Time-lag of cosmic-ray intensity

The best correlation coefficient between the monthly cosmic-ray intensity of the Inuvik Station and various kinds of solar, interplanetary, and geophysical parameters has been found. It is calculated for different time-lags of cosmic-ray intensity with respect to these parameters. The maximum of the...

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Bibliographic Details
Main Authors: Mavromichalaki, H., Petropoulos, B.
Format: Article in Journal/Newspaper
Language:English
Published: 1984
Subjects:
Inuvik
Online Access:https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3019589
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record_format openpolar
spelling ftnkunivathens:oai:lib.uoa.gr:uoadl:3019589 2024-02-11T10:05:20+01:00 Time-lag of cosmic-ray intensity Mavromichalaki, H. Petropoulos, B. 1984-01-01 https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3019589 Αγγλικά English eng uoadl:3019589 https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3019589 scientific_publication_article Επιστημονική δημοσίευση - Άρθρο Περιοδικού Scientific publication - Journal Article 1984 ftnkunivathens 2024-01-18T18:38:17Z The best correlation coefficient between the monthly cosmic-ray intensity of the Inuvik Station and various kinds of solar, interplanetary, and geophysical parameters has been found. It is calculated for different time-lags of cosmic-ray intensity with respect to these parameters. The maximum of these coefficients lead us to a useful empirical model for the 11-year cosmic-ray modulation. © 1984 D. Reidel Publishing Company. Article in Journal/Newspaper Inuvik Pergamos - Library and Information Center of National and Kapodistrian University of Athens Inuvik ENVELOPE(-133.610,-133.610,68.341,68.341)
institution Open Polar
collection Pergamos - Library and Information Center of National and Kapodistrian University of Athens
op_collection_id ftnkunivathens
language English
description The best correlation coefficient between the monthly cosmic-ray intensity of the Inuvik Station and various kinds of solar, interplanetary, and geophysical parameters has been found. It is calculated for different time-lags of cosmic-ray intensity with respect to these parameters. The maximum of these coefficients lead us to a useful empirical model for the 11-year cosmic-ray modulation. © 1984 D. Reidel Publishing Company.
format Article in Journal/Newspaper
author Mavromichalaki, H.
Petropoulos, B.
spellingShingle Mavromichalaki, H.
Petropoulos, B.
Time-lag of cosmic-ray intensity
author_facet Mavromichalaki, H.
Petropoulos, B.
author_sort Mavromichalaki, H.
title Time-lag of cosmic-ray intensity
title_short Time-lag of cosmic-ray intensity
title_full Time-lag of cosmic-ray intensity
title_fullStr Time-lag of cosmic-ray intensity
title_full_unstemmed Time-lag of cosmic-ray intensity
title_sort time-lag of cosmic-ray intensity
publishDate 1984
url https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3019589
long_lat ENVELOPE(-133.610,-133.610,68.341,68.341)
geographic Inuvik
geographic_facet Inuvik
genre Inuvik
genre_facet Inuvik
op_relation uoadl:3019589
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3019589
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