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Peter Menzel Photography
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![Airborne infrared astronomy. Alan Meyer (left) and Roger Hildebrand seen during a flight of the Kuiper Airborne Observatory (KAO). The screen displays show the image made by the alignment telescope (left) and the infrared telescope (right). The KAO is a converted Lockheed C-141A Starlifter aircraft, containing a 90-cm infrared telescope. Flying at up to 12,500 meters, the KAO can cruise well above most of the atmospheric water vapor,, which absorbs far-infrared radiation. The KAO also contains computerized data reduction and analysis stations. Operated by NASA, the first flight of the KAO was in January [1992] NASA AMES Research Center at Moffett Field, Mountain View, California. Infrared telescope looking at gas clouds. [1992]](https://www.menzelphoto.com/img-get2/I0000QSUuCy_gNDY/fill=/fit=180x180/I0000QSUuCy_gNDY.jpg)
![The Natural Resources Defense Council (NRDC]: Seismic Monitor Nuclear test project in The Republic of Kazakhstan. In 1986 the USSR Academy of Sciences allowed the NRDC to install seismic monitoring instruments within a few hundred kilometers of their nuclear test site to verify that the USSR was not testing nuclear weapons underground during the nuclear test ban. By allowing this monitoring on their soil and by monitoring near the Nevada test site in the USA, mutual trust was built that facilitated the end of the Cold War. Jon Berger at the Karkarlinsk Field lab. MODEL RELEASED (1987]](https://www.menzelphoto.com/img-get2/I0000lwQuU_IJ5sM/fill=/fit=180x180/I0000lwQuU_IJ5sM.jpg)
![Physics: Stanford Linear Accelerator Center (SLAC), Menlo Park, California. Control Room [1988]. Instrumentation displays inside the control room of the Stanford Linear Collider (SLC) experiment, Menlo Park, California. With a length of 3km, the Stanford Linear Accelerator is the largest of its kind in the world. The accelerator is used to produce streams of electrons and positrons, which collide at a combined energy of 100 GeV (Giga electron Volts). This massive energy is sufficient to produce Z-zero particles in the collision. The Z-zero is one of the mediators of the weak nuclear force, the force behind radioactive decay, and was first discovered at CERN, Geneva, in 1983. The first Z-zero at SLC was produced on 11 April 1989.](https://www.menzelphoto.com/img-get2/I0000b_6f7D1iczA/fill=/fit=180x180/I0000b_6f7D1iczA.jpg)
![Physics: Stanford Linear Accelerator Center (SLAC), Menlo Park, California. Control Room..Instrumentation displays inside the control room of the Stanford Linear Collider (SLC) experiment, California. With a length of 3km, the Stanford Linear Accelerator is the largest of its kind in the world. The accelerator is used to produce streams of electrons and positrons, which collide at a combined energy of 100 GeV (Giga electron Volts). This massive energy is sufficient to produce Z-zero particles in the collision. The Z-zero is one of the mediators of the weak nuclear force, the force behind radioactive decay, and was first discovered at CERN, Geneva, in 1983. The first Z-zero at SLC was produced on 11 April 1989. [1988]](https://www.menzelphoto.com/img-get2/I0000j1jacgZEQp8/fill=/fit=180x180/I0000j1jacgZEQp8.jpg)
![Alan Weinstein from the Stanford Linear Collider (SLC) experiment, seen with a computer-simulated collision event between an electron and a positron. The SLC produces Z-zero particles by this collision process, which takes place at energies high enough for the electron and positron to annihilate one another, the Z-zero left decaying rapidly into another electron/positron pair or a quark/anti-quark pair. The Z-zero is one of the mediators of the weak nuclear force, the force behind radioactive decay, and was discovered at CERN in 1983. The first Z-zero seen at SLC was detected on 11 April 1989. MODEL RELEASED [1988] Menlo Park, California.](https://www.menzelphoto.com/img-get2/I0000.oMC.oP73Ow/fill=/fit=180x180/I0000.oMC.oP73Ow.jpg)
![Physics: Proton Decay control room. Cleveland, Ohio, Morton Salt Mine proton decay detector located 600 meters underground in the Morton salt mine near Cleveland, Ohio, which consists of a massive tank containing 21 cubic meters of ultra pure water, its walls lined with photomultiplier tubes, which detect faint flashes of Cerenkov light emitted by the passage of charged particles. [1985]](https://www.menzelphoto.com/img-get2/I0000hJiHKLWLWCk/fill=/fit=180x180/I0000hJiHKLWLWCk.jpg)
![Physics: Pat Burchat, with a computer simulation reflected in her glasses at the Stanford Linear Accelerator Center (SLAC) Large Detector. Computer Simulated Event. Stanford Linear Collider (SLC) experiment, Menlo Park, California. With a length of 3km, the Stanford Linear Accelerator is the largest of its kind in the world. The accelerator is used to produce streams of electrons and positrons, which collide at a combined energy of 100 GeV (Giga electron Volts). This massive energy is sufficient to produce Z-zero particles in the collision. The Z-zero is one of the mediators of the weak nuclear force, the force behind radioactive decay, and was first discovered at CERN, Geneva, in 1983. The first Z-zero at SLC was produced on 11 April 1989. MODEL RELEASED [1988]](https://www.menzelphoto.com/img-get2/I0000rpufq2Zpf.A/fill=/fit=180x180/I0000rpufq2Zpf.A.jpg)
