期刊
ASTRONOMY & ASTROPHYSICS
卷 390, 期 2, 页码 717-723出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20020751
关键词
Sun : helioseismology; Sun : interior; astronomical data bases : miscellaneous
The IRIS network has been operated continuously since July 1st 1989. To date, it has acquired more than a complete solar cycle of full-disk helioseismic data which has been used to constrain the structure and rotation of the deep solar interior. However, the duty cycle of the network data has never reached initial expectations. To improve this situation, several cooperations have been developed with teams collecting observations with similar instruments. This paper demonstrates that we are able to merge data from these different instruments in a consistent manner resulting in a very significant improvement in network duty cycle over more than one solar cycle initiating what we call the IRIS++ network.
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