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  • SPACE RADIATION  (535)
  • Inorganic Chemistry  (334)
  • SOLAR PHYSICS  (318)
  • 1975-1979  (622)
  • 1970-1974  (565)
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  • 1
    Publication Date: 2011-08-16
    Description: Detailed analysis of the Pioneer 10 plasma analyzer experiment flight data during the Jupiter flyby in late November and early December 1973 has been performed. The observations show that the interaction of Jupiter's magnetic field with the solar wind is similar in many ways to that at earth, but the scale size is over 100 times larger. Jupiter is found to have a detached standing bow shock wave of high Alfven Mach number. Like the earth, Jupiter has a prominent magnetopause that deflects the magnetosheath plasma and excludes its direct entry into the Jovian magnetosphere. Unlike that of the earth, the sunward hemisphere of Jupiter's outer magnetosphere is found to be highly inflated with thermal plasma and a high-beta region that is highly responsive to changes in solar wind dynamic pressure.
    Keywords: SPACE RADIATION
    Type: Journal of Geophysical Research; 79; Sept. 1
    Format: text
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  • 2
    Publication Date: 2019-06-27
    Description: Pioneer 10 Plasma Analyzer experiment flight data during the Jupiter flyby are presented. The observations show that the interaction of Jupiter's magnetic field with the solar wind is similar in many ways to that at earth, but the scale size is over 100 times larger. Jupiter is found to have a detached standing bow shock wave of high Alfven Mach number. Jupiter has a prominent magnetopause which deflects the magnetosheath plasma and excludes its direct entry into the Jovian magnetosphere. The sunward hemisphere of Jupiter's outer magnetosphere is found to be highly inflated with thermal plasma and a high beta region which is highly responsive to changes in solar wind dynamic pressure. Observational arguments are presented which tend to discount a thin disklike magnetosphere but, rather, favor a Jovian magnetosphere, albeit probabily considerably flattened as compared to the earth's magnetosphere, yet still with reasonable thickness. Results concerning the shock jump conditions, the magnetosheath flow field and inferred internal magnetospheric plasma are presented.
    Keywords: SPACE RADIATION
    Type: NASA-TM-X-62357
    Format: application/pdf
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  • 3
    Publication Date: 2005-11-30
    Description: During the Apollo 16 mission, a solar flare produced an enormous amount of low-energy nuclei, many orders of magnitude greater than the level inferred from studies of tracks in the window of the Apollo 12 spacecraft during a time when the sun was quiet. The differential energy spectrum of nuclei with Z less than or equal to 6 falls by seven orders of magnitude over the interval from 0.1 to 20 MeV/nucleon, then remains almost flat up to approximately 100 MeV/nucleon. The two parts correspond to contributions from the sun and from galactic cosmic rays. Any maximum in the spectrum occurs below the lowest energy studied.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 8 p
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  • 4
    Publication Date: 2011-08-17
    Description: The technical properties, operation, and expected sensitivity are discussed for an experiment intended to search for narrow lines in the spectra of gamma ray bursts during the ISEE-C mission. At the heart of the experiment is a radiatively cooled germanium solid state photon detector. The instrumentation is capable of storing the entire spectrum of all but the largest bursts in the energy range 0.05-6.5 MeV. In addition, it analyzes the signals from two CsI detectors in two other experiments on the spacecraft and records event time histories from these to a few millisecond accuracy. A background mode permits spectral analysis during quiet times and will allow the determination of physically interesting upper limits for narrow lines in the diffuse gamma ray background radiation.
    Keywords: SPACE RADIATION
    Type: Gamma Ray Spectry. in Astrophys.; p 516-528
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  • 5
    Publication Date: 2011-08-17
    Description: Measurements of the gamma-ray emission in the medium-energy range between 15 and 100 MeV, obtained during two balloon flights from Brazil, are presented. The importance of this energy region in determining whether neutral-pion decay or electron bremsstrahlung is the most likely dominant source mechanism is discussed, along with the implications of such observations. Specifically, the data from this experiment suggest that emission from the galactic plane is similar to the theoretical spectrum calculated by Fichtel et al. (1976), including both source mechanisms but with the bremsstrahlung component enhanced by a factor of about 2. A spectral distribution of gamma-rays produced in the residual atmosphere above the instrument is also presented and compared with other data. A rather smooth spectral variation from high to low energies is found for the atmospheric spectrum.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal; vol. 225
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  • 6
    Publication Date: 2019-06-27
    Description: Measurements of the gamma-ray emission in the medium energy range between 15 and 100 MeV, obtained during two ballon flights from Brazil are presented. The importance of this energy region in determining whether pi deg - decay of electron bremsstrahlung is the most likely dominant source mechanism is discussed along with the implications of such observations. Specifically, the data from this experiment suggest that emission from the galactic plane is similar to theoretical spectrum calculations including both sources mechanisms, but with the bremsstrahlung component enhanced by a factor of about 2. A spectral distribution of gamma-rays produced in the residual atmosphere above the instrument is also presented and compared with other data. A rather smooth spectral variation from high to low energies is found for the atmospheric spectrum.
