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  • SPACE RADIATION  (929)
  • 1990-1994
  • 1980-1984  (129)
  • 1970-1974  (800)
  • 1930-1934
  • 1981  (129)
  • 1972  (429)
  • 1971  (371)
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  • 1990-1994
  • 1980-1984  (129)
  • 1970-1974  (800)
  • 1930-1934
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  • 1
    Publication Date: 2005-11-30
    Description: The range and Doppler radio tracking close to the sun made it possible to measure solar plasma dynamics. These were measured by means of a method known as differenced range versus integrated Doppler, which exploits the opposite change of group and phase velocity as the plasma density changes along the radio raypath. A simple solar plasma propagation model is proposed.
    Keywords: SPACE RADIATION
    Type: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 105-110
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  • 2
    Publication Date: 2005-11-30
    Description: The GE experiment consisted of two types of detectors: plastics and glasses located in panel 2 and the lower half of panel 3. In panel 2, the entire exposed detector area of 14.7 by 22.6 cm was composed of 31 sheets of 0.025-cm polycarbonate plastic 9070-112. In panel 3, 39 sheets of 0.02-cm cellulose triacetate with no plasticizer made up the major volume fraction. The lower part of panel 3 contained five types of glass detectors. Particles that entered the array after it was folded were recognized, if they crossed from one sheet to another, by means of a 2-mm relative shift of alternate sheets.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 9 p
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  • 3
    Publication Date: 2005-11-30
    Description: During the Apollo 16 mission, a solar flare produced an enormous amount of low-energy nuclei, many orders of magnitude greater than the level inferred from studies of tracks in the window of the Apollo 12 spacecraft during a time when the sun was quiet. The differential energy spectrum of nuclei with Z less than or equal to 6 falls by seven orders of magnitude over the interval from 0.1 to 20 MeV/nucleon, then remains almost flat up to approximately 100 MeV/nucleon. The two parts correspond to contributions from the sun and from galactic cosmic rays. Any maximum in the spectrum occurs below the lowest energy studied.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 8 p
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  • 4
    Publication Date: 2005-11-30
    Description: All mineral detectors exposed on Apollo 16 had high surface track densities probably produced by a solar flare that occurred during the mission. The heavy ions followed a power law spectrum with exponent approximately 3 down to approximately 200 KeV/nucleon. The abundance of low-energy particle tracks observed in this flare may explain the high track densities observed in lunar dust grains. Pristine heavy-particle tracks in feldspar give long tracks. Shallow pits similar to those expected from extremely heavy solar wind ions were observed in about the expected number. Initial results give a low apparent value of neutron albedo relative to theory.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 14 p
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  • 5
    Publication Date: 2005-11-30
    Description: Investigations on the Fe-group nuclei track density vs depth in lunar rocks and Surveyor 3 TV camera filter glass were critically examined considering more factors than previously. The analysis gives a firmer basis to the observation of the preferential leakage of low energy Fe nuclei from the accelerating region of the sun. The track density gradients in lunar rock 12022 and filter glass are used to determine the lunar erosion rate of 3 angstroms/yr. Track gradients are less steep than predicted from energy spectrum observed in the Surveyor glass, perhaps due to sputtering. High densities of etchable tracks were found at all depths down to 60 cm in fines from Apollo cores and also in thin sections of the Pesjanoe, Pantar, and Fayetteville gas-rich meteorites. It is felt unlikely that suprathermal heavy ions were responsible for the high track densities.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 221-226
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  • 6
    Publication Date: 2005-11-30
    Description: Particle tracks were investigated in the glass plate of a neutral density (clear flint) optical filter housed in the Surveyor 3 TV camera but exposed directly to space. The track density vs depth curve was determined and descends sharply from approximately 2.6 million tracks/sq cm at a depth of 3.6 mg/sq cm to about 35/sq cm at 700 mg/sq cm. Several tracks were of V-shapes characteristic of high energy induced fission. The erosion rate on the moon due to solar wind ions was determined from the energy spectrum, and was found to be low (0 to 2 x 10 to the minus 8th power cm/yr).
