SDO HMI 2014-12-07 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.98 | 545.85 | 126.47 | 810.39 | -19.57 | 85.52 | 69.19 | 249.13 | 0.9438 | 457.5 | 201.8 | |
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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 |
| 27.13 | 532.53 | 43.81 | 793.53 | -18.81 | 87.39 | 71.06 | 250.16 | 0.9532 | 300.6 | 201.2 | |
| 19.54 | -1.00 | 29.05 | -1.00 | -19.18 | 85.60 | 69.27 | 249.57 | 0.9441 | 530.6 | 999999 | |
| 1.62 | -1.00 | 2.31 | -1.00 | -19.78 | 84.57 | 68.24 | 248.80 | 0.9389 | 228.8 | 999999 | |
| 0.00 | 1.19 | 0.00 | 1.55 | -17.77 | 82.68 | 66.35 | 250.68 | 0.9260 | -324.0 | -214.1 | |
| 0.00 | 0.77 | 0.00 | 1.02 | -18.46 | 83.20 | 66.87 | 250.02 | 0.9298 | 513.0 | 408.1 | |
| 0.00 | 1.37 | 0.00 | 1.78 | -18.61 | 82.69 | 66.36 | 249.78 | 0.9268 | 487.0 | 424.1 | |
| 36.69 | -1.00 | 51.30 | -1.00 | -20.41 | 84.12 | 67.79 | 248.08 | 0.9369 | 633.1 | 999999 | |
| 0.00 | 2.22 | 0.00 | 2.89 | -18.83 | 82.62 | 66.29 | 249.54 | 0.9266 | 551.0 | 386.5 | |
| 0.00 | 1.11 | 0.00 | 1.40 | -20.97 | 81.42 | 65.08 | 247.06 | 0.9213 | 380.0 | 359.8 | |
| 0.00 | 4.10 | 0.00 | 5.38 | -21.96 | 82.28 | 65.94 | 246.15 | 0.9276 | 562.0 | 351.0 | |
| 0.00 | 0.26 | 0.00 | 0.31 | -19.57 | 80.33 | 63.99 | 248.38 | 0.9127 | -302.0 | -261.0 | |
| 0.00 | 1.19 | 0.00 | 1.46 | -21.19 | 80.55 | 64.21 | 246.67 | 0.9160 | -124.0 | -41.1 | |
| 0.00 | 0.26 | 0.00 | 0.28 | -21.11 | 77.49 | 61.16 | 246.17 | 0.8952 | -330.0 | -287.0 | |
| 0.00 | 0.85 | 0.00 | 0.79 | -18.61 | 71.97 | 55.63 | 247.76 | 0.8473 | -568.0 | -484.8 | |
| 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. | |