THE EVOLUTION OF ACTIVE REGION LOOP PLASMA

被引：21

作者：

KRALL, KR

ANTIOCHOS, SK

机构：

[1] NASA, GEORGE C MARSHALL SPACE FLIGHT CTR, SPACE SCI LAB, HUNTSVILLE, AL 35812 USA

[2] STANFORD UNIV, INST PLASMA RES, STANFORD, CA 94305 USA

[3] STANFORD UNIV, DEPT APPL PHYS, STANFORD, CA 94305 USA

来源：

ASTROPHYSICAL JOURNAL | 1980年 / 242卷 / 01期

关键词：

D O I：

10.1086/158470

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：374 / 382

页数：9

共 16 条

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[3] STABILITY OF SOLAR CORONAL LOOPS [J].

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[5]

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VAIANA, GS .

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[7] OBSERVATIONAL EVIDENCE OF CONTINUAL HEATING IN X-RAY EMITTING CORONAL LOOPS [J].

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NOLTE, JT .

SOLAR PHYSICS, 1978, 57 (01) :103-110

[8]

LANDINI M, 1975, ASTRON ASTROPHYS, V42, P213

[9]

LEVINE RH, 1977, SOL PHYS, V51, P83, DOI 10.1007/BF00240447

[10] DETERMINATION OF PLASMA PARAMETERS FROM SOFT-X-RAY IMAGES FOR CORONAL HOLES (OPEN MAGNETIC-FIELD CONFIGURATIONS) AND CORONAL LARGE-SCALE STRUCTURES (EXTENDED CLOSED-FIELD CONFIGURATIONS) [J].

MAXSON, CW ;

VAIANA, GS .

ASTROPHYSICAL JOURNAL, 1977, 215 (03) :919-&

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