    Keywords: SPACE RADIATION
    Type: NASA-TM-79543
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  • 7
    Publication Date: 2019-06-27
    Description: Skylab/ATM observations of a disappearing filament near the center of the solar disk are described using XUV and H-alpha spectroheliograms, X-ray filterheliograms, and photospheric magnetograms. The temperature of the coronal plasma as the filament disappeared is estimated to have been in excess of 6 million K, and it is noted that the time history of the soft X-ray and microwave fluxes displayed the gradual-rise-and-fall (GRF) signature, suggesting that the present event may have properties that are characteristic of a wide class of long-duration X-ray and radio events. A comparison with other spatially resolved long-duration X-ray events indicates that all such long-lived bursts involve transients in the outer corona and that some two-thirds of them involve either the eruption or the major activation of a prominence. It is also found that long-lived events are characterized by the appearance of new emission loops in the lower corona during the declining phase of the X-ray emission and that these loops sometimes disappear after the X-ray events and sometimes remain indefinitely.
    Keywords: SOLAR PHYSICS
    Type: Solar Physics; 45; Dec. 197
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  • 8
    Publication Date: 2019-06-27
    Description: A balloon-borne magnetic core digitized spark chamber with two assemblies of spark-chambers above and below the scintillation counters was used to measure the medium energy gamma ray flux from the galactic center region. Gamma ray calculations are based on the multiple scattering of the pair electrons in 15 aluminum plates interleaved in the spark chamber modules. Counting rates determined during ascent and at ceiling indicate the presence of diffuse component in this energy range. Preliminary results give an integral flux between 15 and 70 MeV compared to the differential points in other results.
    Keywords: SPACE RADIATION
    Type: NASA-TM-78331 , INPE-1218-PE/122
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  • 9
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 387 (1972), S. 61-71 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: By adding acetyl halide to solutions of copper(I)acetate in mixtures of acetonitrile and acetic acid, highly pure copper(I) halides can be prepared. These form with pyridine and alkylpyridines (= L) yellow or greenish yellow compounds of the formula Cu(L)3X. Colourless compounds of the formula Cu(L)X can be obtained by thermal decomposition of these compounds. All these compounds exhibit an intensive fluorescence of different colours. Some compounds of the formula Cu(L)X change at low temperatures reversibly the fluorescence colour. It is proposed, to use for this phenomenon the term ‘Fluorescence Thermochromism’.
    Notes: Durch Zugabe von Acetylhalogenid zu Lösungen von Kupfer(I)-acetat in Acetonitril/Essigsäuregemischen sind reinste Kupfer(I)-Halogenide darstellbar. Diese bilden mit Pyridin und Alkylpyridinen (= L) gelbe bis grüngelbe Verbindungen der Zusammensetzung Cu(L)3X. Durch thermische Zersetzung können daraus farblose Verbindungen der Zusammensetzung Cu(L)X dargestellt werden. Alle diese Verbindungen zeigen eine intensive Fluoreszenz der verschiedensten Farben. Einige Verbindungen der Zusammensetzung Cu(L)X ändern bei tiefer Temperatur reversibel ihre Fluoreszenzfarbe. Für diese Erscheinung wird der Begriff ‘Fluoreszenz-Thermochromie’ vorgeschlagen.
    Additional Material: 3 Ill.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 409 (1974), S. 345-352 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: On the Existance of Mn (OCOCH3)2 · 2H2OThe existence of manganous acetate dihydrate is predicted and the conditions for its equilibrium existence are proved.The polyterms of solubility of the systems Mn(OCOCH3)2-H2O and Mn(OCOCH3)2- CH3COOH-H2O are studied at 40 and 60°C. The fields of equilibrium existence are determined for the acid manganous acetates of the composition 2 Mn(OCOCH3)2 · CH3COOH · 6H2O and Mn(OCOCH3)2 · CH3COOH · 1.5 H2O at 40°C as well as the fields of the acid salt of the composition Mn((OCOCH3)2 · CH3COOH · H2O a t 60°C. The crystallisation fields of Mn(OCOCH3)2 · 2H2O and Mn(OCOCH3)2 are determined a t 60°C. The results obtained are confirmed by X-ray investigation. The compositions of the solid phases are also determined from thermogravimetric studies.
    Notes: Die Existenz von Mn(OCOCH3)2 · 2 H2O wird vorausgesagt und die Bedingungen für seine Existenz im Gleichgewicht werden bestimmt.Untersucht werden die Löslichkeitsisothermen des Zweistoffsystems Mn(OCOCH3)2-H2O und des Dreistoffsystems Mn(OCOCH3)2-CH3COOH-H2O bei 40 und 60°C. Dabei werden Kristallisationsfelder saurer Acetate folgender Zusammensetzung festgestellt : 2 Mn(OCOCH3)2 · CH3COOH · 6H2O und Mn(OCOCH3)2 · CH3COOH · 1,5 H2O bei 40°C, sowie Mn(OCOCH3)2 · CH3COOH · H2O bei 60°C; bei 60°C ferner Kristallisationsfelder von Mn(OCOCH3)2 · 2H2O und Mn(OCOCH3)2. Diese Ergebnisse wurden auch röntgenographisch und thermogravimetrisch bestätigt.
    Additional Material: 6 Ill.
    Type of Medium: Electronic Resource
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