Large scale properties of the interplanetary magnetic field
Solar effects and properties of interplanetary magnetic field
Schatten, K. H.↗
Engineering topics
Schatten, K. H.
Publications and source records attributed to Schatten, K. H..
Current sheet magnetic model for the solar corona
Current sheet magnetic model to calculate quiet large-scale magnetic field in solar corona compared with accuracy of other models
Schatten, K. H.↗
The magnetic field structure in the active solar corona.
The structure of the magnetic field of the active solar corona is discussed with reference to optical and radio observations of the solar atmosphere. Eclipse observations provide evidence of fine scale structures in the solar atmosphere that appear to relate to the coronal magnetic field. The coronal magnetic field used for comparison is calculated from potential theory; the influence of solar activity upon the potential theory field is discussed with reference to observations of the Faraday rotation of a microwave signal from Pioneer 6 as it was occulted by the solar atmosphere. Evidence has been found suggesting the existence of expanding magnetic bottles located at 10 solar radii above flaring active regions. The dynamics of these events is discussed. It is further suggested that these magnetic bottles are an important component in the solar corona.
Schatten, K. H.↗
A 'source surface theory' corollary - The mean solar field-interplanetary field correlation
Sun daily mean-interplanetary polarized magnetic fields correlation, using source surface model
Schatten, K. H.↗
The prediction of coronal and interplanetary magnetic fields
Solar coronal structure and interplanetary magnetic fields prediction based on magnetic models, testing accuracy at solar eclipses
Schatten, K. H.↗
Use of two magnetometers for magnetic field measurements on a spacecraft
Methods and equipment for measuring spacecraft magnetic fields
Behannon, K. W.↗
Photospheric magnetic field rotation - Rigid and differential
Photospheric magnetic field direction autocorrelation showing differential and rigid rotation properties at various heliographic latitudes
Howard, R.↗
The quasi-stationary coronal magnetic field and electron density as determined from a Faraday rotation experiment
Quasi-stationary coronal magnetic field and electron density from Faraday rotation experiment, using theoretical model
Levy, G. S.↗
The prediction of coronal and interplanetary magnetic fields
Prediction of coronal and interplanetary magnetic fields
Schatten, K. H.↗
The magnetic field geometry of Jupiter and its relation to Io modulated Jovian decametric radio emission
Jovian magnetic field geometry and Io modulated decametric radio emission
Ness, N. F.↗
Preliminary comparison of predicted and observed structure of the solar corona at the eclipse of March 7, 1970
Solar corona predicted and observed structure compared during eclipse of 7 March 1970
Schatten, K. H.↗
A ''source surface theory'' corollary - The mean solar field-interplanetary field correlation
Correlation of daily mean solar magnetic field with polarity of interplanetary magnetic fields near earth
Schatten, K. H.↗
Evidence for a coronal magnetic bottle at 10 solar radii
Coronal magnetic bottle at ten solar radii from Faraday rotation measurements of occulted spacecraft radio source
Schatten, K. H.↗
Prediction of the coronal structure for the solar eclipse of March 7, 1970
Coronal structure prediction for 7 March 1970 solar eclipse, using model for 22 September 1968 eclipse
Schatten, K. H.↗
Flare identification associated with coronal disturbances
Solar flares responsible for Faraday rotation events observed in passage of Pioneer 6 radio signal through solar corona
Schatten, K. H.↗
Search for magnetic monopoles in the moon
Lunar magnetic monopole charge effects on nearby magnetic field configuration
Schatten, K. H.↗
Magnetic potential model for the structure of the solar corona for the March 1970 eclipse
Magnetic potential model of solar corona structure for March 1970 eclipse
Schatten, K. H.↗
Trajectories of Explorers 33, 34 and 35, July 1966 - April 1969
Solar elliptic projection of orbits for Explorer 33, 34, and 35
Behannon, K. W.↗