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13 Result(s)

within R. G. Stone Remove this filter Atmospheric Sciences Remove this filter Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics) Remove this filter

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  1. No Access

    Article

    Evidence for halo-like radio sources from kilometric type III burst observations

    The radio azimuths for many kilometric type III bursts that originate near or behind the limb of the Sun are observed to drift far to the east or far to the west of the spacecraft-Sun line. It is shown that th...

    M. J. Reiner, R. G. Stone in Solar Physics (1990)

  2. No Access

    Article

    Characteristics of solar coronal source regions producing 3He-rich particle events

    We use Hα, X-ray, and kilometric radio data to examine the solar coronal activity associated with energetic (∼1 MeV/nucl−1) 3He-rich particle events observed near Earth. The basis of the study is the 12 3He-rich ...

    S. W. Kahler, R. P. Lin, D. V. Reames, R. G. Stone, M. Liggett in Solar Physics (1987)

  3. No Access

    Article

    Characteristics of shock-associated fast-drift kilometric radio bursts

    The existence of a class of fast-drift, shock-associated (SA), kilometric radio bursts which occur at the time of metric type II emission and which are not entirely the kilometric continuation of metric type I...

    R. J. MacDowall, R. G. Stone, M. R. Kundu in Solar Physics (1987)

  4. No Access

    Article

    A new method for reconstructing type III trajectories

    A local density approximation (LDA) method is developed for reconstructing the trajectories of type III radio bursts through the interplanetary medium. The method uses the measured source directions and the me...

    M. J. Reiner, R. G. Stone in Solar Physics (1986)

  5. No Access

    Article

    Type II solar radio events observed in the interplanetary medium

    Fifteen type II solar radio events have been identified in the 2 MHz to 30 kHz frequency range by the radio astronomy experiment on the ISEE-3 satellite over the period from September 1978 to December 1979. Th...

    H. V. Cane, R. G. Stone, J. Fainberg, J. L. Steinberg, S. Hoang in Solar Physics (1982)

  6. No Access

    Article

    Radio evidence for an expanding magnetic arch beyond 20 solar radii

    A magnetic loop located beyond 20 R ⊙ appears to be the later evolution of an expanding magnetic arch observed at 2 r ⊙. The expansion speed is of the order of 100 km s−1.

    R. G. Stone, Joseph Fainberg in Solar Physics (1975)

  7. No Access

    Article

    Characteristics of type III exciters derived from low frequency radio observations

    Low frequency radio observations (2.8 MHz-67 kHz) from the RAE-1 and IMP-6 satellites allow the tracking of type III solar burst exciters out to large distances from the Sun (of the order of 1 AU). A study of ...

    Larry G. Evans, J. Fainberg, R. G. Stone in Solar Physics (1973)

  8. No Access

    Article

    A comparison of type III solar radio burst theories using satellite radio observations and particle measurements

    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 satelli...

    Larry G. Evans, Joseph Fainberg, R. G. Stone in Solar Physics (1971)

  9. No Access

    Article

    A U-type solar radio burst originating in the outer corona

    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 R ⊙. A possible model of this loop structure ...

    R. G. Stone, Joseph Fainberg in Solar Physics (1971)

  10. No Access

    Article

    Type III solar radio burst storms observed at low frequencies

    The analysis of a storm of type III solar radio bursts observed in August 1968 between 5 and 0.2 MHz by the RAE-1 satellite has yielded the storm morphology, a possible relation to meter and decameter storms, ...

    Joseph Fainberg, R. G. Stone in Solar Physics (1971)

  11. No Access

    Article

    Type III solar radio burst storms observed at low frequencies

    Storms of type III solar radio bursts observed from 5.4 ot 0.2 MHz consist of a quasi-continuous production of type III events observable for half a solar rotation but persisting in some cases for well over a ...

    Joseph Fainberg, R. G. Stone in Solar Physics (1970)

  12. No Access

    Article

    Type III solar radio burst storms observed at low frequencies

    Storms of type III solar radio bursts observed from 5.4 to 0.2 MHz, indicate the quasicontinuous production of type III events observable for a half solar rotation but persisting in some cases for well over a ...

    Joseph Fainberg, R. G. Stone in Solar Physics (1970)

  13. No Access

    Article

    Type III radio bursts in the outer corona

    Type III solar radio bursts observed from 3.0 to 0.45 MHz with the ATS-II satellite over the period April–October 1967 have been analyzed to derive two alternative models of active region streamers in the oute...

    J. K. Alexander, H. H. Malitson, R. G. Stone in Solar Physics (1969)