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  • SPACE RADIATION  (500)
  • 1990-1994
  • 1980-1984  (129)
  • 1970-1974  (371)
  • 1930-1934
  • 1981  (129)
  • 1971  (371)
Collection
Years
  • 1990-1994
  • 1980-1984  (129)
  • 1970-1974  (371)
  • 1930-1934
Year
  • 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: 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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  • 3
    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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  • 4
    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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  • 5
    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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  • 6
    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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  • 7
    Publication Date: 2006-08-20
    Keywords: SPACE RADIATION
    Type: Res. in the Space Sci., v. 2; 10 p
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  • 8
    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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  • 9
    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
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  • 10
    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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  • 11
    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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  • 12
    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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  • 13
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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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  • 14
    Publication Date: 2011-08-16
    Description: Isotropic cosmic gamma ray flux, discussing extragalactic point sources detection by high resolution spectrometers
    Keywords: SPACE RADIATION
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  • 15
    Publication Date: 2011-08-16
    Description: Multiple periodicity of Cygnus X-1 X ray emission from rocket sounding
    Keywords: SPACE RADIATION
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  • 16
    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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  • 17
    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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  • 18
    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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  • 19
    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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  • 20
    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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  • 21
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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
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  • 22
    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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  • 23
    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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  • 24
    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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  • 25
    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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  • 26
    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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  • 27
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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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  • 28
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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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  • 29
    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
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  • 30
    Publication Date: 2011-08-16
    Description: Solar wind deflection due to permanent lunar surface magnetism
    Keywords: SPACE RADIATION
    Type: ; YAL SOCIETY (
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  • 31
    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
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  • 32
    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
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  • 33
    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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  • 34
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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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  • 35
    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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  • 36
    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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  • 37
    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
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  • 38
    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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  • 39
    Publication Date: 2011-08-16
    Description: Cosmic ray intensity gradient measurement from Lost City meteorite Ar 37/Ar 39 ratio
    Keywords: SPACE RADIATION
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  • 40
    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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  • 41
    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
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  • 42
    Publication Date: 2011-08-16
    Description: Line emission in diffuse cosmic X ray continuum, discussing probable interstellar or intergalactic matter source
    Keywords: SPACE RADIATION
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  • 43
    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
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  • 44
    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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  • 45
    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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  • 46
    Publication Date: 2011-08-16
    Description: Diffusion coefficient estimation for energetic charged particles across magnetic fields from mathematical model
    Keywords: SPACE RADIATION
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  • 47
    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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  • 48
    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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  • 49
    Publication Date: 2011-08-16
    Description: Cygnus XR-1 X ray intensity fluctuations, discussing time scales and periodicities
    Keywords: SPACE RADIATION
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  • 50
    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
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  • 51
    Publication Date: 2011-08-16
    Description: Line emission in diffuse X ray background at high galactic latitudes, interpreting rocket observations
    Keywords: SPACE RADIATION
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  • 52
    Publication Date: 2011-08-16
    Description: Submillimeter background radiation origin possibility from extragalactic discrete sources based on cosmological models
    Keywords: SPACE RADIATION
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  • 53
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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
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  • 54
    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
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  • 55
    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
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  • 56
    Publication Date: 2011-08-16
    Description: Relativistic electrons acceleration in solar proton flares, taking into account plasma density and magnetic field intensity
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  • 57
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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
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  • 58
    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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  • 59
    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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  • 60
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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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  • 61
    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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  • 62
    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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  • 63
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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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  • 64
    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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  • 65
    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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  • 66
    Publication Date: 2011-08-16
    Description: The origin of high-energy cosmic electrons is considered. It is found that electrons of energies below 1000 GeV could have been produced by local supernovae associated with known radio remnants. At higher energies, observations of muon-poor air showers indicate the existence of electrons at 1,000,000 GeV which may have originated entirely from the supernova Vela X.