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 213-216
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  • 7
    Publication Date: 2005-11-30
    Description: The proton-produced Na-22 content of samples of Surveyor 3 TV camera, surface sampler scoop, and other components was determined by nondestructive gamma ray spectrometry. The contributions of the nine most prominent solar flares to Na-22 production were calculated to be 18 dpm/kg. The observed activity in the Surveyor 3 samples was 62 + or - dpm/kg. This indicates a galactic proton contribution of about 44 dpm/kg, which adjusted for spallation of Al gives a value of 42 dpm/kg. This is compared to measurements of 88 dpm/kg in the Lost City meteorite which had an orbit extending to 2.35 AU, with a 4 pi bombardment as compared to the 2 pi bombardment of the samples on the lunar surface. The agreement between Na-22 production in Surveyor 3 and the Lost City meteorite offers evidence that the galactic cosmic ray flux is almost the same at 1 Au and at 2.35 AU.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 196-200
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  • 8
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    Publication Date: 2005-11-30
    Description: Nimbus 3 and 4 observations of ultraviolet active regions of the sun have been investigated. It is not clear what is producing these UV-active regions, however, it could be changes in the overall intensity of the solar continuum near the region of the temperature minimum, or the solar flux variations that have been seen could be due to a continuous type of absorption like that associated with the ionization limits of elements such as aluminum, silicon, or magnesium.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 159-163
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  • 9
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    Publication Date: 2005-11-30
    Description: Intuition regarding the stability of MHD tangential discontinuities of solar wind has been borne out by a linear stability analysis of the MHD equations. In performing the calculation, the model used had no plasma flow and thus corresponded to the solar wind rest frame. The method calculated the change in total energy, plasma plus magnetic, due to the perturbation. This type of stability analysis is analogous to the test of the stability of an equilibrium point in a mechanical potential.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 134-139
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  • 10
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    Publication Date: 2005-11-30
    Description: The ability of a theoretical solar wind model to predict the energy flux density due to heat conduction was investigated. In order to demonstrate this capability, the analysis used simultaneous data from the electron plasma experiment of Ogilvie and Lind, and the vector magnetic field data of Heppner and Sugiura on OGO-5. On the strength of two independent, different, and consistent experimental determinations of the conduction of heat flux by electrons at 149.6 gigameters(1 AU), it was determined that the models for the solar wind must be able to predict a value for the heat conduction in the range 0.007 to 0.008 in order to be in agreement with the observations.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 144-148
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  • 11
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    Publication Date: 2005-11-30
    Description: The process of solar flare acceleration of interplanetary particles, as measured by the fifth orbiting solar observatory, is explained. Data show the acceleration proceeds in two stages: (1) particle acceleration by induced electric fields arising from annihilating magnetic fields at the beginning stages of flares, and (2) a Fermi acceleration mechanism operating in a shock front produced by the flare.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 171-175
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  • 12
    Publication Date: 2005-11-30
    Description: Motion in the general gravity field is described mathematically. A covariance analysis, based on two simple models, is presented. Two drag-free space probes were considered, for which the orbital elements are given.
    Keywords: SPACE RADIATION
    Type: JPL Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 242-244
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  • 13
    Publication Date: 2005-11-30
    Description: Motion of a space probe about a spherical center of attraction is considered, applying the general theory of relativity. Motion of a probe under the influence of the sun's oblateness is also discussed. Estimates of beta, gamma, and J20 using solar probe motion are presented. It is concluded that such measurements are possible if the unknown long-period perturbing acceleration is of the order of 10 to the -11th or -12th power m/sec. sq.
    Keywords: SPACE RADIATION
    Type: JPL Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 222-227
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  • 14
    Publication Date: 2005-11-30
    Description: Results from interferometric measurements of the apparent angular deflection of quasi-stellar object are examined. Some preliminary results from Mariner 6 and 7 experiments, particularly from the plasma effect viewpoint, are discussed, along with future experiments and plasma scintillation. Ray bending studies, plasma relativity separation for Mariner 6 and 7, and radio propagation test of general relativity are reviewed. First order approximations and time delay studies are appended, as well as Doppler velocity effect investigations.
    Keywords: SPACE RADIATION
    Type: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 92-104
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  • 15
    Publication Date: 2005-11-30
    Description: The technique for obtaining range measurements is discussed. It involves measuring elapsed time between the transmission of an encoded signal from the ground station and its return from the spacecraft. The theoretical background for the Mariner Mars 1969 relativity test is presented, including computation of orbits and time transformation. Interplanetary and coronal plasma effects on range and Doppler observations at S-band are also considered. The general relativistic propagation delay was measured and a value of 0.997 for the relativity parameter Gamma star was obtained.
    Keywords: SPACE RADIATION
    Type: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 111-135
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  • 16
    Publication Date: 2005-11-30
    Description: Samples of glass from the Surveyor 3 TV camera filter were examined for particle tracks by optical and scanning electron microscopy. The corrected density value is 1.7 million + or - 0.1 million tracks/sq cm, and the track density vs depth curve is determined. Comparisons with other estimated and calculated data are discussed, and lack of agreement between data sets is considered. It is felt that considerable erosion occurs, and that erosion also occurs by a flaking of small thicknesses of material, possibly caused by solar wind irradiation.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 209-212
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  • 17
    Publication Date: 2005-11-30
    Description: A silica glass window from Apollo 12 CM and a piece of flint glass from the Surveyor 3 camera filter were examined for Fe nuclei tracks. A large difference between observed and predicted track densitites was found. At low rigidity (or energy), the solar particle Fe/He ratio is much higher than the photospheric abundance ratio, but decreases with increasing rigidity until it approaches the photospheric value at a rigidity of about 500 MV. It is felt that the low-energy Fe tracks are of solar origin. The implications that heavy nuclei can be preferentially emitted from a source of energetic particles are discussed. Other conclusions are the following: Rocks exposed on the lunar surface for 10 million yr would accumulate about 6 x 10 to the 12th power tracks/sq cm, and the rate of radiation-induced erosion is about 10 to the -9 cm/yr. The lunar soil should contain heavily irradiated small grains, some with track densities of about 10 to the 12th power/sq cm that have flaked from radiation-damaged rock surfaces and some that were irradiated while at the top of the soil layer.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 217-220
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  • 18
    Publication Date: 2005-11-30
    Description: The first exposure on a spacecraft of a nuclear emulsion apparatus designed to collect 1000 high quality tracks of heavy nuclei under a negligible thickness of matter (0.07 g/sq cm) is described. The cosmic ray detector consisted of a stack of nuclear emulsions that were designed to register at least 400 heavy nuclei tracks for each 10 hours of useful exposure. The spacecraft had to be oriented in a heads-up attitude during the 10-hour period to eliminate atmospheric albedo particles. The results are as follows: (1) a definite odd-even effect, with low abundances for elements of atomic number 7, 9, and 11; (2) a ratio O/C approximately 0.9; (3) Ne/C, Mg/C, and Si/C ratios between 0.2 and 0.3; (4) an abundance gap in the region 15 less than or equal to Z less than or equal to 19; and (5) a ratio (20 less than or equal to Z less than or equal to 28)/C 0.2, with a large concentration at Z = 26. These results are indicative that successful exposures of nuclear emulsions were obtained on the Gemini 11 mission.
