COSMIC RAY INTENSITY VARIATIONS DURING 1966

The recorders have continued as during the last years by one neutron monitor, one cubical telescope and four inclined telescopes in Uppsala and Kiruna. Tables and figures give a detailed account of diurnal and semidiurnal variations during 1966. Six decreases are illustrated in one-hour diagrams. (A...

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Bibliographic Details
Main Authors: Sandstrom,Arne E., Dyring,Eric, Larfors,Ove, Lindgren,Stig, Sporre,Bert
Other Authors: UPPSALA UNIV (SWEDEN) COSMIC RAY GROUP
Format: Text
Language:English
Published: 1967
Subjects:
Astrophysics
(*SOLAR DISTURBANCES
INTENSITY)
(*PERIODIC VARIATIONS
*COSMIC RAYS)
SWEDEN
ROTATION
COSMIC RAYS
PHYSICS LABORATORIES
RADIATION MEASURING INSTRUMENTS
COUNTING METHODS
ASTRONOMICAL OBSERVATORIES
NEUTRON COUNTERS
NEUTRON DETECTORS
NEUTRON FLUX
NEUTRONS
DIURNAL VARIATIONS
TABLES(DATA)
HARMONIC ANALYSIS
Kiruna
Online Access:http://www.dtic.mil/docs/citations/AD0664341
http://oai.dtic.mil/oai/oai?&verb=getRecord&metadataPrefix=html&identifier=AD0664341
Description
Summary:The recorders have continued as during the last years by one neutron monitor, one cubical telescope and four inclined telescopes in Uppsala and Kiruna. Tables and figures give a detailed account of diurnal and semidiurnal variations during 1966. Six decreases are illustrated in one-hour diagrams. (Author) See also AD-653 580.

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