reflective, a light ray will bounce off each in turn, with the net result being a precise 180° turn. (Ever hit a racquetball right into the corner and had it come right back at you?). Retroreflectors are in tail-light covers (feel the sharp bumps on the inside of one), bike reflectors, and in paints for road signs (very tiny crystals). Apollo 11 The Apollo 11 retroreflector array, consisting of 100 corner-cube prisms in a 10×10 array. Each corner cube is made of fused silica (quartz) and is 3.8 cm in diameter. The palette is 0.45 meters square, and carefully designed to minimize thermal gradients across the corner cubes as the array is slammed into and out of the sun's rays as the moon's phase changes. This prevents thermal distortions from seriously degrading the amount of light returned by the reflectors. Apollo 14 The Apollo 14 retroreflector array is very much like the Apollo 11 array in design: 100 3.8 cm reflectors in a 10×10 square pattern. Unlike the picture of the Aollo 11 array, this one has sunlight on its face, enabling a better view of the array of corner cubes. Is that a ziploc bag in the background? Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

Feb 4, 2020 — The objective lens is one of the most important parts of a microscope, since it determines its basic performance and function.

BaslerCameraprice

As we conclude our deep dive into the world of Basler Cameras, it's clear that these innovative imaging solutions stand at the forefront of digital imaging technology. Their exceptional blend of advanced CMOS sensors, versatile connectivity options, and user-friendly software support sets Basler Cameras apart as a leading choice for professionals across a wide spectrum of industries.

The integration of interfaces like USB 3.0, GigE, and Camera Link in Basler Cameras facilitates high-speed data transfer, essential for applications requiring real-time imaging and analysis. This feature is particularly beneficial in dynamic environments where speed and efficiency are paramount, such as in automated production lines or high-traffic monitoring systems.

The Apollo 11 retroreflector array, consisting of 100 corner-cube prisms in a 10×10 array. Each corner cube is made of fused silica (quartz) and is 3.8 cm in diameter. The palette is 0.45 meters square, and carefully designed to minimize thermal gradients across the corner cubes as the array is slammed into and out of the sun's rays as the moon's phase changes. This prevents thermal distortions from seriously degrading the amount of light returned by the reflectors. Apollo 14 The Apollo 14 retroreflector array is very much like the Apollo 11 array in design: 100 3.8 cm reflectors in a 10×10 square pattern. Unlike the picture of the Aollo 11 array, this one has sunlight on its face, enabling a better view of the array of corner cubes. Is that a ziploc bag in the background? Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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Nov 25, 2020 — Hervé Guibert's 'Ghost Image' ... Hervé Guibert's Ghost Image consists of sixty-three mini-essays, some no more than a page or two, which question ...

Basler cameras are not limited to one niche; they thrive across various sectors due to their adaptability and high performance.

The choice of interfaces, including USB 3.0, GigE, and Camera Link, allows for easy integration into existing systems. USB 3.0 offers plug-and-play convenience and high data transfer rates, making it ideal for applications requiring ease of use and speed. GigE provides the advantage of long cable lengths and network integration, suitable for complex industrial environments. Camera Link caters to applications needing high data throughput and minimal latency.

Basler’s commitment to excellence starts with the technology that powers their cameras. By integrating state-of-the-art imaging sensors and offering a variety of interface options, Basler ensures that their cameras can meet the demands of any application.

A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

Apollo 14 The Apollo 14 retroreflector array is very much like the Apollo 11 array in design: 100 3.8 cm reflectors in a 10×10 square pattern. Unlike the picture of the Aollo 11 array, this one has sunlight on its face, enabling a better view of the array of corner cubes. Is that a ziploc bag in the background? Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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Basler VisionCamera

In the realm of digital imaging, Basler stands as a titan, offering a diverse portfolio of high-quality cameras designed to meet the sophisticated demands of industrial, medical, and multimedia applications. With a focus on innovation, reliability, and user satisfaction, Basler cameras are engineered to enhance efficiency, precision, and productivity across various sectors. This blog delves into the world of Basler Cameras, exploring the technology that powers them, their standout features, and the wide array of applications they cater to, shedding light on why they are a top choice for professionals worldwide.

Basler's strategic use of advanced CMOS sensors marks a significant leap in imaging capabilities. These sensors excel in capturing images with high resolution and exceptional clarity, crucial for detailed analysis in industrial inspection, medical diagnostics, and scientific research. Their ability to perform well under various lighting conditions, from the dimly lit labs to brightly illuminated manufacturing floors, underscores their versatility.

