OBSERVATIONAL EVIDENCE FOR QUANTIZATION IN PHOTOSPHERIC MAGNETIC FLUX

被引：69

作者：

LIVINGSTON, W

HARVEY, J

机构：

[1] Kitt Peak National Observatory, Tucson, Ariz.

来源：

SOLAR PHYSICS | 1969年 / 10卷 / 02期

关键词：

D O I：

10.1007/BF00145516

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations are presented which suggest that away from sunspots photospheric magnetic flux is quantized. Assuming the elemental area of a magnetic region to be 1 (arc-sec)2 the elemental field strength is 525 G. © 1969 D. Reidel Publishing Company.

引用

页码：294 / +

页数：1

共 5 条

[1] Beckers J. M., 1968, SOL PHYS, V4, P142
[2] Chapman G. A., 1968, Solar Physics, V5, P442, DOI 10.1007/BF00147012
[3] MAGNETOGRAPH MEASUREMENTS WITH TEMPERATURE-SENSITIVE LINES
HARVEY, J
LIVINGSTON, W
[J]. SOLAR PHYSICS, 1969, 10 (02) : 283 - +
[4] MAGNETOGRAPH OBSERVATIONS OF QUIET SUN .I. SPATIAL DESCRIPTION OF BACKGROUND FIELDS
LIVINGSTON, WC
[J]. ASTROPHYSICAL JOURNAL, 1968, 153 (3P1) : 929 - +
[5] EVOLUTION OF PHOTOSPHERIC NETWORK
SHEELEY, NR
[J]. SOLAR PHYSICS, 1969, 9 (02) : 347 - &

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