DocumentCode
1099765
Title
Effects of Sun Spots and Terrestrial Magnetism on Long-Distance Reception of Low-Frequency Waves
Author
Yokoyama, Eitaro ; Nakai, Tomozo
Author_Institution
Electrotechnical Laboratory, Ministry of Communications, Tokyo, Japan
Volume
19
Issue
5
fYear
1931
fDate
5/1/1931 12:00:00 AM
Firstpage
882
Lastpage
890
Abstract
Daily average variations of sun spots and field intensity are not simply related. What mostly occurs are the effects which vary as the period of the sun´s rotation and one-half thereof. Phase relations are generally found in about 180 degrees and 90 degrees. There is no indication of different effects between daylight and darkness waves. The relation between their monthly average variations is, in general, not obvious. However, direct relation is observed on some stations in summer, whereas inverse relation is noted in winter in several cases, the relation being less clear in the latter season. Daily average variations of terrestrial magnetism and field intensity are also not simply related. However, field intensity usually reaches its maximum from two to four days before the day of occurrence of magnetic disturbance and then gradually decreases until it reaches its minimum from two to four days after that day. There is also no indication of different effects between daylight and darkness waves. The relation is not clearly found for monthly average variations.
Keywords
Atmospheric waves; Frequency measurement; Laboratories; Magnetic field measurement; Magnetic separation; Solar radiation; Storms; Sun; Temperature; Time series analysis;
fLanguage
English
Journal_Title
Radio Engineers, Proceedings of the Institute of
Publisher
ieee
ISSN
0731-5996
Type
jour
DOI
10.1109/JRPROC.1931.222396
Filename
1670989
Link To Document