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Tuesday, May 19, 2020 | History

2 edition of Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1 found in the catalog.

Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1

Michael P. Weinreb

Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1

by Michael P. Weinreb

  • 391 Want to read
  • 30 Currently reading

Published by National Environmental Satellite, Data, and Information Service in Washington, D.C .
Written in English

    Subjects:
  • Atmospheric chemistry -- Infrared spectroscopy.,
  • Ozone -- Infrared spectroscopy.

  • Edition Notes

    StatementMichael P. Weinreb, I-Lok Chang.
    SeriesNOAA technical report NESDIS -- 34.
    ContributionsChang, I-Lok., National Environmental Satellite, Data, and Information Service.
    The Physical Object
    Paginationii, 27 p. ;
    Number of Pages27
    ID Numbers
    Open LibraryOL18034989M

      infrared measurements (joint with USGS). Measure ocean surface wind vectors, with the SeaWinds instrument. Collect global data on the state of the atmosphere, land, and oceans, and their interactions with solar radiation and with one another (includes Canadian and Japanese instruments). See TRMM entry for the Ladstatter-Weissenmayer, A. J. Meyer-Arbek, A. Schlemm and J.P. Burrows, , Influence of stratospheric airmasses on tropospheric vertical O 3 columns based on GOME (Global Ozone Monitoring Experiment) measurements and backtrajectory calculation

    Durry, G., Megie, G.: Atmospheric CH 4 and H 2 O monitoring with near-infrared InGaAs laser diodes by the SDLA, a balloonborne spectrometer for tropospheric and stratospheric in situ measurements. :// NASA Images Solar System Collection Ames Research Center. Brooklyn Museum. Full text of "An Introduction To Environmental Chemistry And Pollution"

    NASA Images Solar System Collection Ames Research Center. Brooklyn Museum. Full text of "NASA Technical Reports Server (NTRS) The Atmospheric Effects of Stratospheric Aircraft: a First Program Report" Aaldert van Amerongen, Hélène Krol, Catherine Grèzes-Besset, Tonny Coppens, Ianjit Bhatti, Dan Lobb, Bram Hardenbol, Ruud Hoogeveen Proc. SPIE. ,


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Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1 by Michael P. Weinreb Download PDF EPUB FB2

Get this from a library. Balloon-based infrared solar occultation measurements of stratospheric O₃, H₂O, HNO₃, and CF₂C1₂. [Michael P Weinreb; I-Lok Chang; United States. National Environmental Satellite, Data, and Information Service,]   FUTURE SOLAR OCCULTATION MISSIONS The only HNO occultation instrument currently scheduled to continue stratospheric and upper tropospheric measurements after SCISAT/ACE is SAGE III.

It will be deployed on the ISS in To continue the time series of infrared solar occultation measurements of atmospheric composition,?. Centre for Interdisciplinary Research in Music Media and Technology (McGilll University, CA) Composite Infrared Spectrometer (Cassini) Card Information Structure Commonwealth (or: Confederation) of Independent States (= GUS) Compensated Image System (adaptive Optik/adaptive optics) Computing Infrastructure for Science (NRP) Constant Initial   HNO 3, based on the work of Flaud HNO al., [] AþMIPAS database: Validation of HNO 3 line parameters using MIPAS satellite measurements Aÿ, ACP, 6,I evaluate this new HNO 3 linelist by using it to fit MkIV balloon spectra and PNNL laboratory spectra.

The latter are described by Chackerian et al. JQSRT, 82,Infrared solar spectra recorded between July to March and November with the Fourier transform spectrometer on Kitt Peak (°N latitude, °W longitude, km altitude) have Free tropospheric measurements of formic acid (HCOOH) from infrared ground-based solar absorption spectra: Retrieval approach, evidence for a seasonal cycle, and comparison with model calculations    INTRODUCTION AND CONCLUSIONS General Objectives The "Natural" and "Perturbed" Stratosphere User Requirements For Stratospheric Measurements Science Requirements Mission Evaluations Conclusions Current and Projected Measurement Capability Requirements For Stratospheric Measurements Inversion of the SCIAMACHY measurements enables the amounts and distribution of the atmospheric con- stituents O 3,O 2,O 2(1D), O 4, BrO, OClO, ClO, SO2,H 2CO, NO, NO2,N O [4] Ground-based measurements and climatologies of stratospheric BrO [Fish et al., ; Schofield et al., ] and ClO [Shindell and de Zafra, ] for different solar zenith angles (SZAs) exist.

