OSCILLATORY PHENOMENA IN QUIESCENT PROMINENCES

被引：92

作者：

KLECZEK, J

KUPERUS, M

机构：

[1] University Observatory 'Sonnenborgh', Utrecht

来源：

SOLAR PHYSICS | 1969年 / 6卷 / 01期

关键词：

D O I：

10.1007/BF00146797

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A model for horizontal oscillations of prominences is presented. It is found that the model of a freely oscillating prominence surrounded by coronal matter explains satisfactorily the observed periods and damping times, as well as the changes in the prominence shape. © 1969 D. Reidel Publishing Company.

引用

页码：72 / &

共 14 条

[1]

ANDERSON GF, 1966, THESIS U COLORADO

[2]

[Anonymous], 1960, IAU S

[3] OBSERVATIONAL STUDY OF MACROSCOPIC INHOMOGENEITIES IN SOLAR ATMOSPHERE .3. VERTICAL OSCILLATORY MOTIONS IN SOLAR PHOTOSPHERE [J].

EVANS, JW ;

MICHARD, R .

ASTROPHYSICAL JOURNAL, 1962, 136 (02) :493-&

[4]

EVANS JW, 1961, T IAU B, V11, P201

[5]

EVANS JW, 1957, PASP, V69, P426

[6]

HYDER CL, 1966, Z ASTROPHYS, V63, P78

[7]

KLECZEK J, 1963, P ASTRON SOC PACIFIC, V75, P14

[8]

KUIPER G, 1953, SUN, P411

[9]

KUIPER G, 1953, SUN, P410

[10]

LINDSAY RB, 1960, MECHANICAL RADIATION

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