Interferometers Stock Photos and Images

(24)See interferometers stock video clips

Page 1 of 1

Interferometers Stock Photos and Images

The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or mirror segments acting Stock Photo

RM2J3JPXX–The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or mirror segments acting

One of the 8-element radio interferometers, called the Submillimeter Array, located at the top of Mauna Kea volcano, Hawaii. Stock Photo

RFH3G8RW–One of the 8-element radio interferometers, called the Submillimeter Array, located at the top of Mauna Kea volcano, Hawaii.

W M Keck Observatories Mauna Kea at Sunset Stock Photo

RMAB4R6G–W M Keck Observatories Mauna Kea at Sunset

. Anthony piazza, a researcher at NASA’s Armstrong Flight Research center in Edwards, California, works with high-temperature strain sensors. This test article is a bending load bar, which enables high-temperature optical strain sensor research up to 1,800 degrees Fahrenheit. Stock Photo

RM2T2AJ47–. Anthony piazza, a researcher at NASA’s Armstrong Flight Research center in Edwards, California, works with high-temperature strain sensors. This test article is a bending load bar, which enables high-temperature optical strain sensor research up to 1,800 degrees Fahrenheit.

Mauna Kea Space Observatories Keck Observatories Stock Photo

RMAGKX2G–Mauna Kea Space Observatories Keck Observatories

. Bulletin . its use. The instrument is made in two different models. The laboratorytype (PI. VII and fig. 25) is of rigid construction, has gas cham-bers 1 meter long, and is employed for exact gas analysis. It cor-responds to apparatus that use mercury as the confining fluid, andwith which results accurate to 0.02 to 0.03 per cent can be obtained.Some experience is required before one becomes sure of the read-ings. The laboratory type only is discussed here. Mohr, 0., Die Verwandung des zeisschen Interferometers zur technischen Rauch-gasanalyse: Ztschr. angew. Chem., Jahi-g. 25, June 28, 191 Stock Photo

RM2CE0TYJ–. Bulletin . its use. The instrument is made in two different models. The laboratorytype (PI. VII and fig. 25) is of rigid construction, has gas cham-bers 1 meter long, and is employed for exact gas analysis. It cor-responds to apparatus that use mercury as the confining fluid, andwith which results accurate to 0.02 to 0.03 per cent can be obtained.Some experience is required before one becomes sure of the read-ings. The laboratory type only is discussed here. Mohr, 0., Die Verwandung des zeisschen Interferometers zur technischen Rauch-gasanalyse: Ztschr. angew. Chem., Jahi-g. 25, June 28, 191

RM2J3JPNJ–The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or mirror segments acting

Very Large Array or the VLA - Radio Telescopes, Socorro, NM Stock Photo

RM2J3JPXJ–Very Large Array or the VLA - Radio Telescopes, Socorro, NM

RM2T2AJ49–. Anthony piazza, a researcher at NASA’s Armstrong Flight Research center in Edwards, California, works with high-temperature strain sensors. This test article is a bending load bar, which enables high-temperature optical strain sensor research up to 1,800 degrees Fahrenheit.

Dramatic Storm and the VLA - Very Large Array - Radio Telescope in Socorro, New Mexico Stock Photo

RM2PMPNPN–Dramatic Storm and the VLA - Very Large Array - Radio Telescope in Socorro, New Mexico

The X-37 advanced technology demonstrator flaperon unit was one of the first ever thermal and mechanical qualification tests of a carbon-carbon control surface designed for space flight. The test also featured extensive use of high-temperature fiber optic strain sensors. Peak temperatures reached 2,500 degrees Fahrenheit. Stock Photo

RM2WBP3J8–The X-37 advanced technology demonstrator flaperon unit was one of the first ever thermal and mechanical qualification tests of a carbon-carbon control surface designed for space flight. The test also featured extensive use of high-temperature fiber optic strain sensors. Peak temperatures reached 2,500 degrees Fahrenheit.

. Carnegie Institution of Washington publication. CHAPTER VIII. THE LINEAR TYPE OF DISPLACEMENT INTERFEROMETERS. 57. Introductory.—This apparatus will be referred to in various places in this book and presents certain interesting features. The incidence of the grating is normal (I = R = o), and both component rays in their vertical pro- jection lie strictly in the same plane. To make the horizontal projection also collinear is not quite possible in practice, because the direct or unreflected rays and the corresponding spectra would overlap with the spectra of the interferometer. As the former Stock Photo

RMRFRCW5–. Carnegie Institution of Washington publication. CHAPTER VIII. THE LINEAR TYPE OF DISPLACEMENT INTERFEROMETERS. 57. Introductory.—This apparatus will be referred to in various places in this book and presents certain interesting features. The incidence of the grating is normal (I = R = o), and both component rays in their vertical pro- jection lie strictly in the same plane. To make the horizontal projection also collinear is not quite possible in practice, because the direct or unreflected rays and the corresponding spectra would overlap with the spectra of the interferometer. As the former

RM2J3JPY4–The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or mirror segments acting

. Carnegie Institution of Washington publication. CHAPTER V. ynf INTERFEROMETERS FOR PARALLEL AND FOR CROSSED RAYS. 34. Introduction. Methods.—To exchange the component beams of the interferometer, to mutually replace the two pencils which interfere, is not an unusual desideratum, for instance, in the famous experiment of Michelson and Morley. To replace two pencils of component rays, traveling more or less parallel to each other, by pencils moving more or less normal to each other, or to be able to operate upon pencils of corresponding rays (from the same source, crossing each other at any an Stock Photo

RMRFRD2D–. Carnegie Institution of Washington publication. CHAPTER V. ynf INTERFEROMETERS FOR PARALLEL AND FOR CROSSED RAYS. 34. Introduction. Methods.—To exchange the component beams of the interferometer, to mutually replace the two pencils which interfere, is not an unusual desideratum, for instance, in the famous experiment of Michelson and Morley. To replace two pencils of component rays, traveling more or less parallel to each other, by pencils moving more or less normal to each other, or to be able to operate upon pencils of corresponding rays (from the same source, crossing each other at any an

The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or Stock Photo

RME71KYR–The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or

. Carnegie Institution of Washington publication. REVERSED AND NON-REVERSED SPECTRA. 109 distances NG (face toward the light) and MG are equal, the interferences are then easily found by moving the mirror M on the micrometer toward the grating. As compared with the other non-linear interferometers used under like conditions, the present instrument, even when mounted on a y^-inch gas- pipe, RR, showed itself remarkably steady, so that rings could be observed in spite of the tremors of the hill on which the laboratory is built. 59. Film=grating adjustment. Michelson's interferometer.—If the grat Stock Photo

RMRFRCTG–. Carnegie Institution of Washington publication. REVERSED AND NON-REVERSED SPECTRA. 109 distances NG (face toward the light) and MG are equal, the interferences are then easily found by moving the mirror M on the micrometer toward the grating. As compared with the other non-linear interferometers used under like conditions, the present instrument, even when mounted on a y^-inch gas- pipe, RR, showed itself remarkably steady, so that rings could be observed in spite of the tremors of the hill on which the laboratory is built. 59. Film=grating adjustment. Michelson's interferometer.—If the grat

RM2PMPN97–The VLA - Very Large Array - Radio Telescope in Socorro, New Mexico An astronomical interferometer is an array of telescopes or mirror segments acting