Variations of the relative abundances of He, /C, N, O/ and Fe-group nuclei in solar cosmic rays and their relationship to solar particle acceleration
Explore the source record for details and available documents.
Bertsch, D. L.↗
SEARCH · Search NASA
Results for “Solarize”
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.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
The solar cycle variation of the solar wind helium abundance
Explore the source record for details and available documents.
Ogilvie, K. W.↗
Solar neutrinos and the influence of radiative opacities on solar models
Explore the source record for details and available documents.
Carson, T. R.↗
Impulsive solar X-ray bursts. II - Statistical correlation of observations with solar longitude
Explore the source record for details and available documents.
Petrosian, V.↗
The relationship between solar flares and solar sector boundaries
Explore the source record for details and available documents.
Dittmer, P. H.↗
Study of He I emission lines in the solar atmosphere. III - The triplet-singlet line intensity ratios in solar prominences
Explore the source record for details and available documents.
Heasley, J. N.↗
Temperature variation with latitude in the upper solar photosphere - Relevance to solar oblateness measurements and facular models
Explore the source record for details and available documents.
Ingersoll, A. P.↗
Toward a mathematical model of solar radiation for engineering analysis of solar energy systems
The currently most-used insolation model and what improvements might be made in it to better suit it for use in designing energy systems is discussed. An approach to constructing an upgraded model is sketched.
Hamilton, C. L.↗
Relation of the observed far ultraviolet solar irradiance to the solar magnetic sector structure
Explore the source record for details and available documents.
Heath, D. F.↗
Relation of large-scale coronal X-ray structure and cosmic rays. V - Solar wind and coronal influence on a Forbush decrease lasting one solar rotation
Explore the source record for details and available documents.
Gold, R. E.↗
Observation using interplanetary scintillations at 34.3 MHz of the effect of a solar wind disturbance on a solar energetic particle event
Explore the source record for details and available documents.
Roelof, E. C.↗
Relation of large-scale coronal X-ray structure and cosmic rays. III Low-intensity solar particle events with enhanced nearly 3 MeV helium and medium fluxes associated with solar wind streams
Explore the source record for details and available documents.
Gold, R. E.↗
Solar radiation measurements at NOAA and Solar radiation at Newport, Rhode Island
Explore the source record for details and available documents.
Riches, M. R.↗
Measurement of insolation at DSET and Measurement of the solar constant by PACRAD on Convair 990 flights in 1968 and Spectral measurements of solar intensity and spectrum conditions at high altitudes (5200 to 14000 ft) and arid (Colorado) conditions
Explore the source record for details and available documents.
Zerlaut, G.↗
Determination of diffuse radiation characteristics for application in solar energy harvesting and Low cost, large area solar simulation and Low cost, AM2 simulator
Explore the source record for details and available documents.
Armstrong, B. H.↗
AP-8 trapped proton environment for solar maximum and solar minimum
Data sets from Ov-3 and Azur indicate a need for improvement in models of the stably trapped proton flux with energies between 0.1 and 400 MeV. Two computer accessible models are described: AP8MAX and AP8MIN. The models are presented in the form of nomographs, B-L plots, R-lambda plots, and equatorial radial profiles. Nomographs of the orbit-integrated fluxes are also discussed. The models are compared with each other, with the data, and with previous AP models. Requirements for future improvements include more complete data coverage and periodic comparisons with new data sets as they become available. The machine-sensible format in which the models are available are described.
Sawyer, D. M.↗
Absolute solar ultraviolet intensities and their variations with solar activity. I - The wavelength region 1750-2100 A
Explore the source record for details and available documents.
Brueckner, G. E.↗
Preliminary results from the Orbiting Solar Observatory 8 - Velocities in the solar chromosphere observed in the Si II lambda 1816 line
Explore the source record for details and available documents.
Chipman, E. G.↗