    Keywords: SPACE RADIATION
    Type: Physical Review Letters; 27; Nov. 8
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  • 67
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    Publication Date: 2011-08-16
    Description: Galatic radio spur association with soft X ray emission
    Keywords: SPACE RADIATION
    Type: ; VIGATION (
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  • 68
    Publication Date: 2011-08-16
    Description: Distributions and average values for the proton speed, azimuthal and polar flow directions, and the proton temperature and density in the solar wind are presented. The data are obtained from the Ames plasma probes on Pioneers 6 and 7. The time periods covered include Dec. 18, 1965 to mid-February 1966, and mid-August to mid-October 1966. The distributions of the parameters, except for the polar flow direction, are skewed, partially because of stream-stream interactions in the solar wind. The average values of the basic plasma parameters from the two spacecraft are different which could be due partially to different solar activity at the two times, and partially to sector and beam structure dependence.
    Keywords: SPACE RADIATION
    Type: Cosmic Electrodynamics; 2; Oct. 197
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  • 69
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    Publication Date: 2011-08-16
    Description: Measurements of flare-related impulsive enhancements in solar emission lines in the extreme ultraviolet, observed from the satellite OSO-III, are reported. The enhancement of a line, expressed in percent of the total disk intensity in the line, is of the same order of magnitude as the flare area, expressed in heliocentric square degrees. Rise-times and decay-times of impulsive enhancements average about 2 min and 5 min, respectively. The maximum enhancements of radiation from ions in the chromosphere-corona transition region precede the H-alpha maximum by an average of 2 min, and occur in the same period of time as the hard component of solar X rays and the impulsive microwave bursts. Coronal lines in the extreme ultraviolet are less impulsive than the transition region lines in flare-related enhancements and their maxima follow the H-alpha maximum.
    Keywords: SPACE RADIATION
    Type: Solar Physics; 21; Dec. 197
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  • 70
    Publication Date: 2011-08-18
    Description: The pitch angle scattering of cosmic ray is modified greatly if the medium through which they propagate contains significant amounts of magnetic helicity. When helicity is present in the medium, the often used expression for the pitch angle diffusion coefficient derived from quasilinear theory must be modified. These modifications are illustrated for slab and isotropic symmetries. Using measurements of helicity in the solar wind determined from single point measurements of the correlation tensor of magnetic fluctuations obtained from Voyager 2, the effects of the observed helicity on both the pitch angle and spatial diffusion coefficients are estimated.
    Keywords: SPACE RADIATION
    Type: Contrib. to the 17th Intern. Cosmic Ray Conf.; p 5-8
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  • 71
    Publication Date: 2011-08-18
    Description: The mean value of the correlation between local magnetic field and vector potential, known as the magnetic helicity, is a measure of the lack of mirror reflection symmetry of magnetic covariances in a turbulent medium. A method is presented for extraction of helicity spectra from magnetometer data, and applied to an evaluation of the magnetic helicity of interplanetary magnetic fluctuations.
    Keywords: SPACE RADIATION
    Type: Contrib. to the 17th Intern. Cosmic Ray Conf.; p 2-4
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  • 72
    Publication Date: 2011-08-18
    Description: One of the results of the EINSTEIN/C.f.A. X-ray stellar survey was a determination of the contribution of the disk stellar population to the galactic component of the diffuse soft (0.28 - 1.0 keV) X-ray background. This analysis employed both binned and unbinned nonparametric statistical methods that have been developed by Avni, et al. (1980). These methods permitted the use of the information contained in both the 22 detections and 4 upper bounds on the luminosities of 26 dM stars in order to derive their luminosity function. Luminosity functions for earlier stellar types are not yet developed. For these earlier stellar types, the median luminosities as determined by Vaiana, et al., are used (1981), which underestimates their contribution to the background. We find that it is the M dwarfs that dominate the disk population stellar contribution to this background. To calculate the contribution of the stellar sources to the background, simple models both for the spatial distribution of the stars and for the properties of the intervening interstellar medium are used. A model is chosen in which all stellar classes have the same functional form for their spatial distribution: an exponentially decreasing distribution above the galactic equatorial plane, and a uniform distribution within the galactic plane for a region of several kiloparsecs centered on the Sun.
