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  • SPACE RADIATION  (371)
  • Polymer and Materials Science
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  • 1970-1974  (371)
  • 1945-1949
  • 1971  (371)
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  • 1970-1974  (371)
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  • 1
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 105-110
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  • 2
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: JPL Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 242-244
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  • 3
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: JPL Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 222-227
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  • 4
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 92-104
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  • 5
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 111-135
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  • 6
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Manned Spacecraft Center The Gemini Program: Phys. Sci. Expt. Sum.; p 215-225
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  • 7
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    In:  CASI
    Publikationsdatum: 2006-08-20
    Schlagwort(e): SPACE RADIATION
    Materialart: Res. in the Space Sci., v. 2; 10 p
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  • 8
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    Publikationsdatum: 2011-08-16
    Beschreibung: Nuclear characteristics of plutonium fuel for thermoelectric generators and required shield thicknesses for sensitive radiation experiment in outer planet spacecraft
    Schlagwort(e): SPACE RADIATION
    Materialart: ; ADEMIE DES SCIENCES
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  • 9
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    Publikationsdatum: 2011-08-16
    Beschreibung: Cosmic ray transport in random magnetic fields, deriving coupled integrodifferential equations for radiant intensity and flux
    Schlagwort(e): SPACE RADIATION
    Materialart: ; 104-111. (
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  • 10
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    Publikationsdatum: 2011-08-16
    Beschreibung: Spectrum and galactic isotropy of diffuse cosmic X rays by balloon-borne detector
    Schlagwort(e): SPACE RADIATION
    Materialart: ; TROPHYSICAL JOURNAL
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  • 11
    Publikationsdatum: 2011-08-16
    Beschreibung: Galactic weak X ray sources observation in Southern Hemisphere for flux and energy spectrum
    Schlagwort(e): SPACE RADIATION
    Materialart: ; 17 (
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  • 12
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    Publikationsdatum: 2011-08-16
    Beschreibung: Cosmic ray produced radionuclides in Lost City meteorite, determining concentrations by nondestructive two-parameter gamma ray analysis
    Schlagwort(e): SPACE RADIATION
    Materialart: ; - PHYSICAL METALLURG
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  • 13
    Publikationsdatum: 2011-08-16
    Beschreibung: Isotropic cosmic gamma ray flux, discussing extragalactic point sources detection by high resolution spectrometers
    Schlagwort(e): SPACE RADIATION
    Materialart: ; 1 (
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  • 14
    Publikationsdatum: 2011-08-16
    Beschreibung: Multiple periodicity of Cygnus X-1 X ray emission from rocket sounding
    Schlagwort(e): SPACE RADIATION
    Materialart: ; ADEMIE DES SCIENCES
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  • 15
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    Publikationsdatum: 2011-08-16
    Beschreibung: Stellar wind flow models associating energy transport with propagation and dissipation of hydrodynamic waves and heat conduction
    Schlagwort(e): SPACE RADIATION
    Materialart: ; ECTRON (
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  • 16
    Publikationsdatum: 2011-08-16
    Beschreibung: Solar cosmic ray acceleration and propagation from time variation and heliocentric distance dependence of relative abundance of protons to helium nuclei
    Schlagwort(e): SPACE RADIATION
    Materialart: ; OMBUSTION IN A FLOW
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  • 17
    Publikationsdatum: 2011-08-16
    Beschreibung: Solar flare two stage particle acceleration from X-ray burst observations, discussing induced electric field and Fermi mechanism
    Schlagwort(e): SPACE RADIATION
    Materialart: ; TROPHYSICAL JOURNAL
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  • 18
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    Publikationsdatum: 2011-08-16
    Beschreibung: Soft galactic X rays role in interstellar grains alignment
    Schlagwort(e): SPACE RADIATION
    Materialart: ; VUE SCIENTIFIQUE ET
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  • 19
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    Publikationsdatum: 2011-08-16
    Beschreibung: Recurrent solar cosmic ray events and M region magnetic storms
