1887
banner image
No data available.
Please log in to see this content.
You have no subscription access to this content.
No metrics data to plot.
The attempt to load metrics for this article has failed.
The attempt to plot a graph for these metrics has failed.
-dimensional generalized Johnson model for cosmic dust-ion-acoustic nebulons with symbolic computation
Rent:
Rent this article for
USD
10.1063/1.2402916
/content/aip/journal/pop/13/12/10.1063/1.2402916
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/12/10.1063/1.2402916
View: Figures

Figures

Image of FIG. 1.
FIG. 1.

From left to right: (a) Absorption of background starlight by the dark cloud Barnard 68 because of the interstellar dust it contains; (b) Ring nebula (M57), about one light-year across and 2000 light-years away in the northern constellation Lyra; (c) Supernova 1987A, the brightest supernova in recent history occurred in the Large Magellanic Clouds in 1987, with its mysterious externalities confirmed by the Hubble Space Telescope in 1994; (d) The first radio occultation observation of Saturn’s rings in 2005 by the Cassini-Huygens mission with simultaneous radio signals sent from Cassini through the rings to Earth. [Pictures reprinted with permission of (a) Ref. 1 (credit: European Southern Observatory), (b) Ref. 16 and NASA’s general permission, (c) Ref. 27 and NASA’s general permission, and (d) NASA’s general permission (photograph posted: Ref. 29; credit: NASA Jet Propulsion Laboratory).]

Image of FIG. 2.
FIG. 2.

Saturn-F-ring-typed, expanding dark nebulon. Left and middle graphs: extremal surfaces (with and 5, respectively) for the electrostatic potential via solutions (8). Right graph: observable surface, with its least values corresponding to the middle graph cross-sectioned at , with , a typical value characteristic of the Saturn’s F-ring from data in Ref. 3, and values of other parameters taken as , , , , , and .

Image of FIG. 3.
FIG. 3.

Supernova-shell-typed, expanding bright nebulon. Left and middle graphs: extremal surfaces (with and 30, respectively) for via solutions (8). Right graph: observable surface with its maximum crests or peaks corresponding to the middle graph cross-sectioned at , with , a typical value characteristic of the supernova shells from data in Ref. 3, and other parameters as , , , , , and .

Loading

Article metrics loading...

/content/aip/journal/pop/13/12/10.1063/1.2402916
2006-12-26
2014-04-24
Loading

Full text loading...

This is a required field
Please enter a valid email address
752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: (3+1)-dimensional generalized Johnson model for cosmic dust-ion-acoustic nebulons with symbolic computation
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/12/10.1063/1.2402916
10.1063/1.2402916
SEARCH_EXPAND_ITEM