Calculation parameters for SLIPCAT
Parameters | Units | STEREO-A | STEREO-B | STEREO-A | STEREO-B | Description (read Wang et al., ApJ, doi:10.1086/349572, 2010 for more details) |
2007/04-2009/12 | 2010/01- | |||||
δ | # | 5.0 | 5.0 | A small value used in creating rescaled images | ||
thknl | # | 2.0 | 3.2 | A threshold for kernel selection | ||
thpro | # | 1.7 | 2.2 | A threshold for region growing | ||
rmax1 | Rs | 1.51 | 1.7 | 1.51 | 1.7 | An upper boundary above which there is no selected kernel |
rmax2 | Rs | 1.54 | 1.73 | 1.54 | 1.73 | An upper boundary, The parameters of any prominences extending into the region above it is considered to be unreliable |
sn | pixels | 5 | 5 | Size of a box used to remove noise-like kernels | ||
sm | pixels | 5 | 5 | Size of a box used to merge regions which are very close to each other | ||
ssp | pixels | 20 | 20 | Size used to smooth the spine of a prominence | ||
tharea | Mm^2 | 500 | 500 | A threshold to remove very small regions | ||
thdis | hours | 2 | 2 | A threshold to judge if a prominence has disappeared | ||
LDF | 14.20, 4.70, 1.36 (Figure) | 1.20, 7.04, 0.30 (Figure) | Linear discriminant function |
Description of the parameter table of the SLIPCAT
Start | The first time detected. | |
End | The last time detected. | |
PA | Position angle of the centroid at the first time, counterclockwise from north pole. | |
HGLon | Longitude of the centroid at the first time in heliographic coordinate. Derived from the heliographic position of spacecraft and the position angle of the prominence. | |
HGLat | Latitude of the centroid at the first time in heliographic coordinate. | |
P/M | P: How many seperate parts in the prominence; M (Y or N): Is the part a major one compared to other parts. | |
Frames | Number of frames in which the prominence is detected. | |
CL | Confidence level. Number 1 has the highest liklihood to be a prominence. | |
r_cen | Heliocentric distance of the brightness centroid of the prominence. | |
PA_cen | Position angle of the brightness centroid of the prominence. | |
r_top | Heliocentric distance of the top of the prominence. | |
Area | Projected area of the prominence on the plane of the sky. | |
Length | Characteristic length of the prominence (i.e., the length of the spine of the prominence). | |
Brightness | Average brightness (i.e., digital number, DN) of the prominence. | |
Mean | Mean value of the given parameter during the detection. | |
Min | Minimum value of the given parameter during the detection. | |
Max | Maximum value of the given parameter during the detection. | |
v | Average first time derivative of the given parameter (i.e., the slope of the linear fitting line of the given parameter during the detection). | |
a | Average second time derivative of the given parameter. | |
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Clickable cell and highlight the multiple-part prominence. | |
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Highlight the prominence with CL=2. | |
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Highlight the prominence with CL=3. |
SLIPCAT is an automated system developed by the STEP Team at USTC. If you want to learn more about SLIPCAT and cite some papers in your researches related to SLIPCAT, refer to the following paper:
This project is supported by the grants from NFSC (40525014), the 973 program (2006CB806304), etc. Comments or questions should be addressed to Yuming Wang. Also, you may leave your thoughts here. |