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 20
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    Publikationsdatum: 2011-08-16
    Beschreibung: Short duration proton energy increases observation by Explorer 34, considering interpretation as acceleration associated interplanetary shocks
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 21
    Publikationsdatum: 2011-08-16
    Beschreibung: Satellite observations of trapped electrons at low and high altitudes for 6 month period in 1965
    Schlagwort(e): SPACE RADIATION
    Materialart: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 22
    Publikationsdatum: 2011-08-16
    Beschreibung: Particle and field oscillations and electron heating due to drift mirror instability in magnetosphere
    Schlagwort(e): SPACE RADIATION
    Materialart: 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
    Publikationsdatum: 2011-08-16
    Beschreibung: Correlation of increases in electron population of outer radiation belt and interplanetary magnetic fields during two geomagnetic storms
    Schlagwort(e): SPACE RADIATION
    Materialart: 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
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 20; Oct. 197
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  • 25
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    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 20; Oct. 197
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  • 26
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    Publikationsdatum: 2011-08-16
    Beschreibung: Solar X-ray line emission, using crystal spectrometers during large chromospheric flare
    Schlagwort(e): SPACE RADIATION
    Materialart: ; HYSICAL PROCESSES IN
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  • 27
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    Publikationsdatum: 2011-08-16
    Beschreibung: Proposed model with with neutrons as energy source for solar corona, discussing validity based on capture gamma ray flux expectation
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 28
    Publikationsdatum: 2011-08-16
    Beschreibung: Excess intensities of diffuse cosmic X rays related to characteristic line spectrum excitation and element abundances in interstellar region and nebulas
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 29
    Publikationsdatum: 2011-08-16
    Beschreibung: Solar wind deflection due to permanent lunar surface magnetism
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 30
    Publikationsdatum: 2011-08-16
    Beschreibung: Line emission in X ray background in galactic plane and at galactic pole based on rocket flight data
    Schlagwort(e): SPACE RADIATION
    Materialart: ; SEARCH(
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  • 31
    Publikationsdatum: 2011-08-16
    Beschreibung: Low energy cosmic ray H 2 and He 3 nuclei intensities /1967-1968/ from Pioneer 8 and IMP 4 measurements
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 32
    Publikationsdatum: 2011-08-16
    Beschreibung: Continuous optical conversion to IR and directional stellar radiation flow conversion to diffused radiation fields in circumstellar dust envelopes
    Schlagwort(e): SPACE RADIATION
    Materialart: ; VUE SCIENTIFIQUE ET
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  • 33
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    Publikationsdatum: 2011-08-16
    Beschreibung: X ray and far IR measurement inconsistency from Centaurus A, discussing metagalactic submillimeter background
    Schlagwort(e): SPACE RADIATION
    Materialart: ; TROPHYSICAL JOURNAL
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  • 34
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    Publikationsdatum: 2011-08-16
    Beschreibung: Outer radiation belt electron fluxes during solar proton event on 5 Feb. 1965
    Schlagwort(e): SPACE RADIATION
    Materialart: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 35
    Publikationsdatum: 2011-08-16
    Beschreibung: Comparison of electron response in magnetosphere at L equals 5 with solar wind during magnetic storm on 17-18 Apr. 1965
    Schlagwort(e): SPACE RADIATION
    Materialart: 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
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    Publikationsdatum: 2011-08-16
    Beschreibung: Solar wind rotational to tangential discontinuities ratio determination and hypothesis concerning origin in interplanetary magnetic field
    Schlagwort(e): SPACE RADIATION
    Materialart: ; ADEMIE DES SCIENCES
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  • 37
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    Publikationsdatum: 2011-08-16
    Beschreibung: Extragalactic cosmic X ray sources at high galactic latitude from sounding rocket experiments, correlating with galactic clusters
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YSICA STATUS SOLIDI
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  • 38
    Publikationsdatum: 2011-08-16
    Beschreibung: Cosmic ray intensity gradient measurement from Lost City meteorite Ar 37/Ar 39 ratio
    Schlagwort(e): SPACE RADIATION
    Materialart: ; - PHYSICAL METALLURG
