Heating of H I regions by soft X rays. II - The effect of galactic soft X-ray sources
Galactic soft X ray and subcosmic ray heating and ionizing of interstellar H I regions
Rees, M. J.↗
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A multiple-plate, multiple-pinhole camera for X-ray gamma-ray imaging
Plates with identical patterns of precisely aligned pinholes constitute lens system which, when rotated about optical axis, produces continuous high resolution image of small energy X-ray or gamma ray source. Camera has applications in radiation treatment and nuclear medicine.
Hoover, R. B.↗
On the origin and isotropy of the cosmic gamma-ray flux between 1 and 6 MeV and its implications for future gamma-ray
Origin and isotropy of cosmic gamma ray flux between 1 and 6 MeV and its implications of future gamma ray investigations
Stecker, F. W.↗
Observed galactic hard X-ray emission as an indication for cosmic ray heating of instellar HI
Intensity and spectral shape of diffuse X ray emission by galactic disk from cosmic ray heating of interstellar hydrogen
Boldt, E. A.↗
Autocorrelation and power spectrum analysis for X-ray and gamma ray spectrometer data
Autocorrelation and power spectrum analysis computer programs for signal analysis of X ray and gamma ray emitting pulsars
Tsai, C. F.↗
Microscopic observations of X-ray and gamma-ray induced decomposition of ammonium perchlorate crystals
The X-ray and gamma-ray induced decomposition of ammonium perchlorate was studied by optical, transmission, and scanning electron microscopy. This material is a commonly used oxidizer in solid propellents which could be employed in deep-space probes, and where they will be subjected to a variety of radiations for as long as ten years. In some respects the radiation-induced damage closely resembles the effects produced by thermal decomposition, but in other respects the results differ markedly. Similar radiation and thermal effects include the following: (1) irregular or ill-defined circular etch pits are formed in both cases; (2) approximately the same size pits are produced; (3) the pit density is similar; (4) the c face is considerably more reactive than the m face; and (5) most importantly, many of the etch pits are aligned in crystallographic directions which are the same for thermal or radiolytic decomposition. Thus, dislocations play an important role in the radiolytic decomposition process.
Herley, P. J.↗
Identification and control of spacecraft radiation sources of interference to X-ray and gamma-ray experiments
Apollo 15 and 16 will carry instruments for the purpose of measuring X-ray and gamma ray fluxes from the lunar surface and in cis-lunar space. The intensity levels expected are low over most of the energy range of interest, requiring that background contributions be minimized. The radiation sources on Apollo determined and their interference with these instruments evaluated. The results were used as a basis for dealing with this problem and for recommendations applicable to future manned and unmanned missions.
Metzger, A. E.↗
Cosmic-ray effects on diffuse gamma-ray measurements.
Evaluation of calculations and experimental evidence from 600-MeV proton irradiation indicating that cosmic-ray-induced radioactivity in detectors used to measure the diffuse gamma-ray background produces a significant counting rate in the energy region around 1 MeV. It is concluded that these counts may be responsible for the observed flattening of the diffuse photon spectrum at this energy.
Fishman, G. J.↗
A comparison of techniques for inversion of radio-ray phase data in presence of ray bending
Derivations are presented of the straight-line Abel transform and the seismological Herglotz-Wiechert transform (which takes ray bending into account) that are used in the reconstruction of refractivity profiles from radio-wave phase data. Profile inversion utilizing these approaches, performed in computer-simulated experiments, are compared for cases of positive, zero, and negative ray bending. For thin atmospheres and ionospheres, such as the Martian atmosphere and ionosphere, radio wave signals are shown to be inverted accurately with both methods. For dense media, such as the solar corona or the lower Venus atmosphere, the refractive recovered by the seismological Herglotz-Wiechert transform provide a significant improvement compared with the straight-line Abel transform.
Wallio, H. A.↗
The Astrophysics of the Diffuse Background of X-rays and Gamma Rays
The origin of the diffuse X-ray and gamma ray background and some of the astrophysical implications of such radiation background are outlined. The range of energies that is of interest here extends from approximately 100 eV to approximately 10 to the 8th power eV.
