TY - GEN
T1 - TimeTubes
T2 - 15th NICOGRAPH International, NicoInt 2016
AU - Xu, Longyin
AU - Nakayama, Masanori
AU - Wu, Hsiang Yun
AU - Watanabe, Kazuho
AU - Takahashi, Shigeo
AU - Uemura, Makoto
AU - Fujishiro, Issei
N1 - Publisher Copyright:
© 2016 IEEE.
PY - 2016/9/9
Y1 - 2016/9/9
N2 - Blazars are active galactic nuclei whose relativistic jets ejected from the central black hole are pointing toward the Earth. Astronomers have attempted to classify blazars, but analyzing the time-dependent multivariate datasets with conventional visualization methods, such as scatter plot matrices, is difficult. This paper presents TimeTubes, a new visualization scheme that allows astronomers to analyze dynamic changes in and feature causality among the multiple time-varying variables. We target six representative time-varying variables from the originals, including two polarization-related parameters and their corresponding errors, intensity, and color. The four polarization parameters with a common time stamp are transformed to an ellipse, and a series of such ellipses are aligned in parallel along the time line to form a volumetric tube in 3D space. The resulting tube is then colorized by the observed intensities and colors of the blazar. We designed a designated interface with nine functions to control the view of the tube interactively. The usability of TimeTubes is discussed with feedback from astronomers.
AB - Blazars are active galactic nuclei whose relativistic jets ejected from the central black hole are pointing toward the Earth. Astronomers have attempted to classify blazars, but analyzing the time-dependent multivariate datasets with conventional visualization methods, such as scatter plot matrices, is difficult. This paper presents TimeTubes, a new visualization scheme that allows astronomers to analyze dynamic changes in and feature causality among the multiple time-varying variables. We target six representative time-varying variables from the originals, including two polarization-related parameters and their corresponding errors, intensity, and color. The four polarization parameters with a common time stamp are transformed to an ellipse, and a series of such ellipses are aligned in parallel along the time line to form a volumetric tube in 3D space. The resulting tube is then colorized by the observed intensities and colors of the blazar. We designed a designated interface with nine functions to control the view of the tube interactively. The usability of TimeTubes is discussed with feedback from astronomers.
KW - 3D information visualization
KW - Blazar
KW - Multivariate data
KW - Time-dependent data
UR - http://www.scopus.com/inward/record.url?scp=84991063678&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84991063678&partnerID=8YFLogxK
U2 - 10.1109/NicoInt.2016.3
DO - 10.1109/NicoInt.2016.3
M3 - Conference contribution
AN - SCOPUS:84991063678
T3 - Proceedings - NICOGRAPH International 2016, NicoInt 2016
SP - 15
EP - 20
BT - Proceedings - NICOGRAPH International 2016, NicoInt 2016
PB - Institute of Electrical and Electronics Engineers Inc.
Y2 - 6 July 2016 through 8 July 2016
ER -