    Keywords: SPACE RADIATION
    Type: Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1; p 201-205
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  • 73
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    Publication Date: 2011-08-18
    Description: It is assumed that cool star chromospheres are heated by mechanical energy dissipation that depends quasilinearly on density and cooled by radiation loss and it is shown that the basic properties of chromospheres are determined by the ionization of hydrogen. It is hydrogen ionization that provides the freedom for chromospheres to adjust their radiation losses to balance the prescribed heat input, resulting in an extended region of low temperature gradient. Chromospheric radiation losses in cool stars occur mainly in the strongest spectral lines at wavelengths greater than about 2000 A and the fraction of the chromosphere is effectively thin. The most important lines include Ca II H and K and the infrared triplet and Mg II h and k. The strong lines of other abundant species, are less important because their high excitation energies reduce the collisional excitation rates. Lyman alpha losses are important because of the overwhelming abundance of hydrogen. However, the inability of chromospheres to adjust their Lyman alpha losses limits the geometrical thickness of the effectively thin region in Lyman alpha and limits the total Lyman alpha flux.
    Keywords: SPACE RADIATION
    Type: Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1; p 3-14
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  • 74
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    Publication Date: 2011-08-18
    Description: Consideration is given to Carr's theory (1980) that most cosmic X-ray background is produced by thermal X-ray emission associated with black hole accretion disks for compact objects. It is posited that the onset of significant X-rays occurs during galaxy formation when accretion disks are formed by the interaction of young galaxies and massive black holes of pregalactic origin. The study suggests that most cosmic X-ray background could be produced from distant sources with a low ratio of optical to X-ray luminosity. Precursor active galaxy objects involving a massive black hole surrounded by a hot optically thin accretion disk radiating near the Eddington luminosity limit and with an effective temperature of about 2 x 10 to the 9th K would fulfill the condition and produce the correct background spectrum and intensity. This model also associates cosmic X-ray background and nonthermal gamma-ray background to active galaxies, thus implying that massive black holes are associated with their internal dynamics.
    Keywords: SPACE RADIATION
    Type: Nature; 290; Apr. 9
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  • 75
    Publication Date: 2011-08-18
    Description: A narrowband highly spin-modulated radio source has been observed with the radio astronomy experiment on ISEE 3 from a position 0.01 AU upstream of the earth. The source is interpreted as radio line emission generated at twice the local plasma frequency in the vicinity of the earth's bow shock by energetic particles. The bandwidth of the 2f(p) emission varies from less than 3 kHz to more than 20 kHz and is probably broadened by solar wind density variations across the source region. The 2f(p) source is visible about 50% of the time, and the true position of its centroid is usually located within 30 earth radii of the subsolar point, but at times is observed at a distance of up to 60 earth radii. But most of these variations might result from changes in the orientation of the polarization vector in a partially polarized source or from refraction across an electron density front.
