Independent Sets in Restricted Line of Sight Networks

Algorithms for Sensor Systems - Lecture Notes in Computer Science ◽

10.1007/978-3-319-72751-6_16 ◽

2017 ◽

pp. 211-222 ◽

Cited By ~ 1

Author(s):

Pavan Sangha ◽

Prudence W. H. Wong ◽

Michele Zito

Keyword(s):

Independent Sets ◽

Line Of Sight

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Finding Large Independent Sets in Line of Sight Networks

Algorithms and Discrete Applied Mathematics - Lecture Notes in Computer Science ◽

10.1007/978-3-319-53007-9_29 ◽

2017 ◽

pp. 332-343 ◽

Cited By ~ 2

Author(s):

Pavan Sangha ◽

Michele Zito

Keyword(s):

Independent Sets ◽

Line Of Sight

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Independent sets in Line of Sight networks

Discrete Applied Mathematics ◽

10.1016/j.dam.2019.03.029 ◽

2020 ◽

Vol 286 ◽

pp. 100-115 ◽

Cited By ~ 1

Author(s):

Pavan Sangha ◽

Michele Zito

Keyword(s):

Independent Sets ◽

Line Of Sight

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Variation of the amount of hydrogen along the galactic ridge

Symposium - International Astronomical Union ◽

10.1017/s0074180900100889 ◽

1967 ◽

Vol 31 ◽

pp. 171-172

Author(s):

Th. Schmidt-Kaler

Keyword(s):

Surface Brightness ◽

Milky Way ◽

Neutral Hydrogen ◽

Line Of Sight ◽

Optical Surface ◽

Hydrogen Density ◽

Continuous Radiation ◽

Galactic Longitude

The integralNHof neutral-hydrogen density along the line of sight is determined from the Kootwijk and Sydney surveys. The run ofNHwith galactic longitude agrees well with that of thermal continuous radiation and that of the optical surface brightness of the Milky Way.

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Structuring, Motions and Shapes of Corona Emission Line Profiles

International Astronomical Union Colloquium ◽

10.1017/s0252921100025720 ◽

1994 ◽

Vol 144 ◽

pp. 421-426

Author(s):

N. F. Tyagun

Keyword(s):

Emission Line ◽

Filling Factor ◽

Direct Relationship ◽

Coronal Plasma ◽

Line Of Sight ◽

Line Profiles ◽

The Difference ◽

Yellow Line ◽

Red Line

AbstractThe interrelationship of half-widths and intensities for the red, green and yellow lines is considered. This is a direct relationship for the green and yellow line and an inverse one for the red line. The difference in the relationships of half-widths and intensities for different lines appears to be due to substantially dissimilar structuring and to a set of line-of-sight motions in ”hot“ and ”cold“ corona regions.When diagnosing the coronal plasma, one cannot neglect the filling factor - each line has such a factor of its own.

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