    Keywords: SPACE RADIATION
    Type: NASA. Manned Spacecraft Center The Gemini Program: Phys. Sci. Expt. Sum.; p 215-225
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  • 19
    Publication Date: 2005-11-30
    Description: The Apollo 16 SWC experiment is a continuation of the earlier experiments; however, an essential change was introduced in the solar wind particle collection technique. Platinum surfaces were incorporated in the collector foil, and use was made of a layer technique for distinguishing particles of different energies and different directions of arrival. The improvements and the expanded scope of the Apollo 16 experiment, relative to the earlier SWC experiments, can be summarized as follows: elimination of possible residual dust contamination by treating the platinum foil sections with dilute hydrofluoric acid before analysis; increased accuracy of solar wind argon abundance; determination of solar wind albedo; and search for helium in the energy range above approximately 40 KeV/nucleon.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 10 p
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  • 20
    Publication Date: 2005-11-30
    Description: The passionate dream of the oppressed solar flare forecaster is the scientific discovery of the cause, the energy source, and the observable antecedent conditions for the solar flare. This tunnel vision has had a profound and deleterious effect on the state-of-the-art. It has diverted attention from many promising approaches and relegated them to limbo. More importantly, it has actually inhibited the scientific search for the underlying physical mechanisms. Examples of neglected aspects of the problem cover the entire range from observing techniques and equipment to the availability and accuracy of the archived scientific data. A cursory inspection of this data leads to an obvious conclusion: there are at least two suns up there.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Phys. of the Space Environment; p 157-171
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  • 21
    Publication Date: 2005-11-30
    Description: The He-4 and Ne-20 contents in sections of the Surveyor 3 support strut samples were determined by optical and scanning electron microscopy and are compared to the results of the Apollo solar wind composition (SWC) experiments. The He-4/Ne-20 ratio in the samples from the sunlit side of the strut was approximately 300; the ratios determined in Apollo 12 lunar fines and SWC foil were below 100. The He-4/He-3 ratios were also determined, and the ratio obtained from Surveyor 3 material is higher than those found with Apollo 11 and 12 SWC experiments. The effects of spallation by cosmic rays or solar protons, stripping by cosmic ray or energetic solar alpha particles, recycling of solar wind He and radiogenic Ne, He from terrestrial atmosphere, mass discrimination near the moon, mass dependence of trapping probability, diffusion, and contamination by lunar dust are considered.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 201-208
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  • 22
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    Publication Date: 2005-11-30
    Description: The results of an investigation on the effects of earth seasonal changes on solar activity, particularly sunspots, are given. These results show corpuscular and electromagnetic activity increased during the equinoctial months. In addition the electromagnetic aspect tends to increase during the winter months. It was suggested that seasonal changes in sunspot numbers may be caused by the tidal forces and the processional torques exerted by the various planets in the solar atmosphere.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 164-170
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  • 23
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    Publication Date: 2005-11-30
    Description: Hydromagnetic heating in the solar wind was investigated using the heating model in which fast-mode hydromagnetic waves propagate outward from below the base and deposit energy by collisionless damping. Ray paths were found by solving Hamilton's equations. As the ray propagates along its path, it will damp, supplying thermal energy to the solar wind gas. The strong agreement of these results with observations is clear indication that the primary nonthermal heat source in the solar wind is the collisionless damping of hydromagnetic waves.
    Keywords: SPACE RADIATION
    Type: Significant Accomplishments in Sci., 1970; p 140-143
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  • 24
    Publication Date: 2006-08-20
    Keywords: SPACE RADIATION
    Type: Res. in the Space Sci., v. 2; 10 p
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  • 25
    Publication Date: 2006-04-26
    Description: A method is examined for calculating the error of experimental data from a standard neutron monitor with the multiplicity of neutron generation. It is shown that use of the Poisson distribution to estimate the real statistical error is inadequate. The method proposed is for analysis of low-amplitude periodicities in the cosmic-ray variations.
    Keywords: SPACE RADIATION
    Type: Morphology of the Quiet and Disturbed Ionosphere; p 79-81
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  • 26
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    Publication Date: 2006-04-26
    Description: It is shown based on data on the cosmic-ray neutron component, ionospheric soundings, and measurements of cosmic radio-emission absorption at Vostok station (Antarctica) that the ionization of the lower ionosphere increases during low intensity of Forbush-type cosmic rays. This is manifested in increased absorption and the appearance of strong sporadic layers in the E-region.
    Keywords: SPACE RADIATION
    Type: Morphology of the Quiet and Disturbed Ionosphere; p 74-77
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  • 27
    Publication Date: 2006-04-26
    Description: Features of the cosmic-ray variations in the geomagnetic pole region and a smooth decrease in the cosmic rays intensity as a result of increased solar activity are reported. A 66-day variation of the cosmic rays was registered, in agreement with the maximum frequency and power of solar chromospheric flares.