    Keywords: SPACE RADIATION
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  • 76
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    In:  Other Sources
    Publication Date: 2011-08-18
    Description: Previous calculations of electrostatic and electromagnetic growth rates for plasma instabilities have neglected the thermal spread of the distribution function of the planetary ions. We consider the effects of finite temperatures for exospheric ions borne in the solar wind. Specifically, growth rates are calculated for electromagnetic instabilities in the low-frequency case for Alfven waves and the intermediate frequency case for whistlers. Also, electrostatic growth rates are calculated for the intermediate frequency regime. From these growth rates, estimates are derived for the pickup times of the planetary ions. The electromagnetic instabilities are shown to produce the most rapid pickup. In the situation where the angle between the local Venus magnetic field and the plasma flow direction is small, the pickup times for both electromagnetic and electrostatic instabilities become very long. A possible consequence of this effect is to produce regions of enhanced planetary ion density in favorable Venus magnetic field-solar wind flow geometries.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 86; June 1
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  • 77
    Publication Date: 2011-08-18
    Description: By simulating the trajectories for scatter free and diffusive propagation of relativistic cosmic rays in a model of the heliospheric magnetic fields containing a representation of corotating interaction regions (CIR's), it is found that, due to the large gradients associated with these compression regions, the motion is strongly affected and differs substantially from the predictions of current modulation theory. For positive (outward) northern hemisphere polarity, particles do not stream purely from high latitudes but can come from almost any latitude in the outer heliosphere; for negative polarity, many particles come along the current sheet (as predicted) but a second, equally important, population exists comprising particles that do not start on the current sheet but are brought to low latitudes by their interaction with CIR's. Thus, it is concluded that CIR's (and other large scale structures) cannot be ignored in analyses of cosmic ray modulation.
    Keywords: SPACE RADIATION
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  • 78
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    Publication Date: 2011-08-18
    Description: Ground-based and satellite-based ionizing radiation monitoring systems are considered as alternative methods for ensuring safe radiation levels for high-altitude aircraft. It is found that ground-based methods are of limited accuracy due to insensitivity to solar particles of energies between the riometer upper cutoff of about 50 MeV and the neutron monitor threshold of about 450 MeV. This energy range is demonstrated to be essential for atmospheric radiation monitoring at high altitude, and must be covered by satellite measurement. On the basis of presently available data, the accuracy to which the incident solar particle flux must be measured by satellite-borne detectors is examined and recommendations are made to establish minimum requirements.
    Keywords: SPACE RADIATION
    Type: Health Physics; 41; Oct. 198
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  • 79
    Publication Date: 2011-08-18
    Description: The intensity changes of galactic cosmic rays associated with the enhanced solar activity during the onset of cycle 21 were observed by Pioneer 10 and Helios 1 and 2, over an extended range of energy and heliocentric distance that provides new insight into the relative importance of the various processes involved in the long-term modulation. A close correspondence is found between changes at 1 AU and those at 23 AU, for hydrogen and helium in the range of 100-200 MeV per nucleon. The time delay observed corresponds to an outward propagation velocity of some 550 km/sec, suggesting that the recently discovered, moderately long-lived, radially propagating shock waves in the outer heliosphere may play a key role in the long-term modulation.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 249
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  • 80
    Publication Date: 2011-08-18
    Description: The onset of the March 5 Gamma-Ray burst was observed with microsecond time resolution by the Monitor Proportional Counter aboard the HEAO-2/Einstein Observatory. The data were analyzed for high frequency periodic pulsations which, if present, would be strong evidence for vibrations of a neutron star following the initial release of energy. Evidence is not found for such pulsations in the data over the period range 29.4737 to 0.0962 ms, and upper limits to the amplitude of 49-70% are set.
