Spurious Late Historical‐Era Warming in CESM2 Driven by Prescribed Biomass Burning Emissions
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J. T. Fasullo↗
SEARCH · Engineering Papers
Results for “LaTe”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Massive stars dying alone: the remote environment of supernova 2010jp and its associated late-time source
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Austin Corgan↗
Simulating Chemical Abundances in the Circumstellar Nebula of the Late Stage Binary RY Scuti
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Sarah H. Taft↗
Fundamental geochemical research on tektites, stony meteorites, and radiation damage in re- lated silicate materials quarterly report, jul.1 - dec. b6, 1961 /two quarters/
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Cohen, A. J.↗
Theoretical study of air forces on an oscil- lating or steady thin wing in a supersonic main stream
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Garrick, I. E.↗
Case of late manifestation of intrapulmonary pressure
Recompression treatment of intrapulmonary pressure trauma
RESPIRATORY SYSTEM↗
Upper-bound estimate of the incidence of large sferic sources in certain areas of the United States in late 1959.
Lightning discharge radiating sferics near Gulf of Mexico and west coast of U.S.
ATMOSPHERICS↗
First U.S.-ESRO satellite launch late this month
Telemetry, antenna, command, power, solar array, battery, attitude control, spin-up, de-spin, housekeeping, and thermal control systems for ESRO II satellite - press kit release
SUBSYSTEM↗
Model atmospheres for late-type stars.
Stellar atmosphere model constructed to test opacity effect due to water vapor on model atmosphere structures
Auman, J. R., Jr.↗
Late-time source of atomic light in the helium afterglow.
Time dependent behavior of atomic light emitted from pulsed helium afterglow, noting absorption measurements and spectrometric system
Collins, C. B.↗
Departures from LTE in the hydrogen lines of late B stars.
Atomic hydrogen departures from LTE computed for models of B star atmospheres, assuming detailed balance in hydrogen lines
Peterson, D. M.↗
Photometry of late type stars
Broad band filter photometry for 57 bright stars of spectral type A2 discussed with peak instrument responses at 3320, 2980, 2460 and 1910 A. The data include nearly all usable filter observations of G, K and M types. Sampling is nearly complete for A and F giants and supergiants, with the exception of Cepheid variables. The basic results presented are relative digital counting rates obtained with a field-stop aperture of 10 minutes of arc. Characteristics of the four filter-photometer combinations and errors are discussed. Some observations require substantial correction if they are to represent the visually brightest star in the field. These corrections and the effects of interstellar reddening are discussed. The adjusted counts are then used to construct color-color diagrams and are compared to the recent SAO grid of model atmospheres.
Doherty, L. R.↗
Late Effects in Man Following Exposure to Ionizing Radiations
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Grahn, D.↗
Abundances in late-type giants.
The narrow-band photometry of Spinrad and Taylor (1969) is analyzed by the synthetic spectra technique. Surface gravities, Doppler broadening velocities, effective temperatures, and metal abundances are determined for 131 K giants. Evolutionary tracks and gravities determined from the photometry are used to give space positions, space velocities, and absolute magnitudes of the 131 stars. We conclude that a class of stars exists with metals and/or nitrogen significantly enhanced with respect to the sun; further that these stars have average space motions similar to those of moderately old Population I stars. The Doppler broadening velocity is found to be a strong function of temperature for K giants, and in some cases, possibly a function of surface gravity.
Gottlieb, D. M.↗
Ultraviolet photometry from the orbiting astronomical observatory. IV - Photometry of late-type stars.
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Doherty, L. R.↗
Late Precambrian microfossils - A new stromatolitic biota from Boorthanna, South Australia.
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Schopf, J. W.↗
A comparison of cosmic ray anisotropies and interplanetary magnetic field data late in a solar flare
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Allum, F. R.↗
Time variations in the OH microwave and infrared emission from late-type stars
The results of a study initiated in the fall of 1969 are reported. The study was concerned with the monthly measurement of the microwave spectra at 1612 MHz and the broadband infrared fluxes at six wavelengths for 10 OH/IR sources. The observations represent the first conclusive evidence for well-defined, periodic variations in the flux from any type of OH microwave emitter. Following the discovery of OH/IR stars that emit mainly at 1665 and/or 1667 MHz the program was expanded to include four of these sources.
Harvey, P. M.↗