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  • 39
    Publikationsdatum: 2011-08-16
    Beschreibung: Magnetospheric electron echo probe experiment, using sounding rocket and injecting gun for controlled particle trapping investigation
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YSICA STATUS SOLIDI
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  • 40
    Publikationsdatum: 2011-08-16
    Beschreibung: Interplanetary magnetic field measurements from lunar surface and lunar orbit, discussing solar wind effects on bulk electrical conductivity of lunar crust
    Schlagwort(e): SPACE RADIATION
    Materialart: ; TROPHYSICAL JOURNAL
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  • 41
    Publikationsdatum: 2011-08-16
    Beschreibung: Line emission in diffuse cosmic X ray continuum, discussing probable interstellar or intergalactic matter source
    Schlagwort(e): SPACE RADIATION
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  • 42
    Publikationsdatum: 2011-08-16
    Beschreibung: 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
    Schlagwort(e): SPACE RADIATION
    Materialart: ; IENCES (
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  • 43
    Publikationsdatum: 2011-08-16
    Beschreibung: Crab Nebula and pulsar NP 0532 X ray spectra discussing pulse profile, emission and interstellar absorption
    Schlagwort(e): SPACE RADIATION
    Materialart: ; BROTECHNIKA, NO. 1(
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  • 44
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    Publikationsdatum: 2011-08-16
    Beschreibung: Decay lifetimes of Starfish electrons in trapped radiation belt inner zone
    Schlagwort(e): SPACE RADIATION
    Materialart: ; BROTECHNIKA, NO. 1(
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  • 45
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    Publikationsdatum: 2011-08-16
    Beschreibung: Diffusion coefficient estimation for energetic charged particles across magnetic fields from mathematical model
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YAL SOCIETY (
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  • 46
    Publikationsdatum: 2011-08-16
    Beschreibung: Cyclotron and bounce resonance scattering of electrons trapped in earth magnetic field
    Schlagwort(e): SPACE RADIATION
    Materialart: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 47
    Publikationsdatum: 2011-08-16
    Beschreibung: Fokker-Planck equation used to describe process of electron loss from Van Allen zones due to pitch angle scattering by electromagnetic disturbances
    Schlagwort(e): SPACE RADIATION
    Materialart: 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
    Publikationsdatum: 2011-08-16
    Beschreibung: Cygnus XR-1 X ray intensity fluctuations, discussing time scales and periodicities
    Schlagwort(e): SPACE RADIATION
    Materialart: ; IENCES (
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  • 49
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    Publikationsdatum: 2011-08-16
    Beschreibung: Pulsating gamma ray flux from pulsar NP 0532 in energy range from 250 keV to 2.3 MeV
    Schlagwort(e): SPACE RADIATION
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  • 50
    Publikationsdatum: 2011-08-16
    Beschreibung: Line emission in diffuse X ray background at high galactic latitudes, interpreting rocket observations
    Schlagwort(e): SPACE RADIATION
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  • 51
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    Publikationsdatum: 2011-08-16
    Beschreibung: Submillimeter background radiation origin possibility from extragalactic discrete sources based on cosmological models
    Schlagwort(e): SPACE RADIATION
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  • 52
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    Publikationsdatum: 2011-08-16
    Beschreibung: Nuclear soft core potential reproduction by isoscalar vector meson in nonlocal field theory of fireball in high energy cosmic ray collisions
    Schlagwort(e): SPACE RADIATION
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  • 53
    Publikationsdatum: 2011-08-16
    Beschreibung: Energetic electrons generating solar flares position relation with active regions associated with type I radio noise storms
    Schlagwort(e): SPACE RADIATION
    Materialart: ; YSICA STATUS SOLIDI
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  • 54
    Publikationsdatum: 2011-08-16
    Beschreibung: Low energy cosmic ray intensity increase at propagating interplanetary shock wave front, discussing one dimensional model with particles undergoing convection and diffusion
    Schlagwort(e): SPACE RADIATION
    Materialart: ; BROTECHNIKA, NO. 1(
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  • 55
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    Publikationsdatum: 2011-08-16
    Beschreibung: Relativistic electrons acceleration in solar proton flares, taking into account plasma density and magnetic field intensity
    Schlagwort(e): SPACE RADIATION
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  • 56
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    Publikationsdatum: 2011-08-16