    Keywords: SPACE RADIATION
    Type: Astrophysical Letters; 22; 2, 19; 1981
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  • 81
    Publication Date: 2011-08-18
    Description: A class of low-speed solar wind flows with velocities of 450 km/s and less, ion temperatures of 40,000 K and less, and heavy ion distributions indicating moderate coronal freezing in temperatures in the range from 1 million to 2.5 millions K is considered. For brevity this class is termed interstream. Interstream flows have as yet, not firm identification with a coronal origin. The considered investigation is concerned with the identification of the coronal origins of interstream flows. It is found that major sources of low speed solar wind are the quiescent, near-equatorial coronal streamers. Such an identification provides a natural explanation for the long term variations of solar wind electron temperature and density observed at 1 AU by Feldman et al. (1979) in terms of the concurrent long term morphological variation in the coronal equatorial streamer belt observed using the Mauna Loa K-coronameters.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 86; July 1
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  • 82
    Publication Date: 2011-08-18
    Description: The chemical composition of cosmic ray nuclei, the value of Z varying between 3 and 28, and being between a few hundred MeV/nucleon and a few hundred GeV/nucleon, is compared with a consistent set of propagation calculations. These include the effects of spallation (energy-dependent cross sections are used), escape, ionization loss in the interstellar medium, and deceleration in the solar cavity. The amount of matter traversed by cosmic rays is found to be approximately 7 g/sq cm, independent of energy between 100 MeV/nucleon and 2 GeV/nucleon. Above 2 GeV/nucleon, the escape length varies as the -0.4 + or 0.1 power of the energy. In addition, a procedure has been developed to measure the shape of the cosmic ray path length distribution. Utilizing the ratio of Fe secondaries to Fe in the cosmic rays, presently available data are found to be consistent with an exponential distribution and they eliminate models in which the path length distribution is severely truncated. To tie down the shape of the distribution more precisely, new measurements of the cosmic ray composition, presently becoming available from experiments on the HEAO 3 satellite, will have to be coupled with improved measurements of the energy dependence of partial and total cross sections.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 247
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  • 83
    Publication Date: 2011-08-18
    Description: At heliocentric distances between 14 and 22 AU, some 14 increases in the flux of 1 MeV protons have been identified over a 3 yr period by the NASA Goddard/University of New Hampshire cosmic-ray experiment on Pioneer 10. These increases appear to be associated with large solar flares. Combining the particle data with the Pioneer 10 plasma observations from the NASA/Ames plasma analyzer reveals that the particle increases are produced by radially propagating shock waves generated by the solar events. While the characteristics of these particle events in the distant heliosphere appear to differ greatly from those observed at 1 AU, they represent the evolution expected as the interplanetary magnetic field becomes almost azimuthal. These long-lived shocks provide a valuable in situ laboratory for directly studying particle acceleration under a variety of conditions. They may also represent a significant factor in producing the long-term modulation of galactic cosmic rays.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 246
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  • 84
    Publication Date: 2011-08-16
    Description: The required electron density to excite a type III solar burst can be predicted from different theories, using the low frequency radio observations of the RAE-1 satellite. Electron flux measurements by satellite in the vicinity of 1 AU then give an independent means of comparing these predicted exciter electron densities to the measured density. On this basis, one theory predicts the electron density in closest agreement with the measured values.
    Keywords: SPACE RADIATION
    Type: Solar Physics; 21; Dec. 197
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  • 85
    Publication Date: 2011-08-16
    Description: The steady motion in sunspot magnetic regions is considered for both current-free and force-free configurations. The sufficient condition for stability is obtained in the presence of both external current-free and force-free magnetic fields and a steady motion. It is shown that the pattern of such steady motion is most important in triggering an instability of sunspot magnetic fields, both for the current-free and force-free configuration. When there is no steady motion, the current-free configuration of sunspot magnetic fields is always stable, whereas the stability in the case of force-free magnetic fields is connected with the configuration. The onset of a solar flare seems to be associated with an instability connected to the steady motion within the sunspot magnetic regions.
