Bison performance

被引：117

作者：

Chaplin, WJ ^{[1
]}

Elsworth, Y ^{[1
]}

Howe, R ^{[1
]}

Isaak, GR ^{[1
]}

McLeod, CP ^{[1
]}

Miller, BA ^{[1
]}

VanderRaay, HB ^{[1
]}

Wheeler, SJ ^{[1
]}

New, R ^{[1
]}

机构：

[1] SHEFFIELD HALLAM UNIV,SCH SCI,SHEFFIELD S1 1WB,S YORKSHIRE,ENGLAND

来源：

SOLAR PHYSICS | 1996年 / 168卷 / 01期

关键词：

D O I：

10.1007/BF00145821

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Since 1981 we have been operating the Birmingham Solar-Oscillations Network (BiSON), a global network of resonant-scattering spectrometers, observing the low-l solar p modes. Here we discuss historical developments, culminating in the establishment of a 6-station network in 1992 September, and the subsequent performance of that network. The data record of each station from 1992 to 1994 has been analysed in terms of weather and equipment breakdowns. Our early experience suggests that the best long-term coverage possible with a 6-station network is limited in practice to about 80%, which falls short of previous predictions.

引用

页码：1 / 18

页数：18

共 20 条

[11] FOSSAT E, 1995, ASTRONOMICAL SOC PAC, P387
[12] FULL-DISK OBSERVATIONS OF SOLAR OSCILLATIONS FROM THE GEOGRAPHIC SOUTH-POLE - LATEST RESULTS
GREC, G
FOSSAT, E
POMERANTZ, MA
[J]. SOLAR PHYSICS, 1983, 82 (1-2) : 55 - 66
[13] HARVEY J, 1982, SKY TELESCOPE, V64, P520
[14] ON THE EXPECTED PERFORMANCE OF A SOLAR OSCILLATION NETWORK
HILL, F
NEWKIRK, G
[J]. SOLAR PHYSICS, 1985, 95 (02) : 201 - &
[15] ATOMIC BEAM SPECTROPHOTOMETER
ISAAK, GR
[J]. NATURE, 1961, 189 (476) : 373 - &
[16] FREQUENCY STABILITY OF SOLAR OSCILLATIONS
JEFFERIES, SM
PALLE, PL
VANDERRAAY, HB
REGULO, C
CORTES, TR
[J]. NATURE, 1988, 333 (6174) : 646 - 649
[17] LAZREK M, 1993, ASTRON ASTROPHYS, V280, P704
[18] LEIBACHER J, 1995, ASTRONOMICAL SOC PAC, P381
[19] THE MEASUREMENT OF LONG-PERIOD OSCILLATIONS AT SACRAMENTO-PEAK-OBSERVATORY AND SOUTH-POLE
STEBBINS, R
WILSON, C
[J]. SOLAR PHYSICS, 1983, 82 (1-2) : 43 - 54
[20] ULRICH R, 1995, ASTRONOMICAL SOC PAC

← 1 2 →