SDO HMI 2014-05-15 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.76 | 63.52 | 11.45 | 35.15 | 8.24 | 195.25 | -24.16 | 65.39 | 0.4470 | -107.5 | 75.5 | |
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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 | 1.35 | 0.00 | 0.74 | 8.40 | 197.01 | -22.41 | 63.47 | 0.4233 | -844.0 | -676.9 | |
| 0.36 | 28.56 | 0.20 | 15.60 | 7.75 | 197.01 | -22.40 | 64.87 | 0.4189 | -1132.2 | -675.2 | |
| 9.79 | -2.00 | 5.34 | -2.00 | 8.03 | 196.96 | -22.45 | 64.31 | 0.4214 | -1127.1 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.22 | 7.48 | 196.96 | -22.45 | 65.52 | 0.4178 | -863.0 | -775.9 | |
| 2.07 | -2.00 | 1.13 | -2.00 | 7.76 | 196.78 | -22.64 | 65.08 | 0.4223 | -896.3 | 999999 | |
| 0.99 | -2.00 | 0.54 | -2.00 | 8.04 | 196.70 | -22.72 | 64.56 | 0.4252 | -736.5 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 8.48 | 196.24 | -23.18 | 64.06 | 0.4347 | -909.0 | -749.6 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 9.10 | 194.38 | -25.04 | 64.48 | 0.4649 | 779.0 | 717.6 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 9.51 | 194.18 | -25.24 | 63.86 | 0.4703 | 751.0 | 711.9 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 9.11 | 194.10 | -25.31 | 64.71 | 0.4688 | 901.0 | 723.2 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 8.92 | 194.08 | -25.33 | 65.09 | 0.4679 | 1160.0 | 968.1 | |
| 0.00 | 3.95 | 0.00 | 2.22 | 8.99 | 193.77 | -25.64 | 65.21 | 0.4727 | 991.0 | 870.2 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 8.01 | 193.61 | -25.81 | 67.29 | 0.4693 | 736.0 | 507.1 | |
| 5.57 | 20.93 | 3.13 | 11.77 | 8.32 | 193.31 | -26.10 | 66.90 | 0.4752 | 948.9 | 715.4 | |
| 1.98 | -14.00 | 1.11 | -14.00 | 8.54 | 193.16 | -26.25 | 66.59 | 0.4786 | 729.9 | 999999 | |
| 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. | |