    Keywords: SPACE RADIATION
    Type: Planetary and Space Science; 19; Oct. 197
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  • 86
    Publication Date: 2011-08-16
    Description: Suprathermal proton bremsstrahlung cross section calculation, using Weizsacker-Williams method
    Keywords: SPACE RADIATION
    Type: ; - PHYSICAL AND RADIO
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  • 87
    Publication Date: 2011-08-16
    Description: Diffuse cosmic X rays small scale structure, comparing Wolfe-Burbridge theoretical autocorrelation functions for galaxies clusters and superclusters with experimental value
    Keywords: SPACE RADIATION
    Type: ; ADEMIE DES SCIENCES
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  • 88
    Publication Date: 2011-08-18
    Description: The diffuse high-energy galactic gamma radiation to be expected from cosmic ray interactions with matter and photons is considered with particular emphasis on the contribution of Compton radiation from cosmic ray electrons. The intensity, spectrum and spatial distribution of the expected galactic gamma radiation are estimated based on models of the matter, cosmic ray and photon distributions to take into account the contributions of bremsstrahlung, high-energy cosmic-ray nucleon and interstellar matter interactions as well as Compton interactions between cosmic ray electrons and background photons. Results suggest that the Compton gamma ray contribution from cosmic ray electron interactions with galactic visible and infrared photons is substantially larger than previously believed. Analysis of the energy spectra and latitude dependence of the various sources reveals that the Compton radiation, bremsstrahlung and nuclear cosmic ray-matter interaction radiation should be separable, with Compton radiation dominating at energies from 10 to 100 MeV at galactic latitudes greater than several degrees. Results demonstrate the potential of gamma ray observations in studies of galactic structure, cosmic ray electrons and galactic photon density.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 250
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  • 89
    Publication Date: 2016-06-07
    Description: The composition of energetic solar particles is reviewed for all solar events in which measurements on helium and heavier nuclei have been made simultaneously in the same detector during a given particle event. For nuclei of equal charge-to-mass ratio, the relative abundances have been the same within uncertainties in every measurement, and consistent with spectroscopic photospheric estimates. Iron has a slightly different charge-to-mass ratio but is still of considerable interest. An observation of the Fe/O in the January 24, 1971 solar event has provided a second determination of this value.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 53-58
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  • 90
    Publication Date: 2016-06-07
    Description: A magnetic core digitized spark chamber gamma ray telescope has been developed for satellite use. The detector has the following characteristics: effective area = 500 cu/cm, solid angle = 1/4 SR; efficiency (high energy) = 0.29; and time resolution of better than two milliseconds.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 42-46
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  • 91
    Publication Date: 2016-06-07
    Description: The survival of high Z nuclei in the X-ray photon field of a pulsar is investigated. For heavy nuclei with energies greater than or equal to 100 GeV/nucleon, 100 keV X-ray photons have sufficient energy to cause photodisintegration with cross sections of approximately 10 to the minus 25th power sq cm. Using the observed properties of the Crab pulsar, extrapolation back to epochs when the pulsar was more active indicates that the photon field is sufficiently dense to prevent the acceleration of heavy nuclei within the velocity of light cylinder. On this model, the upper limit on the energy of the escaping nuclei varies with time. The models for cosmic ray acceleration in supernova explosions or by pulsars will be related to experimental observations.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 33-41
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  • 92
    Publication Date: 2016-06-07
    Description: Experimental results from the balloon borne ionization spectrometer have enabled the extension of the measurement of the energy spectra of cosmic rays to 10 to the 12th power eV. The exposure factor for this flight was 1825 sq m/sr/sec and approximately 10,000 nuclei with Z greater than or equal to 3 have been observed. Differential spectra of individual nuclei from lithium to oxygen and from groups of nuclei with Z = 10-14, 15-19, 20-23, and 24-30 energy range 2 x 10 to the 10th eV to 10 to the 12th eV are described in a power law representation. Results indicate that the composition of galactic cosmic rays remains similar to that observed at lower energies. These results from direct measurements provide evidence for the processes of source acceleration with interstellar propagation remaining essentially energy independent up to 10 to the 12th power eV.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 9-18
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  • 93
    Publication Date: 2016-06-07
    Description: The primary cosmic ray proton and He spectra from 50 GeV to 2000 GeV have been measured by an ionization spectrometer flown on a balloon. At low energies, the energies of individual events are determined to within + or - 30%. At higher energies, the cascade is not fully contained within the four mean free path thick spectrometer and the problems of estimating the energies of these events are discussed. The proton spectrum continued with constant exponent = -2.7 + or - 0.1 up to energies greater than 1000 GeV. This spectrum was in agreement with the results at the low energies. There was no evidence for a spectral break at about 1000 GeV observed.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 1-8
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  • 94
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    Publication Date: 2018-12-01
    Description: Book on cosmic gamma rays covering secondary particle decay, electron-positron annihilation, proton-antiproton interactions, galactic radiation and cosmology
    Keywords: SPACE RADIATION
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  • 95
    Publication Date: 2018-12-01
    Description: Galactic and solar cosmic ray propagation, variations, and energy spectra
    Keywords: SPACE RADIATION
    Type: PROC. OF THE SIXTH WINTER SCHOOL ON SPACE PHYS., PART 2 1971; P 33-93
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  • 96
    Publication Date: 2016-06-07
    Description: Interactions with all 14 of the states in the Western Region over the past three years are reviewed from NASA's perspective. Outreach and training programs using the M mobile analysis and training extension van, the University Program, classes at the Ames Center, demonstration tests with state agencies, and surveying the needs of local governments are highlighted. Planned activities, the continuance of ASVT's, and the impact of the budget cuts on NASA'S technology program are also considered.
