Variations in the H Ly alpha intensity in solar activity cycles from measurements onboard satellites and rockets

Citation
Tv. Kazachevskaya et Vv. Katyushina, Variations in the H Ly alpha intensity in solar activity cycles from measurements onboard satellites and rockets, PHYS CH P C, 25(5-6), 2000, pp. 425-427
Citations number
11
Categorie Soggetti
Earth Sciences
Journal title
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE
ISSN journal
14641917 → ACNP
Volume
25
Issue
5-6
Year of publication
2000
Pages
425 - 427
Database
ISI
SICI code
1464-1917(2000)25:5-6<425:VITHLA>2.0.ZU;2-J
Abstract
Data on radiation intensity of the Sun's Lyman-alpha hydrogen line (lambda= 121.6 nm) for a maximum and minimum of solar activity are considered. Resul ts of longterm measurements, received onboard 5 American and 9 Russian sate llites and space vehicles for a period from 1969 till 1998, as well as data of numerous rocket measurements, since 1955 are analyzed. Radiation of the quiet Sun (without flares) in the L alpha line differs between phases of a solar activity cycle and changes from cycle to cycle were observed. Radiation intensity at the minimum of a solar activity cycle varies from (2 .25 - 4.3).10(11) cm(-2)s(-1) for activity minimum to (6.1 - 9).10(11) cm(- 2)s(-1) for a maximum of a cycle. (C) 2000 Elsevier Science Ltd. All rights reserved.