The deep-sea Cerenkov muon detector with spatial structure

V. V. Kobylyansky; V. V. Moiseichenko; A. I. Myagkikh; Yu. M. Kharlamov; A. A. Zhuchkov

doi:10.1007/bf02197621

The deep-sea Cerenkov muon detector with spatial structure

Soviet Journal of Physical Oceanography ◽

10.1007/bf02197621 ◽

1992 ◽

Vol 3 (2) ◽

pp. 149-153

Author(s):

V. V. Kobylyansky ◽

V. V. Moiseichenko ◽

A. I. Myagkikh ◽

Yu. M. Kharlamov ◽

A. A. Zhuchkov

Keyword(s):

Spatial Structure ◽

Deep Sea ◽

Muon Detector

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Spatial structure of the pink speckled deep-sea shrimp Penaeopsis serrata (Bate, 1881) (Decapoda, Penaeidae) during November-December 2009 in the Colombian Caribbean Sea

Crustaceana ◽

10.1163/156854012x623665 ◽

2012 ◽

Vol 85 (1) ◽

pp. 103-116 ◽

Cited By ~ 1

Keyword(s):

Spatial Structure ◽

Deep Sea ◽

Caribbean Sea

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Observations of the spatial structure of interstellar hydrogen

Symposium - International Astronomical Union ◽

10.1017/s007418090010066x ◽

1967 ◽

Vol 31 ◽

pp. 45-46

Author(s):

Carl Heiles

Keyword(s):

High Resolution ◽

Spatial Structure ◽

Velocity Dispersion ◽

Temperature Variations

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.

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