STRUCTURAL-CHANGES IN THE SOLAR CORONA DURING THE JULY 1991 ECLIPSE

被引：0

作者：

ZIRKER, JB

KOUTCHMY, S

NITSCHELM, C

STELLMACHER, G

ZIMMERMANN, JP

MARTINEZ, P

KIM, I

DZUBENKO, N

KUROCHKA, L

MAKAROV, V

FATIANOV, M

RUSIN, V

KLOCOK, L

MATSUURA, OT

机构：

[1] CNRS, INST ASTROPHYS PARIS, 98 BIS BLVD ARAGO, F-75014 PARIS, FRANCE

[2] NATL SOLAR OBSERV, SUNSPOT, NM 88349 USA

[3] ECOLE NATL SUPER AERONAUT & ESPACE, F-31055 TOULOUSE, FRANCE

[4] MOSCOW MV LOMONOSOV STATE UNIV, STERNBERG ASTRON INST, MOSCOW 119899, USSR

[5] KIEV UNIV, DEPT PHYS, KIEV 252127, USSR

[6] PULKOVO OBSERV, ST PETERSBOURG, USSR

[7] KISLOVODSK HIGH ALTITUDE OBSERV, KISLOVODSK, USSR

[8] SLOVAK ACAD SCI, INST ASTRON, CS-05960 TATRANSKA LOMNIC, CZECHOSLOVAKIA

[9] UNIV SAO PAULO, INST ASTRON & GEOFIS, BR-4200 SAO PAULO, BRAZIL

来源：

ASTRONOMY & ASTROPHYSICS | 1992年 / 258卷 / 02期

关键词：

SOLAR CORONA; TOTAL ECLIPSE; MAGNETIC STRUCTURE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Preliminary results of the analysis of radially filtered pictures obtained at several hours interval during the July 11, 1991 total solar eclipse are given. Instrumental parameters and method are outlined. Structural changes are discussed.

引用

页码：L1 / L4

页数：4

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