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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Meteorology and atmospheric physics 44 (1990), S. 167-194 
    ISSN: 1436-5065
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geography , Physics
    Notes: Summary Low-frequency modes of the monsoon are examined in the context of their radiation balance and diagnosed for the 13-month period between May 1979 and May 1980 using Earth radiation budget and cloud measurements taken by experiments carried on board the Nimbus-7 satellite. Simultaneous observations of the albedo, longwave radiation, absorbed shortwave radiation, and net radiation at the top of the atmosphere (TOA), and the total cloud fraction and cloud-top temperature are considered. The use of broad-band radiation budget measurements permits a description of the observed longwave, shortwave, and net radiative energy exchange by the low-frequency modes. When wavenumber one fields are considered, the entire morphology of the 1979 summer monsoon (pre-onset, onset, break, re-intensification, and withdrawal) can be fully explained in terms of an eastward propagating mode. Ridge passages occurred over the Arabian Sea and India in June prior to onset, during the July break, and during the retreat of the monsoon. Trough passages occurred prior to the onset during a period of increased tropical cyclone activity, at the time of the onset, and immediately following the break. These low-frequency waves can be unambiguously tracked around the world over extended time periods. The latitudinal structure of the waves indicated that a thermally direct Hadley Cell perturbation propagated eastward with the oscillation. These cells were evident from extratropical extensions of the oscillation, each about 180° of longitude out-of-phase with the tropical oscillation. Because the absorbed shortwave and emitted longwave radrative components are in phase and of nearly identical amplitudes, the net radiative effect of the low-frequency mode is small in general. However, in certain latitudinal belts, the passage of the waves induced perturbations in the net radiation. Because longwave cloud-radiative forcing acts in the same direction as latent heat release, it is able to contribute to the diabatic energetics maintaining the structure and propagation of the eastward propagating 30- to 60-day waves. Between trough and ridge, the TOA longwave flux varies in a coherent manner by on the order of 50 to 60 Wm−2.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2003-01-01
    Print ISSN: 0143-1161
    Electronic ISSN: 1366-5901
    Topics: Architecture, Civil Engineering, Surveying , Geography
    Published by Taylor & Francis
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  • 3
    Publication Date: 1990-01-01
    Print ISSN: 0177-7971
    Electronic ISSN: 1436-5065
    Topics: Geography , Physics
    Published by Springer
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  • 4
  • 5
    Publication Date: 2011-08-19
    Description: Nimbus-7 wide-FOV irradiance data collected from 1981-1985 are used to evaluate the effects of the El Chichon eruptions of 1982 on the earth radiation budget. The north polar region displayed a maximum response of 20 percent in the winter of 1982-1983, with the variation being most apparent in the near-IR 2.8 micron and 0.2-3.8 microns shortwave bands. The data indicate that the particle size distribution was constant for a year after eruptions.
    Keywords: GEOPHYSICS
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  • 6
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    In:  Other Sources
    Publication Date: 2011-08-19
    Description: Limits to the accuracy of the Earth Radiation Budget (ERB) data being obtained by the Nimbus-7 satellite are discussed with emphasis on the implications for the measured variabilities in the global climate. Error analyses are performed for both wide and narrow field of view instruments and the success of in-flight calibration efforts is noted. Alterations in the ERB due to the eruptions of El Chichon in 1982 and the 1982-1983 ENSO event are summarized, particularly the teleconnections which were observed during ENSO.
    Keywords: METEOROLOGY AND CLIMATOLOGY
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  • 7
    Publication Date: 2011-08-19
    Description: Nimbus-7 longwave radiation data are analyzed with respect to temporal and spatial changes in the anomalies induced by the El Nino event of 1982-1983. The components and functions of the earth radiation budget (ERB) instruments, which record satellite-altitude irradiances, are described. Local-noon analyses of outgoing longwave radiation (OLR) are presented; interannual variability is observed. El Nino-induced perturbations in the planetary-scale fields which affect OLR are studied. The onset, intensification, expansion, and decay of the OLR associated with El Nino are examined. A comparison of the ERS data with a three month average OLR anomaly map reveals that the ERS data have sufficient accuracy and stability with which to observe OLR anomalies induced by El Nino.
