DETECTION OF NIGHT-TIME COSMIC X-RAY EFFECTS IN THE MIDDLE ATMOSPHERE AT LOW LATITUDES

1980 ◽  
pp. 79-82
Author(s):  
Y.V. Ramanamurty
Keyword(s):  
Middle Atmosphere ◽  
Night Time ◽  
X Ray ◽  
Low Latitudes ◽  
Ray Effects

A REVIEW OF MAGNETIC X-RAY EFFECTS

1987 ◽  
Vol 48 (C9) ◽  
pp. C9-989-C9-996 ◽  
Author(s):  
M. J. COOPER
Keyword(s):  
X Ray ◽  
Ray Effects

A theory of magneto-X-ray effects in FCC cobalt

1990 ◽  
Vol 2 (47) ◽  
pp. 9451-9456 ◽  
Author(s):  
P Strange ◽  
B L Gyorffy
Keyword(s):  
X Ray ◽  
Ray Effects

scholarly journals Recent Dynamic Studies on the Middle Atmosphere at Mid- and Low-Latitudes Using Rayleigh Lidar and Other Technologies

2018 ◽  
pp. 757-776
Author(s):  
Alain Hauchecorne ◽  
Sergey Khaykin ◽  
Philippe Keckhut ◽  
Nahoudha Mzé ◽  
Guillaume Angot ◽  
...  
Keyword(s):  
Middle Atmosphere ◽  
Dynamic Studies ◽  
Low Latitudes ◽  
Rayleigh Lidar

scholarly journals STUDIES ON X-RAY EFFECTS

1921 ◽  
Vol 33 (4) ◽  
pp. 433-439 ◽  
Author(s):  
Waro Nakahara ◽  
James B. Murphy
Keyword(s):  
The State ◽  
X Rays ◽  
X Ray ◽  
Small Doses ◽  
Ray Effects ◽  
Lymphoid Proliferation ◽  
Marked Suppression

Mice treated with small doses of x-rays and inoculated with cancer immediately afterwards, show a marked suppression of lymphoid proliferation. If, however, the cancer inoculation is made 7 days after the exposure to x-rays, thus permitting the primary lymphoid stimulation known to occur soon after the x-ray treatment to arise, a second stimulation takes place in a large proportion of mice thus inoculated. Changes in the blood of mice x-rayed and inoculated with cancer 7 days afterwards show that the state of resistance to cancer inoculation is attended by blood lymphocytosis, as is the case in all other varieties of immunity to transplanted cancer so far studied.

scholarly journals X-RAY EFFECTS IN FRUIT TREES

Hereditas ◽  
2010 ◽  
Vol 35 (3) ◽  
pp. 269-279 ◽  
Author(s):  
I. GRANHALL ◽  
Å. GUSTAFSSON ◽  
FR. NILSSON ◽  
E. J. OLDÉN
Keyword(s):  
Fruit Trees ◽  
X Ray ◽  
Ray Effects

scholarly journals Interstellar Matter in Globular Clusters

1988 ◽  
Vol 126 ◽  
pp. 411-422
Author(s):  
Morton S. Roberts
Keyword(s):  
Mass Loss ◽  
Globular Clusters ◽  
Galactic Plane ◽  
Interstellar Matter ◽  
Sherlock Holmes ◽  
Night Time ◽  
X Ray ◽  
Upper Limits ◽  
Intracluster Matter

“Is there any point to which you would wish to draw my attention?”“To the curious incident of the dog in the night-time.”“The dog did nothing in the night-time.”“That was the curious incident,” remarked Sherlock Holmes.Memoirs of Sherlock HolmesThe source for intracluster matter is seen in various mass loss processes ongoing within clusters and is supported by the theoretical need for mass loss to explain the morphology of cluster colormagnitude diagrams. A variety of techniques ranging from X-ray to radio wavelengths have been employed to search for such matter but with few exceptions has not been found. The amount of material expected to collect between cleansing passages through the galactic plane has variously been estimated at between ∼ 102 and ∼ 103 M⊙. In contrast, observed upper limits for many clusters are well below these values, often > 1 M⊙. The few detections are at levels of ≲10−2 M⊙.

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