SDO HMI 2014-11-23 11:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.90 | 0.00 | 15.42 | -12.78 | 226.34 | 26.59 | 240.16 | 0.5048 | 37.0 | 139.9 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.65 | -12.38 | 228.53 | 28.78 | 242.77 | 0.5310 | 653.0 | 564.2 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -12.14 | 228.50 | 28.75 | 243.17 | 0.5291 | 652.0 | 493.1 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -13.06 | 228.54 | 28.79 | 241.64 | 0.5354 | 581.0 | 496.3 | |
| 0.00 | 4.71 | 0.00 | 2.75 | -12.96 | 228.29 | 28.54 | 241.60 | 0.5314 | 453.0 | 519.8 | |
| 0.00 | 5.14 | 0.00 | 2.99 | -12.80 | 228.03 | 28.28 | 241.66 | 0.5270 | 599.0 | 739.2 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -13.11 | 227.93 | 28.18 | 241.06 | 0.5277 | 695.0 | 555.8 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -13.87 | 227.85 | 28.10 | 239.70 | 0.5318 | 506.0 | 454.5 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -12.81 | 226.62 | 26.87 | 240.47 | 0.5086 | 780.0 | 623.9 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -11.88 | 223.97 | 24.22 | 239.70 | 0.4669 | -271.0 | -341.6 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -14.24 | 223.91 | 24.16 | 235.33 | 0.4844 | -696.0 | -479.4 | |
| 0.00 | 4.03 | 0.00 | 2.24 | -11.51 | 223.47 | 23.72 | 239.92 | 0.4575 | -723.0 | -645.6 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -11.85 | 223.40 | 23.65 | 239.20 | 0.4591 | -935.0 | -788.7 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -13.22 | 223.27 | 23.52 | 236.48 | 0.4679 | -685.0 | -579.8 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -13.53 | 223.27 | 23.52 | 235.92 | 0.4704 | -584.0 | -533.3 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -15.81 | 223.29 | 23.54 | 231.96 | 0.4900 | -470.0 | -505.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |