HMI ring diagram analysis II. Data products

被引：45

作者：

Bogart, R. S. ^{[1
]}

Baldner, C. ^{[2
]}

Basu, S. ^{[2
]}

Haber, D. A. ^{[3
]}

Rabello-Soares, M. C. ^{[1
]}

机构：

[1] Stanford Univ, Stanford, CA 94305 USA

[2] Yale Univ, New Haven, CT USA

[3] Univ Colorado, JILA, Boulder, CO 80309 USA

来源：

GONG-SOHO 24: A NEW ERA OF SEISMOLOGY OF THE SUN AND SOLAR-LIKE STARS | 2011年 / 271卷

关键词：

D O I：

10.1088/1742-6596/271/1/012009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The combination of high resolution, spatial coverage, and continuity of photospheric Doppler and other data from HMI has allowed us to embark on a program of systematic exploration of solar subsurface flows and thermal structure variations using the technique of ring-diagram analysis on an unprecedented scale. There are two ring-diagrams pipelines, as described in [1]. In this paper we discuss the synoptic pipeline execution and describe the data being processed and produced.

引用

页数：4