For those ready to harness the power of Basler Cameras in their projects, the journey begins at Wilco Imaging. As a trusted distributor of Basler products, Wilco Imaging offers a wide selection of Basler Cameras, ensuring that you find the perfect match for your specific needs. With expert advice, comprehensive support, and a commitment to customer satisfaction, Wilco Imaging is your ideal partner in exploring the vast possibilities that Basler Cameras have to offer!

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Diving deeper into the world of Basler Cameras, we find a blend of cutting-edge technology, unparalleled reliability, and user-centric design that sets these cameras apart from the rest. Let’s explore the core aspects, features, and the wide array of applications that Basler cameras serve, along with a comparative analysis with their competitors, to understand what makes Basler a preferred choice in the digital imaging industry.

Basler cameras are designed not just to capture images but to solve real-world challenges, blending high performance with ease of use.

Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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Ghosts can detect active electronics you have in your hand, even if you're hiding, and will proceed to go to your location and kill you.

The Apollo 14 retroreflector array is very much like the Apollo 11 array in design: 100 3.8 cm reflectors in a 10×10 square pattern. Unlike the picture of the Aollo 11 array, this one has sunlight on its face, enabling a better view of the array of corner cubes. Is that a ziploc bag in the background? Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

From enhancing industrial automation and quality control processes to advancing medical research and improving public safety through traffic and surveillance applications, Basler Cameras deliver unparalleled performance, reliability, and ease of use.

Apollo 11 The Apollo 11 retroreflector array, consisting of 100 corner-cube prisms in a 10×10 array. Each corner cube is made of fused silica (quartz) and is 3.8 cm in diameter. The palette is 0.45 meters square, and carefully designed to minimize thermal gradients across the corner cubes as the array is slammed into and out of the sun's rays as the moon's phase changes. This prevents thermal distortions from seriously degrading the amount of light returned by the reflectors. Apollo 14 The Apollo 14 retroreflector array is very much like the Apollo 11 array in design: 100 3.8 cm reflectors in a 10×10 square pattern. Unlike the picture of the Aollo 11 array, this one has sunlight on its face, enabling a better view of the array of corner cubes. Is that a ziploc bag in the background? Apollo 15 A close-up of the Apollo 15 array, which has 300 3.8 cm corner cubes in a hexagonal array. Because this reflector is three times larger than the previous two, it gets preferential treatment by the photon-challenged LLR stations currently in operation. As of 1994, 6,300 of the 8,400 range measurements (75%) had been made to the Apollo 15 array. APOLLO will have much greater sensitivity, and will consequently visit the various retroreflectors in a more uniformly distributed manner. Lunokhod The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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by DB Sanders · 1996 · Cited by 3654 — bulk of the infrared luminosity for all but the most luminous objects is due to dust heating from an intense starburst within giant molecular clouds. At the ...

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Founded in 1993 as a high-tech manufacturing facility specializing in lighting and audio equipment, Godox has now become a lighting equipment expert and ...

The Soviets landed two rovers on the moon, called Lunokhod 1 and Lunokhod 2, on the Luna 17 and Luna 21 missions in 1970 and 1973, respectively. These rovers were equipped with small retroreflector arrays each consisting of 14 corner cubes of triangular configuration (not cut into a circle—imagine slicing off the corner of a cube with a knife). Each reflector is 11 cm on a side for a total package 44 cm long and 19 cm across. The picture at right of the Lunokhod rover shows the reflector jutting out in front (left). Lunokhod 1 was successfully ranged during its maneuvering phase, but then was not seen for almost 40 years until our project (with the help of the Lunar Reconnaissance Orbiter) re-discovered the reflector in April 2010. Now both Lunokhod reflectors are routinely used, though the large size of the cubes makes them more susceptible to thermal distortions, so that the return is about 30 times weaker in lunar daylight than in lunar night. On the other hand, the larger size makes for a tighter diffraction pattern during lunar night, so the effective cross-section becomes slightly larger than the Apollo 11 and Apollo 14 arrays during these periods. Lunokhod 1 plays by this rule, but Lunokhod 2 has become about five times weaker than its twin reflector. Location of the reflector landing sites APOLLO main page.

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When straight lines are curved inwards in the shape of a barrel is called barrel distortion. Please see the illustrations below for barrel ...

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Basler complements its hardware with the pylon Camera Software Suite, a robust set of tools designed to enhance the user experience. This software suite simplifies camera integration, configuration, and operation, making advanced imaging accessible to users of all skill levels. It enables users to customize settings, process images, and develop tailored solutions for specific projects, showcasing Basler's commitment to supporting its customers' success.