Вращение Солнца и звезд и циклы их активности
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Головна астрономічна обсерваторія НАН України
2009
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| Schriftenreihe: | Кинематика и физика небесных тел |
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| Zitieren: | Вращение Солнца и звезд и циклы их активности / О.С. Гопасюк, С.И. Гопасюк // Кинематика и физика небесных тел. — 2009. — Т. 25, № 3. — С. 199-206. — Бібліогр.: 21 назв. — рос. |
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irk-123456789-727452014-12-30T03:01:59Z Вращение Солнца и звезд и циклы их активности Гопасюк, О.С. Гопасюк, С.И. Физика Солнца 2009 Article Вращение Солнца и звезд и циклы их активности / О.С. Гопасюк, С.И. Гопасюк // Кинематика и физика небесных тел. — 2009. — Т. 25, № 3. — С. 199-206. — Бібліогр.: 21 назв. — рос. 0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/72745 524.376+ 523.9E ru Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| language |
Russian |
| topic |
Физика Солнца Физика Солнца |
| spellingShingle |
Физика Солнца Физика Солнца Гопасюк, О.С. Гопасюк, С.И. Вращение Солнца и звезд и циклы их активности Кинематика и физика небесных тел |
| format |
Article |
| author |
Гопасюк, О.С. Гопасюк, С.И. |
| author_facet |
Гопасюк, О.С. Гопасюк, С.И. |
| author_sort |
Гопасюк, О.С. |
| title |
Вращение Солнца и звезд и циклы их активности |
| title_short |
Вращение Солнца и звезд и циклы их активности |
| title_full |
Вращение Солнца и звезд и циклы их активности |
| title_fullStr |
Вращение Солнца и звезд и циклы их активности |
| title_full_unstemmed |
Вращение Солнца и звезд и циклы их активности |
| title_sort |
вращение солнца и звезд и циклы их активности |
| publisher |
Головна астрономічна обсерваторія НАН України |
| publishDate |
2009 |
| topic_facet |
Физика Солнца |
| url |
http://dspace.nbuv.gov.ua/handle/123456789/72745 |
| citation_txt |
Вращение Солнца и звезд и циклы их активности / О.С. Гопасюк, С.И. Гопасюк // Кинематика и физика небесных тел. — 2009. — Т. 25, № 3. — С. 199-206. — Бібліогр.: 21 назв. — рос. |
| series |
Кинематика и физика небесных тел |
| work_keys_str_mv |
AT gopasûkos vraŝeniesolncaizvezdiciklyihaktivnosti AT gopasûksi vraŝeniesolncaizvezdiciklyihaktivnosti |
| first_indexed |
2025-07-05T21:29:12Z |
| last_indexed |
2025-07-05T21:29:12Z |
| _version_ |
1836844007870693376 |
| fulltext |
OI,I3I4KA COJIHIIA KI4HEMATI4KA
I,I OI43I4KA
HEEECHbIX
TEJI rou 25 Ns 3 2009
yAK 524.376 + 523.9E
O. C. lonacox, C.l I . Ionacnx
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c noc mep exy6 aHuJtru nepio)auu uaz uimuoi arcmua uoc mi.
THE ROT:ATTONS OF THE SUN AND SruRS AND THEIR ACTIVITY
CYCLES, by Gopasyut O. S., Gopasyuk S. 1. - The expression for the
determination of the magnetic activity period for lower main-sequence stars is
derived from the analysis of drift of magnetic structures with the solar cycle
activity. The expression linked the activity period of a star with its rotation
period 7,o,, B - V color index and average level of chromospheric emission
(n'n). fhe activity periorls for 30 stars (14 young anrt 16 oltl stars) from the
Wilson sample are calculated. The calculatetl and observetl activity periods
are in good agreement.
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o,qa aKTr{BHocru T[r, or Ha6,rroAaeMoro rrepuo;ia T"r, orAenbHo Ars Mo,'roAbrx
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crr{ cocraBr4nt 0.66 r.r 0.63 Arrr MonoAbrx r,r crapbrx 3Be3A coorBercrseHHo. Bce
UOTYTICHHbIC BbIBOAbI CNPABCA,'IIIBbI NPU YC,'IOBIIIT, IITO APEfiO MATHIITHbIX
crpyKTyp o6yc.rronaeH BpauleHr4eM 3Be3Abr, u nce $rasnuecKne npoqeccbr, uporrc-
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HeFo BparqeHr{rr 3BegAbr, KoHBeKrIrlr4 n ryp6yaeHrHocrrr.