    Beschreibung: Cosmic ray intensity Forbush decrease on 23 September 1966 coincidence with magnetic storm sudden commencement from satellite and ground based monitors data
    Schlagwort(e): SPACE RADIATION
    Materialart: ; 63 (
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  • 57
    Publikationsdatum: 2011-08-16
    Beschreibung: Satellite observations of distribution of energetic protons in earth radiation belts between 1962 - 1964
    Schlagwort(e): SPACE RADIATION
    Materialart: REDUCTION AND ANALYSIS OF PARTICLE DATA FROM EXPLORER 15 AND EXPLORER 26 28 FEB. 1971 (SEE N71-30919 18-29)
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  • 58
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    Publikationsdatum: 2011-08-16
    Beschreibung: Transient behavior of electrons in artificial radiation belts from satellite observations
    Schlagwort(e): SPACE RADIATION
    Materialart: 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
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    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Space Science Reviews; 12; Dec. 197
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  • 60
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Planetary and Space Science; 19; Dec. 197
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  • 61
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Atmospheric and Terrestrial Physics; 33; Dec. 197
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  • 62
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Nature Physical Science; 234; Nov. 8
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  • 63
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 76; Dec. 1
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  • 64
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 20; Oct. 197
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  • 65
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Physical Review Letters; 27; Nov. 8
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  • 66
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: Galatic radio spur association with soft X ray emission
    Schlagwort(e): SPACE RADIATION
    Materialart: ; VIGATION (
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  • 67
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Cosmic Electrodynamics; 2; Oct. 197
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  • 68
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 21; Dec. 197
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  • 69
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 21; Dec. 197
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  • 70
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    In:  Other Sources
    Publikationsdatum: 2011-08-16
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Planetary and Space Science; 19; Oct. 197
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  • 71
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    Publikationsdatum: 2011-08-16
    Beschreibung: Suprathermal proton bremsstrahlung cross section calculation, using Weizsacker-Williams method
    Schlagwort(e): SPACE RADIATION
    Materialart: ; - PHYSICAL AND RADIO
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  • 72
    Publikationsdatum: 2011-08-16
    Beschreibung: Diffuse cosmic X rays small scale structure, comparing Wolfe-Burbridge theoretical autocorrelation functions for galaxies clusters and superclusters with experimental value
    Schlagwort(e): SPACE RADIATION
    Materialart: ; ADEMIE DES SCIENCES
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  • 73
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    In:  CASI
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 53-58
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  • 74
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 42-46
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  • 75
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 33-41
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  • 76
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 9-18
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  • 77
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 1-8
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  • 78
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    In:  Other Sources
    Publikationsdatum: 2018-12-01
    Beschreibung: Book on cosmic gamma rays covering secondary particle decay, electron-positron annihilation, proton-antiproton interactions, galactic radiation and cosmology
    Schlagwort(e): SPACE RADIATION
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  • 79
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    In:  Other Sources
    Publikationsdatum: 2018-12-01
    Beschreibung: Galactic and solar cosmic ray propagation, variations, and energy spectra
    Schlagwort(e): SPACE RADIATION
    Materialart: PROC. OF THE SIXTH WINTER SCHOOL ON SPACE PHYS., PART 2 1971; P 33-93
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  • 80
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    In:  CASI
