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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Wood science and technology 2 (1968), S. 292-298 
    ISSN: 1432-5225
    Source: Springer Online Journal Archives 1860-2000
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition , Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Description / Table of Contents: Zusammenfassung An Holz von Zweitwuchs-Ponderosa pine wurden die Rohdichte und die Schwindung bestimmt. Zu diesem Zweck wurden in Abständen von 4.8 m Stammscheiben entnommen. Das Holz dieser Bäume unterschied sich von jenen aus Altbeständen mit engen Jahrringen durch etwas niedrigere Rohdichtewerte sowie etwas niedrigere Radial-und Tangentialschwindung und durch etwas höhere Werte der Längsschwindung. Das Holz der aus dem Stammfuß entnommenen Scheiben erwies sich als dichter und zeigte häufig anormal hohe Schwindung und unregelmäßigen Faserverlauf. In den höher gelegenen Stammteilen beschränkte sich die übernormale Längsschwindung auf den Kernteil mit rund 25... 50 mm Durchmesser, d. h. auf den Bereich der ersten 2... 3 Jahrringe. Von diesen Ausnahmen ab-gesehen, zeigte das weitringige Holz eine ziemlich gleichmäßige Qualität. In diesem Zusammenhang wird empfohlen, den Fällungsschnitt etwas höher als gewölnlich anzusetzen, wenn es darauf ankommt, auch für den Erdstamm gleichmäßigere Holzqualität zu erzielen.
    Notes: Summary Wood specific gravity and shrinkage determinations were made on disks cut at 16-foot intervals from eight open-grown wide ringed second-growth ponderosa pines. This wood differed from forest grown narrower-ringed wood by having somewhat lower values for specific gravity and radial and tangential shrinkage and slightly higher values for axial shrinkage. Wood from the lowermost (stump) disks was denser and often had excessive axial shrinkage and irregular grain. At higher levels in the tree excessive axial shrinkage was limited to a 1... 2-inch core including the first 2... 3 growth rings. With these exceptions, the wideringed wood was uniform in quality. Slightly higher stumps were advocated if more uniform quality along the length of the butt log is desired.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Solar physics 10 (1969), S. 245-253 
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A very high quality wiggly-line spectrogram was analyzed by making high-resolution spectral scans of numerous small solar features. An attempt from the line profiles to detect a magnetic field difference between the granular and intergranular regions, resulted in a field increase of 20 ± 15 G in the darker regions of the granular field. Line width increases apparently due to small-scale turbulent velocities are seen in the darker regions. It is postulated that in general darker regions show increased turbulent velocities. Conspicuous asymmetries in line profiles are seen in dark intergranular regions. It is suggested that these are the result of velocity gradients in the downward flow of material. An ionized Cr line showed a conspicuous increase in equivalent width in the darker regions of the granular field, thus indicating a decrease in electron pressure in these areas.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Solar physics 7 (1969), S. 28-38 
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A study of the Mount Wilson magnetic-field synoptic chart material divided into latitude zones for the interval 1959–67, and a comparison of the data with sunspot groups have provided a better understanding of the structure of the background-field pattern and its relation to activity. The interaction of old and new fields within the pattern seems to result in long-lived sections of alternating polarity in both hemispheres. We postulate subsurface sources with rotation periods of about 27 days which produce active regions over a longitude zone of some tens of degrees. There is a tendency for the background-field features with strong fields to resist to some extent the shearing effects of differential rotation. A prediction is made concerning the nature of the interplanetary magnetic field above the ecliptic.
    Type of Medium: Electronic Resource
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  • 4
    Publication Date: 1969-04-01
    Print ISSN: 0038-0938
    Electronic ISSN: 1573-093X
    Topics: Physics
    Published by Springer
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  • 5
    Publication Date: 1969-12-01
    Print ISSN: 0038-0938
    Electronic ISSN: 1573-093X
    Topics: Physics
    Published by Springer
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