SDO HMI 2014-09-07 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.69 | 75.95 | 30.89 | 65.79 | -9.36 | 194.30 | 52.75 | 253.21 | 0.8221 | -17.0 | 217.3 | |
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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 | 1.16 | 0.00 | 1.06 | -9.08 | 196.47 | 54.92 | 254.22 | 0.8418 | 143.0 | 139.5 | |
| 12.49 | 34.00 | 11.38 | 30.68 | -9.53 | 196.25 | 54.70 | 253.64 | 0.8410 | 386.9 | 498.4 | |
| 5.35 | -2.00 | 4.80 | -2.00 | -9.29 | 195.77 | 54.22 | 253.77 | 0.8360 | 692.7 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.48 | -8.66 | 195.47 | 53.93 | 254.41 | 0.8317 | 571.0 | 548.3 | |
| 0.00 | 0.98 | 0.00 | 0.87 | -8.88 | 195.47 | 53.92 | 254.15 | 0.8322 | 612.0 | 517.7 | |
| 0.00 | 0.89 | 0.00 | 0.79 | -9.33 | 194.94 | 53.40 | 253.47 | 0.8285 | 255.0 | 266.5 | |
| 0.00 | 2.50 | 0.00 | 2.20 | -9.47 | 194.82 | 53.27 | 253.26 | 0.8277 | 279.0 | 349.1 | |
| 0.00 | 0.98 | 0.00 | 0.84 | -8.36 | 194.03 | 52.48 | 254.32 | 0.8173 | -255.0 | -156.5 | |
| 0.00 | 1.52 | 0.00 | 1.30 | -9.05 | 193.76 | 52.22 | 253.42 | 0.8166 | 232.0 | 225.5 | |
| 0.00 | 1.07 | 0.00 | 0.90 | -9.11 | 193.12 | 51.58 | 253.13 | 0.8106 | -196.0 | -157.0 | |
| 17.85 | 30.79 | 14.71 | 25.44 | -9.38 | 192.10 | 50.56 | 252.46 | 0.8013 | -643.1 | -88.6 | |
| 0.00 | 1.52 | 0.00 | 1.23 | -8.24 | 191.65 | 50.10 | 253.68 | 0.7934 | -589.0 | -446.5 | |
| 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. | |