    Keywords: SPACE RADIATION
    Type: Morphology of the Quiet and Disturbed Ionosphere; p 113-116
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  • 28
    Publication Date: 2006-06-04
    Description: Heavy cosmic ray nuclei with nuclear charge, Z, equal to or greater than 3 are to be measured using an isotopic stack consisting of passive visual track detectors which remain sensitive throughout the entire mission. The scientific data are stored in latent tracks which are produced by heavy ions and which can be revealed in the investigator's laboratory after recovery. During the mission, only housekeeping data have to be collected. The exposure onboard Spacelab 1 allows the study of the chemical composition and energy spectrum of articles which have energies in the range 20 to 100 million electron volts per atomic mass unit, as well as the isotopic composition of heavy galactic cosmic rays with energies in the range 100 to 1000 million electron volts per atomic mass unit.
    Keywords: SPACE RADIATION
    Type: NASA. Marshall Space Flight Center Spacelab Mission 1 Expt. Descriptions; 3 p
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  • 29
    Publication Date: 2011-08-16
    Description: Nuclear characteristics of plutonium fuel for thermoelectric generators and required shield thicknesses for sensitive radiation experiment in outer planet spacecraft
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 30
    Publication Date: 2011-08-16
    Description: Cosmic ray transport in random magnetic fields, deriving coupled integrodifferential equations for radiant intensity and flux
    Keywords: SPACE RADIATION
    Type: ; 104-111. (
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  • 31
    Publication Date: 2011-08-16
    Description: Spectrum and galactic isotropy of diffuse cosmic X rays by balloon-borne detector
    Keywords: SPACE RADIATION
    Type: ; TROPHYSICAL JOURNAL
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  • 32
    Publication Date: 2011-08-16
    Description: Galactic weak X ray sources observation in Southern Hemisphere for flux and energy spectrum
    Keywords: SPACE RADIATION
    Type: ; 17 (
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  • 33
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    Publication Date: 2011-08-16
    Description: Cosmic ray produced radionuclides in Lost City meteorite, determining concentrations by nondestructive two-parameter gamma ray analysis
    Keywords: SPACE RADIATION
    Type: ; - PHYSICAL METALLURG
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  • 34
    Publication Date: 2011-08-16
    Description: Isotropic cosmic gamma ray flux, discussing extragalactic point sources detection by high resolution spectrometers
    Keywords: SPACE RADIATION
    Type: ; 1 (
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  • 35
    Publication Date: 2011-08-16
    Description: Multiple periodicity of Cygnus X-1 X ray emission from rocket sounding
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 36
    Publication Date: 2011-08-16
    Description: Stellar wind flow models associating energy transport with propagation and dissipation of hydrodynamic waves and heat conduction
    Keywords: SPACE RADIATION
    Type: ; ECTRON (
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  • 37
    Publication Date: 2011-08-16
    Description: Solar cosmic ray acceleration and propagation from time variation and heliocentric distance dependence of relative abundance of protons to helium nuclei
    Keywords: SPACE RADIATION
    Type: ; OMBUSTION IN A FLOW
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  • 38
    Publication Date: 2011-08-16
    Description: Solar flare two stage particle acceleration from X-ray burst observations, discussing induced electric field and Fermi mechanism
    Keywords: SPACE RADIATION
    Type: ; TROPHYSICAL JOURNAL
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  • 39
    Publication Date: 2011-08-16
    Description: Soft galactic X rays role in interstellar grains alignment
    Keywords: SPACE RADIATION
    Type: ; VUE SCIENTIFIQUE ET
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  • 40
    Publication Date: 2011-08-16
    Description: Recurrent solar cosmic ray events and M region magnetic storms
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 41
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    Publication Date: 2011-08-16
    Description: Short duration proton energy increases observation by Explorer 34, considering interpretation as acceleration associated interplanetary shocks
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 42
    Publication Date: 2011-08-16
    Description: Satellite observations of trapped electrons at low and high altitudes for 6 month period in 1965
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 43
    Publication Date: 2011-08-16
    Description: Particle and field oscillations and electron heating due to drift mirror instability in magnetosphere
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 44
    Publication Date: 2011-08-16
    Description: Correlation of increases in electron population of outer radiation belt and interplanetary magnetic fields during two geomagnetic storms
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 45
    Publication Date: 2011-08-16
    Description: Demonstration that, during the process of dielectronic recombination, the energy of a recombined ion after a resonance capture and subsequent stabilization may still be higher than the first ionization limit. If that happens, a secondary autoionization can take place and reduce the recombination coefficient. The importance of this effect is considered for iron ions Fe(9+) to Fe(13+).