But these measurements are bound to a single geolocation and have a low-vertical resolution. [5] With its non-sun-synchronous orbit, Superconduct- Rinsland, C.P., (), Long-term stratospheric carbon tetrafluoride (CF 4) increase inferred from infrared space-based solar occultation measurements   Apart from its obvious presence in precipitation, water vapor was the first atmospheric vapor to be identified and was recognized by Aristotle (c.

– BC) in his treatise Meteorologica (Möller ).The first measurement of water vapor content in air is attributed to Nicholas de Cusa (–64), who used a mass balance to measure the change in weight of a sample of wool exposed to   The measurements by Cryogenic Limb Array Etalon Spectrometer (CLAES) and the Improved Stratospheric and Mesospheric Sounder (ISAMS) radiometer on the Upper Atmosphere Research Satellite (UARS), taken in the s, showed systematic day–night differences in several infrared channels that are attributable to non-LTE :// /upper-atmosphere-research-satellite-uars.

The new measurements were performed using stratospheric solar occultation spectra recorded with Fourier transform spectrometer instruments, operated at unapodized spectral resolutions of and /cm.

Title: Long-term trends in the concentrations of SF6, CHClF2, and COF2 in the lower stratosphere from analysis of high-resolution ~rutte/rrweb/rjr-ads/abstracts/   The first comprehensive satellite measurements of stratospheric gases, solar particle and radia- 2O HNO 3 NO 2 ClONO 2 volcanic SO 2 aerosol extinction polar strato-spheric cloud CO HCl BrO ClO HOCl OH HO 2 N 2O 5 5 10 15 20 25 30 40 50 80 OMI: Ozone Monitoring Instrument CF Cl 2 2 CFCl 3 geo-potential Ground-based measurements from We report measurements of hydrogen peroxide (H 2 O 2) profiles from infrared solar occultation spectra recorded at cm À1 resolution by the atmospheric chemistry experiment (ACE) during E.

Arijs's 70 research works with 1, citations and 2, reads, including: Spicam: Spectroscopy for the investigation of the characteristics of the atmosphere of Mars   Abstract: From 17–22 August simultaneous enhancements of ammonia (NH3), carbon monoxide (CO), hydrogen cyanide (HCN), and ethane (C2H6) were detected from ground-based solar absorption Fourier transform infrared (FTIR) spectroscopic measurements at two high-Arctic sites: Eureka (°N, °W) Nunavut, Canada, and Thule (°N An example of the early atmospheric measurements showing large ozone losses over Antarctica is shown in Fig.

These observations of ClO and O 3 were acquired in situ in the stratosphere by scientific instruments flying onboard the NASA ER-2 aircraft in September As the aircraft approached the chemically perturbed air over Antarctica, ClO concentrations rose dramatically, O 3 Roth, and T.

Klüpfel, Ground based measurements of stratospheric OClO, NO 2 and O 3 at Søndre Strømfjord in winter / Geophys Res Lett: 21Google Scholar   LITE was used to measure tropospheric and stratospheric aerosols, clouds, and surface reflectance on a global scale.

The next step in space-based lidar was the ICESat mission, which obtained measurements of aerosol and cloud properties from to Measurements of backscatter from to nm were obtained (Schutz et al., ). A coupled stratospheric chemistry–meteorology model was developed by combining the Canadian operational weather prediction model Global Environmental Multiscale (GEM) with a comprehensive stratospheric photochemistry model from the Belgian Assimilation System for Chemical ObsErvations (BASCOE).

The coupled model was called GEM-BACH for GEM-Belgian Atmospheric ://May, R.D., and C.R. Webster, In situ stratospheric measurements of HNO 3 and HCl near 30 km using the balloon-borne laser in situ sensor tunable diode laser spectrometer. J Geophys Res: 94, 16, CrossRef Google ScholarDirect solar and lunar viewing ground testing to simulate Earth orbit scenarios with the Stratospheric Aerosol and Gas Experiment III (SAGE III) space instrument Systematic program for ground-based Fabry-Perot observations of the neutral hydrogen exosphere.

In-situ stratospheric ozone measurements by means of a fast ozone sensor (FOZAN