B
Bruce W. Lites
Researcher at National Center for Atmospheric Research
Publications - 262
Citations - 19894
Bruce W. Lites is an academic researcher from National Center for Atmospheric Research. The author has contributed to research in topics: Sunspot & Photosphere. The author has an hindex of 74, co-authored 262 publications receiving 19051 citations. Previous affiliations of Bruce W. Lites include Association of Universities for Research in Astronomy & University of Colorado Boulder.
Papers
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Journal ArticleDOI
The polarization properties of Fe II 614.9 nm
TL;DR: The anomalous splitting of the Fe II line at 614.9 nm in the presence of magnetic fields has been studied in this paper, showing that it exhibits a depolarizing self-absorption.
Journal ArticleDOI
Emergence of a Helical Flux Rope Under an Active Region Prominence
Takenori J. Okamoto,Takenori J. Okamoto,Saku Tsuneta,Bruce W. Lites,Masahito Kubo,Takaaki Yokoyama,Thomas E. Berger,Kiyoshi Ichimoto,Yukio Katsukawa,Shin’ichi Nagata,Kazunari Shibata,Toshifumi Shimizu,Richard A. Shine,Y. Suematsu,Theodore D. Tarbell,Alan M. Title +15 more
TL;DR: In this article, a prominence was located over the polarity inversion line (PIL) in the south-east of the main sunspot, and continuous observations were obtained with a time series of vector magnetic fields on the photosphere under the prominence.
Journal ArticleDOI
Unresolved Mixed Polarity Magnetic Fields at Flux Cancellation Site in Solar Photosphere at 0".3 Spatial Resolution
TL;DR: In this article, anomalous circular polarization (Stokes V) profiles are observed in the photosphere along the polarity inversion line (PIL) at the cancellation sites.
Proceedings ArticleDOI
Pattern recognition techniques and the measurement of solar magnetic fields
TL;DR: The latest achievements of FATIMA and DIANNE are presented, two powerful examples of how pattern recognition techniques can revolutionize data analysis in astronomy.
Journal Article
Very high spatial resolution two-dimensional solar spectroscopy with video CCDs
TL;DR: In this paper, a method for recording and reducing spectra of solar fine structure with complete coverage of two-dimensional areas at very high spatial resolution and with a minimum of seeing-induced distortions is presented.