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Science 7 December 2007:
Vol. 318. no. 5856, pp. 1585 - 1588
DOI: 10.1126/science.1147292


Continuous Plasma Outflows from the Edge of a Solar Active Region as a Possible Source of Solar Wind
Taro Sakao, Ryouhei Kano, Noriyuki Narukage, Jun'ichi Kotoku, Takamasa Bando, Edward E. DeLuca, Loraine L. Lundquist, Saku Tsuneta, Louise K. Harra, Yukio Katsukawa, Masahito Kubo, Hirohisa Hara, Keiichi Matsuzaki, Masumi Shimojo, Jay A. Bookbinder, Leon Golub, Kelly E. Korreck, Yingna Su, Kiyoto Shibasaki, Toshifumi Shimizu, Ichiro Nakatani

Supporting Online Material

This supplement contains:
Movie S1

Movie S1
A series of CCD images taken with the Hinode XRT of the active region, with the Ti/Poly filter at a constant exposure duration of 16 seconds and at an exposure cadence of 100 seconds. Image jitter has been corrected using Sun-sensor data from the spacecraft. The movie has a spatial scale of 371 Mm square, with 512 512 pixels (the pixel size is 725 km square on the Sun). The movie covers a period of nearly 6 hours, ranging from 12:36 UT to 18:17 UT on 22 February 2007.

To view these movies, download a QuickTime viewer.





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Science. ISSN 0036-8075 (print), 1095-9203 (online)