    Keywords: SPACE RADIATION
    Type: Western Reg. Remote Sensing Conf. Proc., 1981; p 2-7
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  • 97
    Publication Date: 2016-06-07
    Description: There are certain conceptual difficulties in the theory of the generation of ultraviolet radiation which is presumed for the creation of the optical fluorescence mechanism of supernova light emission and ionization of a nebula as large as the Gum nebula. Requirements concerning the energy distribution of the ultraviolet photons are: 1) The energy of the greater part of the photons must be sufficient to cause both helium fluorescence and hydrogen ionization. 2) If the photons are emitted in an approximate black body spectrum, the fraction of energy emitted in the optical must be no more than what is already observed. Ultraviolet black body emission depends primarily on the energy source. The probability that the wide mixture of elements present in the interstellar medium and supernova ejecta results in an emission localized in a limited region with less than 0.001 emission in the visible, for either ionization or fluorescence ultraviolet, is remote. Therefore transparent emission must be excluded as unlikely, and black body or at least quasi-black-body emission is more probable.
    Keywords: SPACE RADIATION
    Type: NASA. Goddard Space Flight Center The Gum Nebula and Related Probl.; p 163-165
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  • 98
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    In:  CASI
    Publication Date: 2016-06-07
    Description: The effects of low energy heavy nuclei from the supernova explosion on nearby interstellar space were investigated. In addition to the ionization and heating of the Gum nebula, these particles may produce detectable fluxes of X-rays and gamma rays, both as continuum radiation and line emission.
    Keywords: SPACE RADIATION
    Type: The Gum Nebula and Related Probl.; p 97-109
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  • 99
    Publication Date: 2016-06-07
    Description: Time variations of the 3-12 MeV interplanetary electron intensity, observed by the Explorer-18, -28, and -33 spacecrafts, have been studied in detail. Apart from solar flare effects, there are five distinct periods when the electron intensity has undergone a series of increases, and these are strongly correlated with solar rotation. The intensity increases are separate phenomena, and are strikingly anticorrelated with increases in the low energy solar proton intensity. The electron energy spectrum during those quiet-time increases is typically represented by dJ/dE = k E/2.0 + or - 0.25 similar to the galactic electron spectrum. There are, in addition, Forbush decreases in the electron intensity frequently coincident with those in the neutron monitor. It is concluded that these characteristics all support the hypothesis of a galactic origin for the electrons observed during quiet-time increases.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 71-76
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  • 100
    Publication Date: 2016-06-07
    Description: Observations of the scatter-free electron events from solar active region McMath No. 8905 are presented. The measurements were made on Explorer 33 satellite. The data show that more than 80% of the electrons from these events undergo no or little scattering and that these electrons travel only approximately 1.5 a.u. between the sun and the earth. The duration of these events cannot be accounted fully by velocity dispersion alone. It is suggested that these electrons could be continuously injected into interplanetary medium for a time interval of approximately 2 to 3 minutes. Energy spectra of these electrons are discussed.
    Keywords: SPACE RADIATION
    Type: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 65-70
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