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JreHa yrJroBoft cropoctrrc BpauleHurr 3Be3Abr vr Brvrs,er Ha npoAo,'r)Kr4TeJrbHocrb
urrKJ'ra uargnrnori aKTrlBHocrr4 3Be3rbr.
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nepr{oAoM ee BparrleHr,rfl, noKa3areJreM rlBera r,r noKa3areJreM xpoMocSepHofi
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noKa3areJrb xportroc$epHoit swuccuu trurtuir H vr K Ca II, u neprloA aKT[BHocrr{
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MO,'rOAbrX eneeq na6.rroAaeMbre nepHoAbr 6o,rr'rue BbrrrucJreHHbrx n 6-7 pas.
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sB,'rseTcrr pe3y,'rbTaroM HarpeBa xporrroc$epu, cBq3aHHoro c MarHr4THbrMr{ [o,'rs-
Mr4 Ha noBepxHocrrr 3Be3Abr, Bo-nroprrx, cpeAnr,rrl ypoBeHb xporr.roc$epHofi
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nocJ'reAoBareJrbHocrr,r s 6o,rruer; creneHrr ynpaBrserc{ napaMeTpow T,o,/t, -
quc,rroM Pocc6n (T, - BpeMs o6opora KoHBeKTuBHoro sJreMeHra). Be.nprqltra
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MeHee aKTr{BHbrx MeAJreHHo Bparqanquxcs (crapbrx) 3Be3Aax, [oAo6Hbrx Coan-
qy [6, 14]. Torqa, ecJ'rr xpoMoc$epnar gMr{ccrlfl or nqreH He yBenr,rquBaercs
nponopqnoHa,'rbHo c yBennr{eHrreM MarHr,ITHoro noroKa nrrreH (na Coanqe
xporraoc$epHaq 3Mr4ccr,rrr yMeHr,[raercrr HaA nqrHauu) vr ecJrvr Ha 6r'rc'rponparqa-
roullrxcr Kapnr,rKax (uoroAux seesAax) Ao,rc MarHr4THoro rroroKa, npnxoAsulaq-
cs Ha rrqTHa, 6o,rrrue, To oTHorueHue H- u K-SMlvtccvtrr or 3Be3Abr Moxer
AOCTI,ITaTb HaCbIIrIeHI,Ig C yBeJlr{r{eHrreM Ar{HaMO-aKTI{BHOCTI{ Aa)Ke B TOM CJIyr{ae,
ec.ru o6ulnri uarHurnrrfi noroK He yBennqunaerca [13].
Taxlru o6pasou, [epuoA MarHr4THofi aKTrrBHocru 3Be3A 3aBr.rcr,rr or MHorr{x
rapaMerpoB (nnpaxenue (6)). Ao6aureHr,re KoHBeKrIuu vr cvrrrbr Kopuoruca
Mox.er noBJrr,rrrb Ha cKopocrb oceBoro BparqeHr,rs 3Be3Abr c r,ry6nuofi, uro
cyulecrBeHHo u3MeHlrr cKopocrb aperiSa MarHr4THbrx crpyKryp rr, coorBercrBeH-
HO, npoAoJ'I)Kr4TeJ'rr,HocTb MaIHI,ITHOT0 qnKna. Eeeyc'rorHo, BaxHo 3HaTr, B
Aera.rrrx cBq3b Me)KAy orHorrreHr,rflMr4 oMuccnu Ca II u no4$oroc$epHbrMr.r
MarHr4THbrMr4 noroKaMn Anrr 3Be3A pa3nr{rrHbrx cneKTpanbHbrx KJraccoB rr c
pa3,'rr4qHbrMr4 cKopocrrrMr4 BpauleHurr, unQopr"raqurc o nnoulaAu noKpbrrr4rr
nrrrHaMr4 (rpxocrr'ro nonepxHocru) u nnoulaAr,r noKpbrrrlrr xpouocQepHuvra
aKTr4BHbrMr4 o6aacrcNara.
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