    Keywords: SPACE RADIATION
    Type: Astrophysical Letters; 10; Apr. 197
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  • 46
    Publication Date: 2011-08-16
    Description: Evaluation of gamma-ray spectra calculated for relativistic-electron bremsstrahlung interactions at cosmological distances under the assumption of a single power-law source spectrum for the electrons. It is concluded that such spectra cannot match the form of the observed cosmic gamma-ray spectrum above 1 MeV, as has previously been suggested.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 171; Jan. 15
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  • 47
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    Publication Date: 2011-08-16
    Description: Most atoms that are evaporated from interplanetary dust near the sun are quickly ionized and are probably carried away by the interplanetary magnetic field and the solar wind. The contribution of these heavy ions to the solar-wind flux has been estimated by using estimates of the mass required to maintain the zodiacal cloud. This contribution appears to be small compared with the heavy-ion flux of coronal origin. Many ions from dust remain singly ionized; some of these, such as Ca(+), can resonantly scatter solar radiation. The contribution of this interplanetary glow to the background of twilight glow has been estimated. Interplanetary glow may be detectable. Some atoms from dust may be accelerated by radiation pressure before being ionized. Estimates of velocities and fluxes for Fe indicate that this acceleration is not very effective.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 77; Apr. 1
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  • 48
    Publication Date: 2011-08-16
    Description: Measurement of the solar wind electron integral spectrum yielding electron temperatures ranging from 100,000 to 400,000 K and having an average value of 182,000 K, electron densities having an average value of 4.6 per cu cm, and electron-temperature anisotropies ranging from 1 to 1.4. The electron temperature is found to be independent of solar-wind speed over the range from 290 to 675 km/sec. Comparison of the simultaneous alignment of the local magnetic-field vector with the direction of the electron-temperature anisotropy reveals a high correlation. Necessary conditions for the fire-hose instabilities were satisfied in the electron and proton components of the solar-wind plasma immediately behind an interplanetary shock.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 77; Apr. 1
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  • 49
    Publication Date: 2011-08-16
    Description: A high-sensitivity scan of the galactic plane from 70 to 30 deg was performed to search for 2-20-keV X rays from supernova remnants. The spectra of five X-ray sources detected between 44 and 31 deg longitude are presented, of which only two might be associated with suggested supernova remnants. Upper limits are given for the 19 possible supernova remnants scanned.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 173; Apr. 15
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  • 50
    Publication Date: 2011-08-16
    Description: Differential energy spectra of cosmic-ray protons and He nuclei have been measured for the first time by an ionization spectrometer flown at balloon altitudes. The energy range extended from 50 to more than 1000 GeV. The observed differential intensities can be represented with power-law spectra with a slope of -2.75 (plus or minus 0.03) for protons and of -2.77 (plus or minus 0.05) for He nuclei. The proton-to-He ratio is 26 (plus or minus 3) at 40 GeV/nucleon and is constant within errors up to 400 GeV/nucleon.
    Keywords: SPACE RADIATION
    Type: Physical Review Letters; 28; Apr. 10
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  • 51
    Publication Date: 2011-08-16
    Description: The use of magnetometers for azimuth determination of balloon-borne X-ray astronomy payloads is examined, with special emphasis placed on the experiments of the University of Adelaide Cosmic Ray Group. A critical evaluation is made of the effectiveness of the magnetometers, including discussion of effects due to geomagnetic field variations, magnetometer misorientation and spurious contaminant magnetic fields. Calibration techniques and details of in-flight performance are also presented.
    Keywords: SPACE RADIATION
    Type: Planetary and Space Science; 20; Mar. 197
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  • 52
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    Publication Date: 2011-08-16
    Description: Two current models for Eta Carinae are discussed. It is shown that the recently observed soft X-ray flux seems to indicate a surprisingly high density for the ambient gas around Eta Carinae, and that some useful constraints on models of this object may result from X-ray observations.
    Keywords: SPACE RADIATION
    Type: Nature Physical Science; 236; Mar. 20
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  • 53
    Publication Date: 2011-08-16
    Description: The acceleration phase of solar cosmic rays and relativistic electrons is studied on the basis of the observational data available on the optical, radio, X-ray, and particle events associated with the solar flare that occurred on July 7, 1966. The generating process of hydromagnetic shock waves which excited the type-II radio burst detected at a frequency below about 100 MHz is also discussed. The results of the study suggest that no secondary acceleration process after the explosive phase can contribute much to the generation of high energy particles. The ejection of solar cosmic rays and relativistic electrons seems to be related to the expansion of the magnetic bulge which can trap accelerated electrons from the triggering region of solar flares.
    Keywords: SPACE RADIATION
    Type: Solar Physics; 20; Oct. 197
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  • 54
    Publication Date: 2011-08-16
    Description: The observation of a U-type solar radio burst with a reversing frequency of approximately 0.7 MHz suggests the presence of a magnetic bottle extending out to about 35 solar radii. A possible model of this loop structure is developed from the data. The occurrence of low-frequency U-bursts seems to be extremely rare although magnetic bottles may develop frequently during solar maximum.
