SDO HMI 2014-07-22 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.12 | 155.35 | 21.41 | 97.85 | -21.00 | 69.02 | 28.40 | 226.00 | 0.6194 | 465.5 | 264.4 | |
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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 |
| 25.04 | 122.22 | 15.85 | 77.43 | -20.92 | 69.69 | 29.07 | 226.78 | 0.6251 | 1024.3 | 304.3 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -20.19 | 68.58 | 27.96 | 226.62 | 0.6076 | 829.0 | 692.9 | |
| 2.00 | 11.52 | 1.25 | 7.20 | -21.09 | 68.35 | 27.73 | 225.26 | 0.6134 | 694.3 | 643.1 | |
| 0.00 | 1.36 | 0.00 | 0.85 | -20.48 | 68.12 | 27.50 | 225.80 | 0.6056 | 791.0 | 681.9 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -19.59 | 67.80 | 27.18 | 226.62 | 0.5944 | 630.0 | 404.4 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -19.99 | 67.69 | 27.08 | 225.99 | 0.5969 | 601.0 | 489.5 | |
| 1.00 | 2.45 | 0.61 | 1.50 | -21.28 | 65.43 | 24.81 | 221.96 | 0.5870 | -821.1 | -623.1 | |
| 0.00 | 1.09 | 0.00 | 0.68 | -22.99 | 65.61 | 24.99 | 220.12 | 0.6057 | -448.0 | -321.2 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -21.88 | 65.18 | 24.56 | 220.95 | 0.5907 | -560.0 | -498.5 | |
| 0.00 | 2.00 | 0.00 | 1.22 | -21.64 | 65.10 | 24.48 | 221.15 | 0.5875 | -839.0 | -712.9 | |
| 5.17 | 7.44 | 3.15 | 4.54 | -21.69 | 64.78 | 24.16 | 220.72 | 0.5852 | -893.2 | -722.6 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -20.87 | 64.64 | 24.02 | 221.56 | 0.5755 | -672.0 | -627.4 | |
| 0.91 | 2.54 | 0.55 | 1.54 | -22.10 | 63.85 | 23.23 | 219.16 | 0.5809 | -782.8 | -630.4 | |
| 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. | |