Cowsik, R.↗
Design and mathematical analysis of a three-mirror X-ray telescope based on ATM S-056 X-ray telescope hardware
The mathematical design of the aspheric third mirror for the three-mirror X-ray telescope (TMXRT) is presented, along with the imaging characteristics of the telescope obtained by a ray trace analysis. The present design effort has been directed entirely toward obtaining an aspheric third mirror which will be compatible with existing S-056 paraboloidal-hyperboloidal mirrors. This compatability will facilitate the construction of a prototype model of the TMXRT, since it will only be necessary to fabricate one new mirror in order to obtain a working model.
Foreman, J. W., Jr.↗
Gamma-ray astronomy and cosmic-ray origin theory
A theory on the origin of cosmic rays is presented. Specifically, magellanic clouds and the galactic center were investigated as possible cosmic ray sources.
Ginzburg, V. L.↗
Galactic gamma rays: Models involving variable cosmic-ray density
Mathematical models were developed to determine variable cosmic ray flux around the galactic plane. Data indicate point sources, molecular hydrogen concentration, increased cosmic ray density toward the galactic center, and neutral pion production combine to cause radiation density variables in the galactic plane.
Strong, A. W.↗
Feasibility of coherent X-ray production by X-ray pumping
It is suggested that coherent X-rays can be produced by inverting the electron population in a suitable target, such as Li, through irradiation with X-rays generated by fast electrons traversing an electromagnetic field (as in a storage ring). Conditions to be satisfied by target and radiation parameters are stated, and examples given.
Csonka, P. L.↗
Possible evidence for structured acceleration of cosmic rays on a galactic scale from recent gamma-ray observations
Recent data from SAS-2 on the galactic gamma-ray line flux as a function of longitude reveal a broad maximum in the region below 30 deg. These data, as unfolded here, imply that the low-energy (1-10 GeV) galactic cosmic-ray flux varies with the radial distance from the galactic center and is about an order of magnitude higher than the local value in a toroidal region for radial distances between 4 and 5 kpc. We further show that this enhancement can be plausibly accounted for by Fermi acceleration and compression caused by a hydrodynamic shock driven by the expanding gas in the 3-kpc arm and invoked in some versions of galactic structure theory.
Stecker, F. W.↗
A new model of atmospheric gamma rays and its implications for measurement of diffuse cosmic gamma rays from within the atmosphere
A semi-empirical model is discussed which describes atmospheric gamma rays in the range 0.3 less then or equal to E less than or equal to 10 MeV based on the production per unit mass of air. The model is based on the concept of a source strength (photon/g sec MeV) which is energy- and depth-dependent, and derived from measured fluxes. Quantities such as directional fluxes, angular distributions, and growth curves are calculated directly from this model. The source function is described by four energy-dependent parameters determined empirically from fluxes measured with a 7.5 cm x 7.5 cm Nal counter over the atmospheric depth range from 3.5 to 500 g/sq cm. From S(E,x), obtained for both continuum and discrete gamma rays at lambda = 40 deg, the depth and angle dependence of directional fluxes were calculated. Growth-curve predictions needed to separate atmospheric from diffuse cosmic fluxes were determined.
Matteson, J. L.↗
Spectroscopic analysis of solar and cosmic X-ray spectra. 1: The nature of cosmic X-ray spectra and proposed analytical techniques
Techniques for the study of the solar corona are reviewed as an introduction to a discussion of modifications required for the study of cosmic sources. Spectroscopic analysis of individual sources and the interstellar medium is considered. The latter was studied via analysis of its effect on the spectra of selected individual sources. The effects of various characteristics of the ISM, including the presence of grains, molecules, and ionization, are first discussed, and the development of ISM models is described. The expected spectral structure of individual cosmic sources is then reviewed with emphasis on supernovae remnants and binary X-ray sources. The observational and analytical requirements imposed by the characteristics of these sources are identified, and prospects for the analysis of abundances and the study of physical parameters within them are assessed. Prospects for the spectroscopic study of other classes of X-ray sources are also discussed.
Walker, A. B. C., Jr.↗
One-dimensional focusing X-ray telescope for stellar X-ray astronomy
A one-dimensional X-ray telescope of the Kirkpatrick-Baez design is described. The instrument consists of a grazing-incidence X-ray telescope and a multiwire proportional counter. The optics were provided with a gold reflecting surface to yield an energy response from below 0.25 to above 4.0 keV. The angular resolution of the system is 6 min by 9.5 deg over a 1.1 deg by 9.5 deg field of view.
Helava, H.↗