    Keywords: SPACE RADIATION
    Type: Solar Physics; 20; Oct. 197
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  • 55
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    Publication Date: 2011-08-16
    Description: Solar X-ray line emission, using crystal spectrometers during large chromospheric flare
    Keywords: SPACE RADIATION
    Type: ; HYSICAL PROCESSES IN
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  • 56
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    Publication Date: 2011-08-16
    Description: Proposed model with with neutrons as energy source for solar corona, discussing validity based on capture gamma ray flux expectation
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 57
    Publication Date: 2011-08-16
    Description: Excess intensities of diffuse cosmic X rays related to characteristic line spectrum excitation and element abundances in interstellar region and nebulas
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 58
    Publication Date: 2011-08-16
    Description: Solar wind deflection due to permanent lunar surface magnetism
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    Type: ; YAL SOCIETY (
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  • 59
    Publication Date: 2011-08-16
    Description: Line emission in X ray background in galactic plane and at galactic pole based on rocket flight data
    Keywords: SPACE RADIATION
    Type: ; SEARCH(
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  • 60
    Publication Date: 2011-08-16
    Description: Low energy cosmic ray H 2 and He 3 nuclei intensities /1967-1968/ from Pioneer 8 and IMP 4 measurements
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 61
    Publication Date: 2011-08-16
    Description: Continuous optical conversion to IR and directional stellar radiation flow conversion to diffused radiation fields in circumstellar dust envelopes
    Keywords: SPACE RADIATION
    Type: ; VUE SCIENTIFIQUE ET
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  • 62
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    Publication Date: 2011-08-16
    Description: X ray and far IR measurement inconsistency from Centaurus A, discussing metagalactic submillimeter background
    Keywords: SPACE RADIATION
    Type: ; TROPHYSICAL JOURNAL
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  • 63
    Publication Date: 2011-08-16
    Description: Outer radiation belt electron fluxes during solar proton event on 5 Feb. 1965
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 64
    Publication Date: 2011-08-16
    Description: Comparison of electron response in magnetosphere at L equals 5 with solar wind during magnetic storm on 17-18 Apr. 1965
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 65
    Publication Date: 2011-08-16
    Description: Solar wind rotational to tangential discontinuities ratio determination and hypothesis concerning origin in interplanetary magnetic field
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 66
    Publication Date: 2011-08-16
    Description: Extragalactic cosmic X ray sources at high galactic latitude from sounding rocket experiments, correlating with galactic clusters
    Keywords: SPACE RADIATION
    Type: ; YSICA STATUS SOLIDI
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  • 67
    Publication Date: 2011-08-16
    Description: Cosmic ray intensity gradient measurement from Lost City meteorite Ar 37/Ar 39 ratio
    Keywords: SPACE RADIATION
    Type: ; - PHYSICAL METALLURG
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  • 68
    Publication Date: 2011-08-16
    Description: Magnetospheric electron echo probe experiment, using sounding rocket and injecting gun for controlled particle trapping investigation
    Keywords: SPACE RADIATION
    Type: ; YSICA STATUS SOLIDI
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  • 69
    Publication Date: 2011-08-16
    Description: Interplanetary magnetic field measurements from lunar surface and lunar orbit, discussing solar wind effects on bulk electrical conductivity of lunar crust
    Keywords: SPACE RADIATION
    Type: ; TROPHYSICAL JOURNAL
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  • 70
    Publication Date: 2011-08-16
    Description: Line emission in diffuse cosmic X ray continuum, discussing probable interstellar or intergalactic matter source
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 71
    Publication Date: 2011-08-16
    Description: Iron nuclei emission during 1967-1969 solar flares from spacecraft window and lunar camera lens etched tracks, discussing Fe/He ratio and lunar soil densities
    Keywords: SPACE RADIATION
    Type: ; IENCES (
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  • 72
    Publication Date: 2011-08-16
    Description: Crab Nebula and pulsar NP 0532 X ray spectra discussing pulse profile, emission and interstellar absorption
    Keywords: SPACE RADIATION
    Type: ; BROTECHNIKA, NO. 1(
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  • 73
    Publication Date: 2011-08-16
    Description: Decay lifetimes of Starfish electrons in trapped radiation belt inner zone
    Keywords: SPACE RADIATION
    Type: ; BROTECHNIKA, NO. 1(
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  • 74
    Publication Date: 2011-08-16
    Description: Diffusion coefficient estimation for energetic charged particles across magnetic fields from mathematical model
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 75
    Publication Date: 2011-08-16
    Description: Cyclotron and bounce resonance scattering of electrons trapped in earth magnetic field
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 76
    Publication Date: 2011-08-16
    Description: Fokker-Planck equation used to describe process of electron loss from Van Allen zones due to pitch angle scattering by electromagnetic disturbances
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 77
    Publication Date: 2011-08-16
    Description: Cygnus XR-1 X ray intensity fluctuations, discussing time scales and periodicities
    Keywords: SPACE RADIATION
    Type: ; IENCES (
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  • 78
    Publication Date: 2011-08-16
    Description: Pulsating gamma ray flux from pulsar NP 0532 in energy range from 250 keV to 2.3 MeV
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 79
    Publication Date: 2011-08-16
    Description: Line emission in diffuse X ray background at high galactic latitudes, interpreting rocket observations
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 80
    Publication Date: 2011-08-16
    Description: Submillimeter background radiation origin possibility from extragalactic discrete sources based on cosmological models
    Keywords: SPACE RADIATION
    Type: ; 1 (
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  • 81
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    Publication Date: 2011-08-16
    Description: Nuclear soft core potential reproduction by isoscalar vector meson in nonlocal field theory of fireball in high energy cosmic ray collisions
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 82
    Publication Date: 2011-08-16
    Description: Energetic electrons generating solar flares position relation with active regions associated with type I radio noise storms
    Keywords: SPACE RADIATION
    Type: ; YSICA STATUS SOLIDI
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  • 83
    Publication Date: 2011-08-16
    Description: Low energy cosmic ray intensity increase at propagating interplanetary shock wave front, discussing one dimensional model with particles undergoing convection and diffusion
    Keywords: SPACE RADIATION
    Type: ; BROTECHNIKA, NO. 1(
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  • 84
    Publication Date: 2011-08-16
    Description: Relativistic electrons acceleration in solar proton flares, taking into account plasma density and magnetic field intensity
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 85
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    Publication Date: 2011-08-16
    Description: Cosmic ray intensity Forbush decrease on 23 September 1966 coincidence with magnetic storm sudden commencement from satellite and ground based monitors data
    Keywords: SPACE RADIATION
    Type: ; 63 (
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  • 86
    Publication Date: 2011-08-16
    Description: Satellite observations of distribution of energetic protons in earth radiation belts between 1962 - 1964
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 87
    Publication Date: 2011-08-16
    Description: Transient behavior of electrons in artificial radiation belts from satellite observations
    Keywords: SPACE RADIATION
    Type: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 88
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    Publication Date: 2011-08-16
    Description: Development of a theory of hydromagnetic waves and discontinuities which is appropriate for the solar wind. The experimental evidence for the various waves, discontinuities, and some of the instabilities which are predicted by this theory is reviewed. Nearly all of the discontinuities given by the theory are shown to exist in the solar wind. These include tangential discontinuities, forward and reverse fast and slow shocks, perpendicular shocks, and Alfven shocks. Parallel shocks and contact discontinuities have not been found. A number of special cases are considered which show the basic physical properties of hydromagnetic waves in an anisotropic, multifluid, collisionless plasma. A treatment of discontinuities is presented which most resembles those of Chao (1970) and Hudson (1970). On the basis of the experimental results reviewed it is concluded that hydromagnetic theory is applicable to the solar wind.