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA. Goddard Space Flight Center The Gum Nebula and Related Probl.; p 163-165
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  • 81
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    In:  CASI
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: The Gum Nebula and Related Probl.; p 97-109
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  • 82
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 71-76
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  • 83
    Publikationsdatum: 2016-06-07
    Beschreibung: 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.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 65-70
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  • 84
    Publikationsdatum: 2016-06-07
    Beschreibung: Proton, helium, and medium nuclei energy spectra have been measured from the Explorer 35 satellite for a recent solar flare. Above 2 MeV/nucleon these spectra are based upon single and dual parameter pulse height analysis in addition to threshold rate counting. Pulse height analysis of medium nuclei is assigned a high priority for telemetry readout so that telemetry does not become saturated by the high proton intensity. In this manner the number of pulse height analyzed medium nuclei has been increased by a factor of approximately 200. Individual medium nuclei have been resolved in the energy interval 8 - 23 MeV/nucleon.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 59-64
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  • 85
    Publikationsdatum: 2016-06-07
    Beschreibung: An ionization spectrometer consisting of 10.8 radiation lengths of tungsten and 35 radiation lengths of iron has been used to determine the energy spectrum of cosmic ray electrons above 10 GeV. The spectrometer was calibrated with electrons from 5.4 to 18 GeV and then flown at an altitude of 6 gm-cm/2 for 16 hours. Separation of electron initiated events from proton events was achieved by utilizing starting point distributions, the shower development in tungsten, and the energy deposited in the large thickness of iron absorber. The exponent of the differential energy spectrum of the electrons is -3.1 + or - 0.2 while the exponent of the background is consistent with the proton exponent of -2.7 + or -0.2.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 27-32
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  • 86
    Publikationsdatum: 2016-06-07
    Beschreibung: An ionization spectrometer consisting of 12 layers of tungsten each 6.13 gm cm/2 thick and 7 iron modules each 70 gm cm/2 thick was flown in a balloon at an altitude of 6 gm cm/2 for 16 hours. The distributions of the first interaction points are used to determine the mean free path of the incident particles. At energies of 20 GeV the proton m.f.p. of 140 gm cm/2 is in agreement with that of other workers. The m.f.p.'s of heavy nuclei have been determined as a function of energy up to a total energy of 1000 GeV. These results are compared with the overlap model of nucleus-nucleus collisions. For C nuclei interacting with W the overlap parameter is -2.6 x 10/13 cm. The energy dependence of this parameter is discussed.
    Schlagwort(e): SPACE RADIATION
    Materialart: Goddard Space Flight Center Contrib. to the Twelfth Intern. Conf. on Cosmic Rays; p 19-25
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  • 87
    Publikationsdatum: 2019-06-27
    Beschreibung: X-ray emission from the Cygnus Loop was observed in the energy region around 0.2 to 1 keV with a collector that focused X-rays along one dimension while scanning across the nebula. The total integrated intensity is 13 nanoerg per square centimeter per second. The one-dimensional X-ray structure has the same angular size - about 3 degrees - as the outermost boundaries of the optical filaments. There is no increase in X-ray emission at the center of the nebula nor at the strong feature that is seen in certain radio maps. The X-ray spectrum is consistent with thermal radiation from a hot plasma at a temperature of about 4 million K.
    Schlagwort(e): SPACE RADIATION
    Materialart: Science; 172; Apr. 23
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  • 88
    Publikationsdatum: 2019-06-27
    Beschreibung: We have used the Ar-40/Ar-39 dating technique on eight samples of Apollo 14 rocks (14053, 14310), breccia fragments (14321), and soil fragments (14001, 14167). The large basalt fragments give reasonable Ar-40/Ar-39 release patterns and yield well defined crystallization ages of 3.89-3.95 aeons. Correlation of the Ar-40/Ar-39 release patterns with Ar-39/Ar-37 patterns showed that the low temperature fractions with high radiogenic argon loss came from K-rich phases. A highly shocked sample and fragments included in the breccia yield complex release patterns with a low temperature peak. The total argon age of these fragments is 3.95 aeons. Cosmic ray exposure ages on these samples are obtained from the ratio of spallogenic Ar-38 to reactor induced Ar-37 and show a distinct grouping of low exposure ages of 26 m.y. correlated with Cone crater. Other samples have exposure ages of more than 260 m.y. and identify material with a more complex integrated cosmic age exposure history.
