The solar acoustic spectrum and eigenmode parameters

被引:154
作者
Hill, F
Stark, PB
Stebbins, RT
Anderson, ER
Antia, HM
Brown, TM
Duvall, TL
Haber, DA
Harvey, JW
Hathaway, DH
Howe, R
Hubbard, RP
Jones, HP
Kennedy, JR
Korzennik, SG
Kosovichev, AG
Leibacher, JW
Libbrecht, KG
Pintar, JA
Rhodes, EJ
Schou, J
Thompson, MJ
Tomczyk, S
Toner, CG
Toussaint, R
Williams, WE
机构
[1] UNIV CALIF BERKELEY,DEPT STAT,BERKELEY,CA 94720
[2] UNIV CALIF BERKELEY,SPACE SCI LAB,BERKELEY,CA 94720
[3] UNIV COLORADO,JOINT INST LAB ASTROPHYS,BOULDER,CO 80309
[4] TATA INST FUNDAMENTAL RES,BOMBAY 400005,MAHARASHTRA,INDIA
[5] NATL CTR ATMOSPHER RES,HIGH ALTITUDE OBSERV,BOULDER,CO 80307
[6] STANFORD UNIV,NASA,GODDARD SPACE FLIGHT CTR,CTR ASTROPHYS & SPACE SCI,STANFORD,CA
[7] NASA,GEORGE C MARSHALL SPACE FLIGHT CTR,HUNTSVILLE,AL 35812
[8] UNIV LONDON QUEEN MARY & WESTFIELD COLL,ASTRON UNIT,LONDON E1 4NS,ENGLAND
[9] NATL OPT ASTRON OBSERV,NASA,GODDARD SPACE FLIGHT CTR,TUCSON,AZ 85726
[10] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138
[11] CALTECH,PASADENA,CA 91125
[12] UNIV SO CALIF,DEPT PHYS & ASTRON,LOS ANGELES,CA 90089
关键词
D O I
10.1126/science.272.5266.1292
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Global Oscillation Network Group (GONG) project estimates the frequencies, amplitudes, acid linewidths of more than 250,000 acoustic resonances of the sun from data sets lasting 36 days. The frequency resolution of a single data set is 0.321 microhertz. For frequencies averaged over the azimuthal order m, the median formal error is 0.044 microhertz, and the associated median fractional error is 1.6 x 10(-5). For a 3-year data set, the fractional error is expected to be 3 x 10(-6). The GONG m-averaged frequency measurements differ from other helioseismic data sets by 0.03 to 0.08 microhertz. The differences arise from a combination of systematic errors, random errors, and possible changes in solar structure.
引用
收藏
页码:1292 / 1295
页数:4
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