    Keywords: SPACE RADIATION
    Type: Space Science Reviews; 12; Dec. 197
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  • 89
    Publication Date: 2011-08-16
    Description: Perturbations of the solar wind downstream of the moon and lying outside of the rarefaction wave that defines the diamagnetic cavity are used to define possible source regions comprised of intrinsically magnetized areas of the moon. A map of the moon is constructed showing that a model in which the sources are exposed to the grazing solar wind during the lunation yields a selenographically invariant set of regions strongly favoring the lunar highlands over the maria. An alternative model with the source due to electromagnetic induction is explored. The ages of the field sources should be consistent with those based on the basalt ages and possibly far older if the sources are connected with the formation of the highland rocks themselves. The perturbations are tentatively identified as weak shock waves, and a Mach angle in accord with nominal values for the solar wind is found.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 77; Feb. 1
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  • 90
    Publication Date: 2011-08-16
    Description: Type IV radio bursts with wide band from microwave to metric-wave frequency are generally associated with solar proton flares. Recently, Castelli et al. (1967, 1968) have shown that the type IV radio bursts associated with solar proton flares show the U-shaped peak flux spectra with the minimum flux at decimetric frequencies. In this paper, the center-to-limb variation of such peak flux spectra is investigated in order to examine the effect of decrease of the peak flux at metric frequencies with increase of the angular distance from the central meridian of the sun. It is shown that the U-shaped spectra are obtained independent of the position of proton flares, although the spectral form changes significantly in the case of the flares near the limb. It is further suggested that the U-shaped spectra consist of the two essentially independent components for microwave and metric-wave frequencies, respectively.
    Keywords: SPACE RADIATION
    Type: Planetary and Space Science; 19; Dec. 197
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  • 91
    Publication Date: 2011-08-16
    Description: Data from two flights of a new superconducting magnetic spectrometer are reported. This instrument was capable of a direct matter-antimatter separation in the cosmic rays. Antimatter events would appear in the spectrometer as trajectories which curve in the opposite direction to common matter, because of their negative charge. A brief description of the equipment and of the characteristics of the instrument is presented, along with the data processing techniques used. A new upper limit on the amount of antimatter in primary cosmic rays has been established. The limits are considerably lower than those for any previous experiment.
    Keywords: SPACE RADIATION
    Type: Nature; 236; Apr. 14
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  • 92
    Publication Date: 2011-08-16
    Description: Detailed study of the observed ionospheric effects of the X-ray flare on July 8, 1968, which was of considerable importance both from the ionospheric and solar physics point of view. The associated optical flare was of importance 3B. The ionospheric effects were examined in order to derive a suitable physical model of flare-induced ionization below 100 km, and hence to estimate the spectral characteristics of the ionizing radiations from the observed SID s. The electron loss coefficients below 70 km height calculated from the formula developed in the analysis are in agreement with available data.
    Keywords: SPACE RADIATION
    Type: Journal of Atmospheric and Terrestrial Physics; 33; Dec. 197
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  • 93
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    Publication Date: 2011-08-16
    Description: Suggestion that, under certain circumstances, the absence of an apparent flattening of the ultrahigh energy cosmic ray spectrum at an energy level above 3 x 10 to the 18th power eV may have implications concerning the origin of ultrahigh energy cosmic rays (UECR). On the basis of the discussion presented, it seems that a heavy composition is indicated. It is therefore concluded that recent air-shower studies seem to indicate the resurrection of the galactic origin model.
    Keywords: SPACE RADIATION
    Type: Nature Physical Science; 234; Nov. 8
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  • 94
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    Publication Date: 2011-08-16
    Description: The mechanism proposed involves the occurrence of a flare in a region of high magnetic field on the surface of a star. The flare produces oscillations in the magnetic field structure. The oscillations lead to heating of the plasma in a flux tube which emits thermal radiation. The heating may be caused by magnetic pumping or particles accelerated in periodic bursts by the flare. Synchrotron radiation from high energy particles accounts for the hard X-ray emission.
