SDO HMI 2014-04-22 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.50 | 0.00 | 9.06 | -20.43 | 161.76 | 4.93 | 196.27 | 0.2821 | -770.9 | -633.7 | |
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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 | 1.07 | 0.00 | 0.56 | -20.27 | 168.09 | 11.26 | 214.63 | 0.3237 | -712.0 | -547.8 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -23.62 | 167.35 | 10.52 | 207.54 | 0.3635 | -680.0 | -576.2 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -28.25 | 166.25 | 9.42 | 199.99 | 0.4233 | -682.0 | -507.6 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -30.99 | 165.01 | 8.18 | 195.52 | 0.4578 | -764.0 | -627.7 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -16.46 | 162.07 | 5.24 | 203.71 | 0.2187 | -813.0 | -665.6 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -18.71 | 161.91 | 5.08 | 199.42 | 0.2532 | -912.0 | -725.2 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -19.33 | 161.86 | 5.03 | 198.44 | 0.2628 | -811.0 | -659.8 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.68 | 161.84 | 5.01 | 197.94 | 0.2682 | -881.0 | -702.8 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -16.65 | 161.54 | 4.71 | 201.22 | 0.2182 | -599.0 | -680.7 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -19.87 | 161.56 | 4.73 | 196.77 | 0.2698 | -744.0 | -572.5 | |
| 0.00 | 0.89 | 0.00 | 0.47 | -24.25 | 160.48 | 3.64 | 189.95 | 0.3367 | -631.0 | -423.7 | |
| 0.00 | 3.37 | 0.00 | 1.72 | -17.70 | 159.91 | 3.08 | 193.10 | 0.2272 | -906.0 | -722.3 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -18.54 | 159.71 | 2.87 | 191.46 | 0.2403 | -876.0 | -733.1 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -20.22 | 155.37 | -1.46 | 174.79 | 0.2651 | -782.0 | -507.0 | |
| 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. | |