Jovian emission at 18 cm during the comet S-L 9 impacts observed with RATAN-600 radio telescope

Gosachinskij, I. V.; Morozov, A. S.; Venger, A. P.

doi:10.1007/bf00612886

Cited by 2 publications

(1 citation statement)

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“…Stankevich et al (1995a, b) report dips in thermal emission at 0.81 and 3.66 cm, perhaps due to shielding by an optically thin cloud layer in the stratosphere. An undisputed enhancement in synchrotron emission at 6 to 90 cm occurred during impact week de Pater et al 1995;Gosachinskij et al 1994;Klein et al 1995;Leblanc and Dulk 1995;Mingaliev and Stolyarov 1995;Sukumar 1995). Long wavelength bursts at 16.7 to 40 MHz associated with several of the impacts were reported (Carr et al 1995;Cousins et al 1994;Han et al 1994;Oya et al 1994;Zhang et al 1994).…”

Section: And Proposed Explanationsmentioning

confidence: 97%

Astrophysics in 1995

Trimble¹,

Leonard²

1996

PASP

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Ap95 differs from Ap91 to Ap94 primarily in Ap number. That is, it once again attempts to highlight some areas of our mutual science where a major event has occurred during the year (a possible solution of the Type II supernova problem, the faintness of quasar host galaxies, the collision of Shoemaker-Levy 9 with Jupiter), but also to focus on some topics where dogged determination is producing more gradual advances (dense star clusters, the second-parameter problem, inventories of nearby objects, and dark-matter candidates). In moderate departure from the rules of Ap92-94, there has been some deliberate up-dating of topics discussed previously. The topics are only partly ordered from nearby to far away.

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