    Keywords: SPACE RADIATION
    Type: Nature; 235; Jan. 14
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  • 95
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    Publication Date: 2011-08-16
    Description: The model involves an assessment of the effect of beaming as indicated by the pulsations themselves rather than by assuming gamma-ray absorption by interaction with an isotropic photon field. The chief absorption process to be taken into account is that of pair production in the intense photon field. Most important is the pair production in the intense photon field which occurs during the pulse.
    Keywords: SPACE RADIATION
    Type: Nature Physical Science; 235; Jan. 3
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  • 96
    Publication Date: 2011-08-16
    Description: Results of observations of the solar eclipse of Mar. 7, 1970, with photometers sensitive to narrow bands of radiation at Lyman-alpha (1216 A) and at 2600 A included in the payloads of four Nike Apache rockets flown before and during the eclipse. At the center of totality, the flux of Lyman-alpha from the solar corona is 0.15% of the flux from the unobscured sun. The flux at second contact is 0.64%; at third contact, two observations give 0.52 and 0.59%. The brightness of the chromosphere in Lyman-alpha decreases exponentially over the range from 5 to 30 arc-sec from the limb with a scale height of 3835 plus or minus 70 km. In addition to the coronal and chromospheric Lyman-alpha a diffuse source is found. This is restricted to within 20 deg of the earth's horizon and is nearly uniform in azimuth at 170 km, the flux is about 3% of that from the unobscured sun. The flux of Lyman-alpha during the eclipse is considered in relation to the observed variation in electron density. It is concluded that, in totality, the ionosphere near 80 km is not in equilibrium with the ionizing radiation and that the production rate for electrons is not negligible if the loss process is recombination; it is negligible if the loss process is attachment-like.
    Keywords: SPACE RADIATION
    Type: Journal of Atmospheric and Terrestrial Physics; 34; Apr. 197
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  • 97
    Publication Date: 2011-08-16
    Description: Measurement of the absorption profiles and residual fluxes of three bands of solar X-rays before and during the eclipse of Mar. 7, 1970. In the bands 2 to 8 A, 8 to 20 A, and 44 to 60 A the residual flux in totality is found to be respectively 5, 7, and 16% of the flux from the uneclipsed sun. It is shown that the radiation maintaining the E-layer varies in proportion to the 44- to 60-A flux. In the D-layer, ionization by the residual flux of 2 to 8 A is less important in totality than is ionization of nitric oxide by Lyman-alpha.
    Keywords: SPACE RADIATION
    Type: Journal of Atmospheric and Terrestrial Physics; 34; Apr. 197
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  • 98
    Publication Date: 2011-08-16
    Description: Measurement of the charge composition for several of the multicharged nuclei and the energy spectra for hydrogen, helium, and medium (6 less than or equal to Z less than or equal to 9) nuclei in the Apr. 12, 1969, solar-particle event. The energy/nucleon spectral shape of the medium nuclei was again the same as that of the helium nuclei, and the ratio of these two species was consistent with the present best average of 58 plus or minus 5. By combining the results obtained here with previous work, improved estimates of the Ne/O and Mg/O values of 0.16 plus or minus 0.03 and 0.056 plus or minus 0.014, respectively, were obtained. Silicon and sulfur abundances relative to O were determined to be 0.208 plus or minus 0.008 plus or minus 0.006, respectively, and 85% confidence upper limits for Ar and Ca relative to O of 0.017 and 0.010 were obtained. Previously, these last four nuclei had only been listed as a group.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; 171; Jan. 1
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  • 99
    Publication Date: 2011-08-16
    Description: Evaluation of two daytime D-region positive-ion composition measurements performed at Thumba, India, for solar zenith angles of 53.2 and 27.8 deg. Comparison of upleg ram with downleg wake data shows a large increase in the concentration of heavy ions 48(+), NO(+) . H2O; 55(+), H3O(+) . (H2O)2; and M(+) greater than 65(+) for the downleg reduced shock condition. Peak concentrations of 48(+) and 55(+) occur at unit optical depth for Lyman alpha radiation. The ion 37(+), H3O(+) . H2O, is dominant for chi = 27.8 deg, but not for chi = 53.2 deg, consistent above 80 km with an origin from the X-ray production of O2(+). Laboratory measurements have shown that the ion, NO(+), can be transferred to heavy hydrates 48(+), 55(+), and M(+) greater than 65(+) by a reaction chain starting with NO(+) + X + M = NO(+) . X + M, where X can be O2, N2, CO2 or a combination of all three, depending on the rate of reaction. This chain, together with a similar reaction scheme starting with O2(+) and ending in 19(+), 37(+), and heavier clusters, is used to provide a consistent explanation for the hydrated ions observed in the D region.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 76; Dec. 1
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  • 100
    Publication Date: 2011-08-16
    Description: Previous work by Balasubrahmanyan and Venkatesan (1970) on the general problem of the solar activity relationship with the 27-day recurrence and long term modulation of cosmic ray intensity, and Lockwood's (1971) comments thereon are discussed in the light of some further work. A possible explanation proposed for the absence of any time lag in both short and long term cosmic ray intensity changes views the long term variation as a result of a superposition of a number of short term decreases.
    Keywords: SPACE RADIATION
    Type: Solar Physics; 20; Oct. 197
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