'Synchrotron' Bilder und Clips Suchergebnisse page 1 of 1

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Erweiterte Suche Suchtipps

Bilder zu 'Synchrotron' gefunden, 14

Accelerator Saturne Synchrotron Made in France in 1979 (photo)

Accelerator Saturne Synchrotron Made in France in 1979 (photo)

Unknown photographer, (20th century)

XRF1655229

Switzerland Cern, 1958 (b/w photo)

Switzerland Cern, 1958 (b/w photo)

Gassmann

KES6253846

Switzerland Cern, 1976 (b/w photo)

Switzerland Cern, 1976 (b/w photo)

Stringer (STR)

KES6253833

Switzerland Cern, 1976 (b/w photo)

Switzerland Cern, 1976 (b/w photo)

Stringer (STR)

KES6253832

High angle view of a synchrotron in a laboratory, California Institute of Technology, Pasadena, California, USA

High angle view of a synchrotron in a laboratory, California Institute of Technology, Pasadena, California, USA

SSI2176718

John Adams, leader of the construction team of Proton Synchrotron which accelerated particles to 24 GeV, 24 November 1959 (b/w photo)

John Adams, leader of the construction team of Proton Synchrotron which accelerated particles to 24 GeV, 24 November 1959 (b/w photo)

UIS3506778

Magnet Synchrotron Radiation at Atomic Center of Frascati, Italy 1958 (b/w photo)

Magnet Synchrotron Radiation at Atomic Center of Frascati, Italy 1958 (b/w photo)

UIT6190624

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Franco Vitale

MEP1763291

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Franco Vitale

MEP1763289

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Rainier III and Grace Kelly visiting the Synchrotron of Frascati, Frascati, Italy, 1959 (b/w photo)

Franco Vitale

MEP1763292

Switzerland Prince Philip, 1960 (b/w photo)

Switzerland Prince Philip, 1960 (b/w photo)

Stringer (STR)

KES6243710

Switzerland Television, 1962 Director of Cern (b/w photo)

Switzerland Television, 1962 Director of Cern (b/w photo)

Krebs

KES6252679

Collision of a sulphur ion with a gold nucleus - A sulphur ion collides a gold nucleus - A sulfur ion of 6400 GeV hits a nucleus in a gold target. The resulting particle rain is recorded in a chamber with bright wake. Experience NA35 of the CERN Super Proton Synchrotron (SPS) accelerator. In this image the real particles produced by the collision of a 6400 GeV sulphur ion with a gold target can be seen as they pass through a streamer chamber. Streamer chambers consist of a gas chamber through which a strong pulsed electric field is passed, creating sparks as a charged particle passes through it. The NA35 experiment, which was in operation in the 1980s, was part of CERN's ongoing heavy ion project

Collision of a sulphur ion with a gold nucleus - A sulphur ion collides a gold nucleus - A sulfur ion of 6400 GeV hits a nucleus in a gold target. The resulting particle rain is recorded in a chamber with bright wake. Experience NA35 of the CERN Super Proton Synchrotron (SPS) accelerator. In this image the real particles produced by the collision of a 6400 GeV sulphur ion with a gold target can be seen as they pass through a streamer chamber. Streamer chambers consist of a gas chamber through which a strong pulsed electric field is passed, creating sparks as a charged particle passes through it. The NA35 experiment, which was in operation in the 1980s, was part of CERN's ongoing heavy ion project

PIX4650601

Remains of the Crab Supernova (M1) in the Taurus - M1, the Crab Nebula, is a supernova remnant from a star that exploded in July or August of 1054 AD and was witnessed and described by Chinese astronomers as being six times brighter than Venus. The supernova, located in the constellation of Taurus and about 7,000 light years away from the Earth, shined with the light of 400 million suns, was visible in the daytime for almost a month, and remained visible in the evening sky for more than a year. Today, some 900 years later, we see the remains of the exploded star as a cloud of gaseous debris, illuminated by the remnants of the core of the original star, which is now a rapidly spinning neutron star called a pulsar. The colors in the nebula come from two different sources. The red filaments come from typical hydrogen emission such as in emission nebula like M8. The diffuse blue background has a continuous spectrum composed of synchrotron radiation which is emitted by high energy electrons

Remains of the Crab Supernova (M1) in the Taurus - M1, the Crab Nebula, is a supernova remnant from a star that exploded in July or August of 1054 AD and was witnessed and described by Chinese astronomers as being six times brighter than Venus. The supernova, located in the constellation of Taurus and about 7,000 light years away from the Earth, shined with the light of 400 million suns, was visible in the daytime for almost a month, and remained visible in the evening sky for more than a year. Today, some 900 years later, we see the remains of the exploded star as a cloud of gaseous debris, illuminated by the remnants of the core of the original star, which is now a rapidly spinning neutron star called a pulsar. The colors in the nebula come from two different sources. The red filaments come from typical hydrogen emission such as in emission nebula like M8. The diffuse blue background has a continuous spectrum composed of synchrotron radiation which is emitted by high energy electrons

Jerry Lodriguss

PIX4583001

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