    Schlagwort(e): SPACE RADIATION
    Materialart: Earth and Planetary Science Letters; 12; Sept
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  • 89
    Publikationsdatum: 2019-06-27
    Beschreibung: The solar particle events of 18 November 1968, 25 February 1969, and 30 March 1969 were studied using data from the detector system aboard the lunar orbiting satellite Explorer 35. Protons, alpha particles, and Z or = 3 nuclei were registered in the solid state detector of the system. Interplanetary propagation, particle anisotropy, and the intensity ratios of protons to alpha particles and of alpha particles to C, N, and O nuclei above a common specific energy of 0.5 MeV/nucleon were studied. Diffusion coefficients and decay constants for the three events are given, as well as magnitudes and directions of anisotropies.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-CR-126661 , U-OF-IOWA-71-27
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  • 90
    Publikationsdatum: 2019-06-27
    Beschreibung: A description is given of a wide dynamic range pulse height analyzer system developed for use on High Energy Cosmic Ray Experiment (HECRE) Balloon Flights. A wide dynamic range of 100,000 is obtained by extending the range of a basic 1024 channel analyzer through the use of multiple ranges and range selection. The system described here contains four 100,000 pulse height analyzers. Each 100,000 pulse height analyzer consists of a group of cordwood welded modules mounted and interconnected on a printed circuit card. Four of these card assemblies, the required clock drive circuitry (discrete components mounted and interconnected on a separate card) and three input-output connectors are interconnected and mounted on the system board.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-TM-X-65836 , X-711-71-500
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  • 91
    Publikationsdatum: 2019-06-27
    Beschreibung: Kinetic and hydrodynamic descriptions of a collisionless solar wind proton gas are compared. Heat conduction and viscosity are neglected in the hydrodynamic formulation but automatically included in the kinetic formulation. The results of the two models are very nearly the same, indicating that heat conduction and viscosity are not important in the solar wind proton gas beyond about 0.1 AU. It is concluded that the hydrodynamic equations provide a valid description of the collisionless solar wind protons, and hence that future models of the quiet solar wind should be based on a hydrodynamic formulation.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-CR-125802
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  • 92
    Publikationsdatum: 2019-06-27
    Beschreibung: Impulsive increases in the low energy proton flux observed by the Explorer 34 satellite, in very close time association with geomagnetic storm sudden commencements are described. It is shown that these events are of short duration (20-30 min) and occur only during the decay phase of a solar cosmic-ray flare event. The differential energy spectrum and the angular distribution of the direction of arrival of the particles are discussed. Two similar increases observed far away from the earth by the Pioneer 7 and 8 deep-space probes are also presented. These impulsive increases are compared with Energetic Storm Particle events and their similarities and differences are discussed. A model is suggested to explain these increases, based on the sweeping and trapping of low energy cosmic rays of solar origin by the advancing shock front responsible for the sudden commencement detected on the earth.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 21; Dec. 197
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  • 93
    Publikationsdatum: 2019-06-27
    Beschreibung: Use of a balloon-borne counter telescope with a gas Cerenkov counter to measure the energy of primary cosmic ray electrons between 2 and 200 GeV. Electrons are identified by the characteristic electron-photon shower which they produce in a 15 radiation length deep stack of high-Z material interleaved with scintillation counters. Calibrations with monoenergetic electrons up to 14 GeV and monoenergetic protons up to 28 GeV from accelerators are used to develop criteria to statistically separate electrons from proton-induced events. The results from six balloon flights (total exposure time 63 hours) are combined to obtain the electron energy spectrum. Up to about 30 GeV, the spectrum measured in this experiment can be directly checked with calibrations and agrees well with results from other experiments. Above this energy, the flux reported in the present work is somewhat higher than the determinations reported by most other authors. An apparent flattening of the energy spectrum above 50 GeV is not regarded as significant. There is no evidence for a steepening of the spectrum at energies below 200 GeV.
