Author: Crofton B. Farmer
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 544
Book Description
A High-resolution Atlas of the Infrared Spectrum of the Sun and Earth Atmosphere from Space
Author: Crofton B. Farmer
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 544
Book Description
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 544
Book Description
A High-resolution Atlas of the Infrared Spectrum of the Sun and Earth Atmosphere from Space: Key to identification of solar features
Author: Crofton B. Farmer
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 768
Book Description
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 768
Book Description
A High-resolution Atlas of the Infrared Spectrum of the Sun and Earth Atmosphere from Space: The Sun
Author: Crofton B. Farmer
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 694
Book Description
Publisher:
ISBN:
Category : Infrared spectra
Languages : en
Pages : 694
Book Description
A High-Resolution Atlas of the Infrared Spectrum of the Sun and the Earth Atmosphere from Space. Volume 3
Author: National Aeronautics and Space Administration (NASA)
Publisher: Createspace Independent Publishing Platform
ISBN: 9781723498411
Category :
Languages : en
Pages : 464
Book Description
During the period April 29 through May 2, 1985, the Atmospheric Trace Molecule Spectroscopy (ATMOS) experiment was operated as part of the Spacelab-3 (SL-3) payload on the shuttle Challenger. The instrument, a Fourier transform spectrometer, recorded over 2000 infrared solar spectra from an altitude of 360 km. Although the majority of the spectra were taken through the limb of the Earth's atmosphere in order to better understand its composition, several hundred of the 'high-sun' spectra were completely free from telluric absorption. These high-sun spectra recorded from space are, at the present time, the only high-resolution infrared spectra ever taken of the Sun free from absorptions due to constituents in the Earth's atmosphere. Volumes 1 and 2 of this series provide a compilation of these spectra arranged in a format suitable for quick-look reference purposes and are the first record of the continuous high-resolution infrared spectrum of the Sun and the Earth's atmosphere from space. In the Table of Identifications, which constitutes the main body of this volume, each block of eight wavenumbers is given a separate heading and corresponds to a page of two panels in Volume 1 of this series. In addition, three separate blocks of data available from ATMOS from 622-630 cm(exp -1), 630-638 cm(exp -1) and 638-646 cm(exp -1), excluded from Volume 1 because of the low signal-to-noise ratio, have been included due to the certain identification of several OH and NH transitions. In the first column of the table, the corrected frequency is given. The second column identifies the molecular species. The third and fourth columns represent the assigned transition. The fifth column gives the depth of the molecular line in millimeters. Also included in this column is a notation to indicate whether the line is a blend or lies on the shoulder(s) of another line(s). The final column repeats a question mark if the line is unidentified. Geller, Murray Jet Propulsion Laboratory NASA-RP-1...
Publisher: Createspace Independent Publishing Platform
ISBN: 9781723498411
Category :
Languages : en
Pages : 464
Book Description
During the period April 29 through May 2, 1985, the Atmospheric Trace Molecule Spectroscopy (ATMOS) experiment was operated as part of the Spacelab-3 (SL-3) payload on the shuttle Challenger. The instrument, a Fourier transform spectrometer, recorded over 2000 infrared solar spectra from an altitude of 360 km. Although the majority of the spectra were taken through the limb of the Earth's atmosphere in order to better understand its composition, several hundred of the 'high-sun' spectra were completely free from telluric absorption. These high-sun spectra recorded from space are, at the present time, the only high-resolution infrared spectra ever taken of the Sun free from absorptions due to constituents in the Earth's atmosphere. Volumes 1 and 2 of this series provide a compilation of these spectra arranged in a format suitable for quick-look reference purposes and are the first record of the continuous high-resolution infrared spectrum of the Sun and the Earth's atmosphere from space. In the Table of Identifications, which constitutes the main body of this volume, each block of eight wavenumbers is given a separate heading and corresponds to a page of two panels in Volume 1 of this series. In addition, three separate blocks of data available from ATMOS from 622-630 cm(exp -1), 630-638 cm(exp -1) and 638-646 cm(exp -1), excluded from Volume 1 because of the low signal-to-noise ratio, have been included due to the certain identification of several OH and NH transitions. In the first column of the table, the corrected frequency is given. The second column identifies the molecular species. The third and fourth columns represent the assigned transition. The fifth column gives the depth of the molecular line in millimeters. Also included in this column is a notation to indicate whether the line is a blend or lies on the shoulder(s) of another line(s). The final column repeats a question mark if the line is unidentified. Geller, Murray Jet Propulsion Laboratory NASA-RP-1...
