SDO HMI 2014-05-26 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.62 | 0.00 | 11.25 | -19.59 | 49.87 | -16.87 | 139.51 | 0.4186 | 459.4 | 417.6 | |
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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 | 1.44 | 0.00 | 0.76 | -15.71 | 53.31 | -13.43 | 138.07 | 0.3361 | 869.0 | 646.3 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -18.96 | 52.73 | -14.01 | 142.97 | 0.3819 | 705.0 | 482.9 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -19.15 | 52.25 | -14.50 | 142.38 | 0.3890 | 829.0 | 648.8 | |
| 0.00 | 2.52 | 0.00 | 1.35 | -18.90 | 52.24 | -14.51 | 141.93 | 0.3859 | 838.0 | 594.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | -18.89 | 51.84 | -14.90 | 141.19 | 0.3899 | 771.0 | 661.2 | |
| 0.00 | 3.07 | 0.00 | 1.66 | -19.59 | 51.54 | -15.20 | 141.82 | 0.4014 | 837.0 | 671.1 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -18.96 | 51.57 | -15.18 | 140.80 | 0.3934 | 750.0 | 603.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -17.91 | 51.53 | -15.21 | 138.89 | 0.3813 | 739.0 | 520.5 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -21.55 | 50.89 | -15.85 | 143.76 | 0.4314 | 678.0 | 552.1 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -20.42 | 50.65 | -16.10 | 141.61 | 0.4202 | 775.0 | 655.9 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -20.61 | 50.56 | -16.18 | 141.77 | 0.4233 | 518.0 | 396.0 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -20.14 | 43.42 | -23.32 | 131.09 | 0.4952 | 691.0 | 526.7 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -21.68 | 42.41 | -24.33 | 132.40 | 0.5205 | -698.0 | -528.9 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -22.26 | 41.83 | -24.91 | 132.66 | 0.5321 | -722.0 | -572.7 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -22.03 | 41.73 | -25.01 | 132.21 | 0.5312 | -689.0 | -553.2 | |
| 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. | |