    Schlagwort(e): SPACE RADIATION
    Materialart: Astrophysics and Space Science; 14; Dec. 197
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 94
    Publikationsdatum: 2019-06-27
    Beschreibung: An analytic solution was obtained to the complete Fokker-Planck equation including the effects of convection, interplanetary deceleration and acceleration, corotation, and anisotropic diffusion. The solution yields a time to maximum for the particle flux of about 10 h and an exponential decay time of about 5 h. Several solar flare particle events were observed with the solar and galactic cosmic ray experiment on OGO-6. Comparisons of the calculated time dependence of the fluxes with these observations of 1 to 70 MeV protons show that the model adequately describes both the rise and decay times.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-CR-128295 , SRL-71-3
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 95
    Publikationsdatum: 2019-06-27
    Beschreibung: An explicit expression is obtained for the phase matrix in the I, Q, U, and V Stokes vector representation for a system containing a polydispersion of spherical particles. All of the symmetry relations derived by Hovenier using general arguments are established explicitly. Convenient algorithms are given for the computation of the phase matrix for a spherical polydispersion. Since this theory is so vitally important in radiative transfer, many researchers will need to compute these functions for realistic aerosols distributions. Therefore, results are presented for a haze L distribution so that other researchers will have a way of checking their programs which compute these quantities.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-CR-128174
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 96
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2019-06-27
    Beschreibung: The formation of the strongest ultra-violet emission lines of Mg II, O I, C II, and C III in the solar atmosphere is studied in detail. The equations of statistical equilibrium and radiative transfer for each ion are solved using a general computer program that is capable of solving non-LTE line-formation problems for arbitrary atmospheric and atomic models. Interpreting the results in terms of the structure of the solar atmosphere, it is concluded that the HSRA atmosphere has a temperature too low by about 500 K near h = 1100 km and that a temperature plateau with T sub e approximately = 18,000 K and width close to 60 km exists in the upper chromosphere. The structure of the solar atmosphere in the range 20,000 to 100,000 K and the effects of microturbulence on the formation of lines are also investigated. Approximate analytic line-formation problems are solved, and more exact solutions are derived later. An attempt is made to make the best possible fit to the Ca II K line center-to-limb profiles with a one-component atmosphere, with an assumed source function and microturbulent velocity.
    Schlagwort(e): SPACE RADIATION
    Materialart: NASA-CR-125981 , SAO-SPECIAL-REPT-338
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 97
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: Development of a model to account for the release of solar cosmic rays from the sun. The solar atmosphere out to 3 to 5 solar radii above the photosphere is permeated with magnetic field lines which trap low-rigidity (less than or equal to 50 MV) flare particles. Plasma heated by the flare process disturbs the trapping field, and not until the disturbance reaches 3 to 5 solar radii can the low-rigidity flare particles have access to interplanetary space. If the plasma is not heated sufficiently to overcome the coronal field, flare particles are trapped efficiently. Subsequent leakage of these particles into interplanetary space forms corotating streams. Reference is made to satellite observations of solar electromagnetic radiation and charged particles.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 20; Nov. 197
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 98
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: Observation of a flare surge at the limb in C III 977 A by the Harvard OSO 6 spectroheliometer. The kinematic behavior of the surge is the same in C III and in H alpha. The amount of C III emission is consistent with a model in which the C III ions occupy sheaths with a thickness of about 100 km surrounding the cooler H alpha-emitting threads. The mass of the material containing C III ions is about 0.01 times that emitting H alpha.
    Schlagwort(e): SPACE RADIATION
    Materialart: Solar Physics; 20; Nov. 197
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 99
    Publikationsdatum: 2019-06-27
    Beschreibung: The observations of impulsive solar-flare X-rays above 10 keV made with OGO-5 satellite have been analyzed in order to study the variation of the nonthermal electron spectrum from one flare to another. The X-ray spectrum at the maxima of 129 impulsive X-ray bursts is represented by KE to the minus-gamma power photons per sq cm per sec per keV, and the frequency of occurrence of bursts with different values of gamma is studied. It is found that for gamma less than 4.0 the frequency of bursts rapidly decreases with the decrease in the value of gamma. The probability of occurrence of a burst with gamma less than 2.3 is extremely small.
    Schlagwort(e): SPACE RADIATION
    Materialart: NSSDC-ID-68-014A-04-PM , Astrophysical Journal; 170; Dec. 15
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 100
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2019-06-27
    Beschreibung: The observation reported by Murray et al. (1971), in which a feature or ?kink' in the kinetic-energy spectrum of solar cosmic rays from a solar burst was seen to decrease with time, is examined. By means of calculations based on a model for cosmic ray bursts, it is demonstrated that the observed rate cannot be interpreted immediately as the rate of loss of energy, and factors are indicated which must be considered in the interpretation of the data.
    Schlagwort(e): SPACE RADIATION
    Materialart: Journal of Geophysical Research; 76; Dec. 1
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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