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Books on the topic 'Far-infrared spectra'

Author: Grafiati

Published: 3 June 2025

Last updated: 31 July 2025

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1

Gezari, Daniel Y. Far infrared supplement: Catalog of infrared observations. 2nd ed. National Aeronautics and Space Administration, Scientific and Technical Information Division, 1988.

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2

United States. National Aeronautics and Space Administration., ed. Far-infrared emission line spectroscopy of planetary nebulae from the KAO: Final technical report for NASA airborne astronomy grant NAG 2-372. National Aeronautics and Space Administration, 1994.

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3

A, Harper D., and Ames Research Center, eds. Far-infrared observations of Sagittarius B2: Reconsideration of source structure. National Aeronautics and Space Administration, Ames Research Center, 1985.

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4

Thronson, Harley A. Far-infrared observations of Sagittarius B2: Reconsideration of source structure. National Aeronautics and Space Administration, Ames Research Center, 1985.

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5

A, Harper D., and Ames Research Center, eds. Far-infrared observations of Sagittarius B2: Reconsideration of source structure. National Aeronautics and Space Administration, Ames Research Center, 1985.

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6

United States. National Aeronautics and Space Administration., ed. UV extinction and IR emission in diffuse HII regions: Final technical report, August 15, 1991 - August 14, 1994. National Aeronautics and Space Administration, 1994.

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7

Juanola-Parramon, Roser. A Far-Infrared Spectro-Spatial Space Interferometer. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-29400-1.

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8

George C. Marshall Space Flight Center., ed. Vehicle/atmosphere interaction glows: Far ultraviolet, visible, and infrared. National Aeronautics and Space Administration, Marshall Space Flight Center, 1999.

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9

Q, Ma, and United States. National Aeronautics and Space Administration., eds. Calculation of far wings of allowed spectra: The water continuum. National Aeronautics and Space Administration, 1995.

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10

United States. National Aeronautics and Space Administration, ed. Far-infrared spectral studies from the G.P. Kuiper Airborne Observatory: Final technical report. Center for Radiophysics and Space Research, Cornell University ; [Washington, D.C., 1986.

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11

Harwit, Martin. Far-infrared spectral studies from the G.P. Kuiper Airborne Observatory: Final technical report. Center for Radiophysics and Space Research, Cornell University ; [Washington, D.C., 1986.

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12

Far-infrared emission line spectroscopy of planetary nebulae from the KAO: Final technical report for NASA airborne astronomy grant NAG 2-372. National Aeronautics and Space Administration, 1994.

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13

Far-infrared emission line spectroscopy of planetary nebulae from the KAO: Final technical report for NASA airborne astronomy grant NAG 2-372. National Aeronautics and Space Administration, 1994.

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14

UV extinction and IR emission in diffuse HII regions. National Aeronautics and Space Administration, 1994.

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15

National Aeronautics and Space Administration (NASA) Staff. Far-Infrared Spectral Energy Distributions of Quasars. Independently Published, 2018.

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16

Juanola-Parramon, Roser. Far-Infrared Spectro-Spatial Space Interferometer: Instrument Simulator and Testbed Implementation. Springer International Publishing AG, 2016.

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17

Juanola-Parramon, Roser. Far-Infrared Spectro-Spatial Space Interferometer: Instrument Simulator and Testbed Implementation. Springer, 2016.

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18

Juanola-Parramon, Roser. A Far-Infrared Spectro-Spatial Space Interferometer: Instrument Simulator and Testbed Implementation. Springer, 2018.

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19

Calculation of far wings of allowed spectra: The water continuum. National Aeronautics and Space Administration, 1995.

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20

Doucas, George. Smith-Purcell Radiation. Oxford University PressOxford, 2025. https://doi.org/10.1093/9780198951360.001.0001.

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Abstract Smith–Purcell radiation is the name given to the radiation produced when a charged particle beam, usually electrons, passes close to the surface of a metallic grating. The wavelength of the emitted radiation depends on the period of the grating and on the angle of observation. This makes this phenomenon a very useful tuneable source of radiation in the far-infrared (or THz) part of the spectrum, where tuneable sources are scarce. Moreover, a spectral analysis of the radiation can be used to reconstruct the time profile of the very short (picosecond or sub-picosecond) electron bunches

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