SDO HMI 2014-10-12 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.08 | 0.00 | 12.40 | -21.66 | 70.82 | 38.35 | 232.26 | 0.7328 | -78.2 | -172.1 | |
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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 | 1.23 | 0.00 | 0.96 | -16.38 | 78.43 | 45.96 | 243.04 | 0.7761 | 405.0 | 372.0 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -16.82 | 77.40 | 44.93 | 242.02 | 0.7678 | 507.0 | 461.4 | |
| 0.00 | 0.96 | 0.00 | 0.73 | -16.66 | 76.65 | 44.18 | 241.83 | 0.7597 | 698.0 | 644.1 | |
| 0.00 | 1.23 | 0.00 | 0.90 | -15.96 | 74.99 | 42.52 | 241.82 | 0.7395 | 537.0 | 352.6 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -19.20 | 74.18 | 41.71 | 237.43 | 0.7480 | 565.0 | 533.8 | |
| 0.00 | 1.05 | 0.00 | 0.80 | -24.50 | 72.34 | 39.87 | 230.20 | 0.7616 | 479.0 | 376.0 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -22.51 | 69.23 | 36.77 | 230.32 | 0.7208 | -590.0 | -481.6 | |
| 0.00 | 4.81 | 0.00 | 3.41 | -23.59 | 68.11 | 35.65 | 228.26 | 0.7181 | -722.0 | -647.2 | |
| 0.00 | 1.05 | 0.00 | 0.75 | -24.23 | 68.00 | 35.53 | 227.45 | 0.7217 | -321.0 | -294.5 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -23.64 | 67.77 | 35.30 | 227.95 | 0.7153 | -680.0 | -602.6 | |
| 0.00 | 2.28 | 0.00 | 1.61 | -24.06 | 67.50 | 35.03 | 227.26 | 0.7160 | -704.0 | -489.4 | |
| 0.00 | 1.05 | 0.00 | 0.74 | -23.71 | 67.31 | 34.84 | 227.52 | 0.7117 | -568.0 | -465.9 | |
| 0.00 | 0.53 | 0.00 | 0.37 | -24.27 | 67.00 | 34.54 | 226.65 | 0.7131 | -622.0 | -466.5 | |
| 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. | |