TY - GEN
T1 - Viewing Structure In Coronal Images
AU - Morgan, H.
AU - Habbal, Shadia Rifai
AU - Fineschi, S.
PY - 2006/10/1
Y1 - 2006/10/1
N2 - New image processing techniques, applied to white-light, pB , UV or EUV
observations, reveal the fine-scale detail of the corona whilst
accurately depicting the large-scale structure. The images produced by
the techniques give new insights into the structure of streamers, are
useful to unravel the complex topology of the solar maximum corona, and
can help make connections between coronal and solar disk features. CMEs
are seen in striking de- tail out to ˜18R . The quality of imaging
produced by missions such as Solar Orbiter have a strong influence on
the impact of that mission, and the solar remote sensing
instrumentation, in particular the EUV imager and coro- nagraph, can
maximize their scientific effectiveness by employing the new processing
techniques.
AB - New image processing techniques, applied to white-light, pB , UV or EUV
observations, reveal the fine-scale detail of the corona whilst
accurately depicting the large-scale structure. The images produced by
the techniques give new insights into the structure of streamers, are
useful to unravel the complex topology of the solar maximum corona, and
can help make connections between coronal and solar disk features. CMEs
are seen in striking de- tail out to ˜18R . The quality of imaging
produced by missions such as Solar Orbiter have a strong influence on
the impact of that mission, and the solar remote sensing
instrumentation, in particular the EUV imager and coro- nagraph, can
maximize their scientific effectiveness by employing the new processing
techniques.
UR - http://hdl.handle.net/2160/9916
M3 - Conference Proceeding (Non-Journal item)
SN - 92-9291-205-2
SP - 15
BT - Proceedings of The Second Solar Orbiter Workshop
ER -