Scattering Properties of Interstellar Particles. I. Diffuse Galactic Radiation

1968 ◽  
Vol 152 ◽  
pp. 59 ◽  
Author(s):  
Adolf N. Witt
Keyword(s):  
Galactic Radiation

scholarly journals A Survey of Galactic Radiation at 178 Mc/s

1962 ◽  
Vol 124 (6) ◽  
pp. 459-476 ◽  
Author(s):  
A. J. Turtle ◽  
J. E. Baldwin
Keyword(s):  
Galactic Radiation

A survey of the cosmic radiation exposure of Air Canada pilots during maximum galactic radiation conditions in 2009

2013 ◽  
Vol 49 ◽  
pp. 103-108 ◽  
Author(s):  
L.G.I. Bennett ◽  
B.J. Lewis ◽  
B.H. Bennett ◽  
M.J. McCall ◽  
M. Bean ◽  
...  
Keyword(s):  
Radiation Exposure ◽  
Cosmic Radiation ◽  
Radiation Conditions ◽  
Galactic Radiation

scholarly journals An investigation of galactic radiation in the radio spectrum

1948 ◽  
Vol 192 (1030) ◽  
pp. 425-445 ◽  
Keyword(s):  
Reference Signal ◽  
Galactic Structure ◽  
General Distribution ◽  
Method Of Successive Approximations ◽  
Galactic Centre ◽  
Finite Width ◽  
Main Body ◽  
Astronomical Data ◽  
The Galaxy ◽  
Galactic Radiation

An investigation of the distribution of the sources of galactic radiation at 64 Mcyc./sec. is described. Methods are discussed by which the characteristics of the receiving antenna were measured and by which the magnitude of the received galactic power was estimated by comparison with a reference signal of similar amplitude characteristics. The method of analysis of results is described in detail, with emphasis on the need for allowing for the finite width of the main cone of reception of signal power and for the sensitivity of the antenna to signal sources outside the main cone. The necessary corrections are effected by a method of successive approximations, and contours of the distribution of the signal source between declinations + 50° and — 30° are derived. The results are expressed in terms of power flux and also of effective aerial temperature. Possible sources of error are discussed and an accuracy better than 1.2 db. (30 %) is expected for the regions of highest radiation intensity. Reference is made to the fluctuations observed in the radiations coming from Cygnus. The correlation of the derived distribution of galactic radiations with other astronomical data is discussed with special reference to the galactic structure. It is shown that correlation with the near galactic structure, as indicated by the general distribution of visible sources of light, is not very good, but that a more satisfactory correlation is obtained with data which are believed to be characteristic of the structure of the galaxy as a whole. The bias to the south of the galactic circle shown by radiation sources in the vicinity of the galactic centre is especially significant. Various relevant astronomical data are collected together in the accompanying diagrams. The bearing of these correlations on the question of the nature of the source of radiation is examined. It is shown that they do not clearly favour any one theory, and that neither a simple theory in terms of a distributed source in interstellar gas nor one in terms of discrete centres of radiation analogous to sunspots appears adequate to account for the observed phenomena. It is suggested that sources of both types contribute to the observed radiation and that, in general, they must be very distant and associated with the main body of the galaxy.

scholarly journals Diffuse Galactic Radiation.

1967 ◽  
Vol 72 ◽  
pp. 838 ◽  
Author(s):  
Adolf N. Witt
Keyword(s):  
Galactic Radiation

scholarly journals The Gem Project: An International Collaboration to Survey Galactic Radiation Emission

2005 ◽  
pp. 113-122
Author(s):  
S. Torres1 ◽  
V. Canon ◽  
R. Casas ◽  
A. Umana ◽  
C. Tello ◽  
...  
Keyword(s):  
International Collaboration ◽  
Radiation Emission ◽  
Galactic Radiation

THE EXPERIMENTAL DATA ON THE HIGH ENERGY GALACTIC COSMIC RAYS FROM EAS-TOP

2005 ◽  
Vol 20 (29) ◽  
pp. 6817-6820
Author(s):  
◽  
P. L. GHIA ◽  
G. NAVARRA
Keyword(s):  
Experimental Data ◽  
Cosmic Rays ◽  
Energy Range ◽  
High Energy ◽  
Galactic Cosmic Rays ◽  
Direct Measurements ◽  
Galactic Radiation

We summarize the main results reported by EAS-TOP in the study of cosmic rays in the energy range 1012 – 1016 eV (from the direct measurements up to above the "knee"), i.e. the region which is generally considered to represent the high energy galactic radiation.

Galactic radiation belts

Nature ◽  
1979 ◽  
Vol 282 (5737) ◽  
pp. 386-388 ◽  
Author(s):  
J. G. Luhmann
Keyword(s):  
Radiation Belts ◽  
Galactic Radiation

scholarly journals Galactic Radiation at Radio Frequencies. V. The Sea Interferometer

1953 ◽  
Vol 6 (4) ◽  
pp. 420 ◽  
Author(s):  
JG Bolton ◽  
OB Slee
Keyword(s):  
Radio Frequencies ◽  
Galactic Radiation

The factors involved in the study of discrete sources of galactic noise by the sea interferometer are discussed. Three new forms of sea interferometer which increase the effectiveness of this technique are described.

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