    Keywords: METEOROLOGY AND CLIMATOLOGY
    Type: Monthly Weather Review (ISSN 0027-0644); 114; 415-433
    Format: text
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  • 8
    Publication Date: 2011-08-19
    Description: Over six years of data from the earth-radiation-budget (ERB) experiment on board the Nimbus-7 spacecraft have been received to date. Five years of data have been archived and are readily available to the scientific community, while the sixth year's data will be archived by the fall of 1985. There are three complementary, but independent, data sets: earth-radiation-budget data, solar-irradiance data, and shortwave- and longwave-radiance data suitable for bidirectional-reflectance studies. The solar and the wide-field-of-view earth-flux channels are still recording high-quality data, but the narrow-field-of-view scanner failed after 20 months. The condition of the three data sets is described. In addition, plans for data-set improvement are discussed and a simple algorithm to improve the wide-field-of-view data is presented.
    Keywords: GEOPHYSICS
    Type: American Meteorological Society, Bulletin (ISSN 0003-0007); 66; 1378-138
    Format: text
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  • 9
    Publication Date: 2011-08-18
    Description: In-flight calibration adjustments are developed to process data obtained from the wide-field-of-view channels of Nimbus-6 and Nimbus-7 after the failure of the Nimbus-7 longwave scanner on June 22, 1980. The sensor characteristics are investigated; the satellite environment is examined in detail; and algorithms are constructed to correct for long-term sensor-response changes, on/off-cycle thermal transients, and filter-dome absorption of longwave radiation. Data and results are presented in graphs and tables, including comparisons of the old and new algorithms.
    Keywords: SPACECRAFT INSTRUMENTATION
    Type: Journal of Geophysical Research (ISSN 0148-0227); 89; 5057-507
    Format: text
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  • 10
    Publication Date: 2019-06-28
    Description: Computer simulations of orbital scenarios were performed to examine the effects of orbital altitude, equator crossing time, attitude uncertainty, and orbital eccentricity on ozone observations by future satellites. These effects were assessed by determining changes in solar and viewing geometry and earth daytime coverage loss. The importance of these changes on ozone retrieval was determined by simulating uncertainties in the TOMS ozone retrieval algorithm. The major findings are as follows: (1) Drift of equator crossing time from local noon would have the largest effect on the quality of ozone derived from TOMS. The most significant effect of this drift is the loss of earth daytime coverage in the winter hemisphere. The loss in coverage increases from 1 degree latitude for + or - 1 hour from noon, 6 degrees for + or - 3 hours from noon, to 53 degrees for + or - 6 hours from noon. An additional effect is the increase in ozone retrieval errors due to high solar zenith angles. (2) To maintain contiguous earth coverage, the maximum scan angle of the sensor must be increased with decreasing orbital altitude. The maximum scan angle required for full coverage at the equator varies from 60 degrees at 600 km altitude to 45 degrees at 1200 km. This produces an increase in spacecraft zenith angle, theta, which decreases the ozone retrieval accuracy. The range in theta was approximately 72 degrees for 600 km to approximately 57 degrees at 1200 km. (3) The effect of elliptical orbits is to create gaps in coverage along the subsatellite track. An elliptical orbit with a 200 km perigee and 1200 km apogee produced a maximum earth coverage gap of about 45 km at the perigee at nadir. (4) An attitude uncertainty of 0.1 degree in each axis (pitch, roll, yaw) produced a maximum scan angle to view the pole, and maximum solar zenith angle).
    Keywords: METEOROLOGY AND CLIMATOLOGY
    Type: NASA-CR-4361 , REPT-91B00079 , NAS 1.26:4361
    Format: application/pdf
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