NASA Scientific and Technical Publications
NASA Reference Publication
Scientific and Technical Aerospace Reports
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 1460
Book Description
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 1460
Book Description
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
Radiative Transfer in the Atmosphere and Ocean
Author: Gary E. Thomas
Publisher: Cambridge University Press
ISBN: 9780521890618
Category : Nature
Languages : en
Pages : 554
Book Description
Provides a foundation of the theoretical and practical aspects of radiative transfer, for the atmospheric, oceanic and environmental sciences.
Publisher: Cambridge University Press
ISBN: 9780521890618
Category : Nature
Languages : en
Pages : 554
Book Description
Provides a foundation of the theoretical and practical aspects of radiative transfer, for the atmospheric, oceanic and environmental sciences.
Infrared Solar Physics
Author: D.M. Rabin
Publisher: Springer Science & Business Media
ISBN: 9401119260
Category : Science
Languages : en
Pages : 587
Book Description
Infrared Solar Physics contains the proceedings of the 154th Symposium of the International Astronomical Union held in Tucson, Arizona, March 2--5, 1992. Aimed at active workers and graduate students in solar physics, this volume provides the first comprehensive view of a rapidly expanding discipline that gives us a new perspective on the sun. Measurements across the wide infrared spectral range -- here, from 1 mum to 1 mm -- can probe the solar atmosphere from below the visible surface through the outer reaches of the corona. Taking full advantage of revolutionary advances in detector technology, infrared observations from the ground, aircraft and space have led to a better understanding of solar magnetic fields, atmospheric structure and activity, and elemental abundances. The infrared has also provided new interpretive challenges, such as the appearance of the 12-mum emission lines of magnesium. These and other developments are discussed here by the leading contributors to the field, who also give their perspectives on the future of this rich field of study.
Publisher: Springer Science & Business Media
ISBN: 9401119260
Category : Science
Languages : en
Pages : 587
Book Description
Infrared Solar Physics contains the proceedings of the 154th Symposium of the International Astronomical Union held in Tucson, Arizona, March 2--5, 1992. Aimed at active workers and graduate students in solar physics, this volume provides the first comprehensive view of a rapidly expanding discipline that gives us a new perspective on the sun. Measurements across the wide infrared spectral range -- here, from 1 mum to 1 mm -- can probe the solar atmosphere from below the visible surface through the outer reaches of the corona. Taking full advantage of revolutionary advances in detector technology, infrared observations from the ground, aircraft and space have led to a better understanding of solar magnetic fields, atmospheric structure and activity, and elemental abundances. The infrared has also provided new interpretive challenges, such as the appearance of the 12-mum emission lines of magnesium. These and other developments are discussed here by the leading contributors to the field, who also give their perspectives on the future of this rich field of study.
Infrared Tools For Solar Antrophysics: What's Next? - Proceedings Of The Fifteenth National Solar Observatory/sacramento Peak Summer Workshop
Author: Jeffrey R Kuhn
Publisher: World Scientific
ISBN: 9814549487
Category :
Languages : en
Pages : 486
Book Description
These proceedings sample new results derived from extended-objected IR observations and explore the capabilities of large-aperture, low-scattered-light instrumentation. The latest results from IR solar observations are described and a broad range of night-time problems from gravitational lens detection to planetary detection are explored in the context of what capabilities a large reflecting coronagraphic telescope could offer.
Publisher: World Scientific
ISBN: 9814549487
Category :
Languages : en
Pages : 486
Book Description
These proceedings sample new results derived from extended-objected IR observations and explore the capabilities of large-aperture, low-scattered-light instrumentation. The latest results from IR solar observations are described and a broad range of night-time problems from gravitational lens detection to planetary detection are explored in the context of what capabilities a large reflecting coronagraphic telescope could offer.