SDO HMI 2014-05-23 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.17 | 138.72 | 24.94 | 108.99 | -10.91 | 64.85 | -50.39 | 102.68 | 0.7764 | 403.6 | 238.1 | |
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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 |
| 19.91 | 101.89 | 15.04 | 77.06 | -10.56 | 66.65 | -48.59 | 102.49 | 0.7574 | 986.4 | 343.2 | |
| 0.00 | 1.62 | 0.00 | 1.29 | -12.85 | 64.25 | -50.99 | 105.04 | 0.7867 | 440.0 | 300.7 | |
| 0.00 | 1.44 | 0.00 | 1.13 | -8.66 | 64.50 | -50.74 | 99.75 | 0.7789 | -589.0 | -467.2 | |
| 0.00 | 0.81 | 0.00 | 0.64 | -8.96 | 64.10 | -51.14 | 100.08 | 0.7834 | -500.0 | -432.8 | |
| 0.00 | 0.99 | 0.00 | 0.80 | -9.65 | 63.26 | -51.98 | 100.86 | 0.7930 | -193.0 | -250.5 | |
| 0.00 | 1.80 | 0.00 | 1.51 | -11.18 | 61.75 | -53.48 | 102.59 | 0.8100 | 668.0 | 507.5 | |
| 0.00 | 1.26 | 0.00 | 1.07 | -11.61 | 61.37 | -53.86 | 103.06 | 0.8143 | 506.0 | 359.9 | |
| 4.95 | 8.74 | 4.19 | 7.40 | -10.99 | 61.44 | -53.80 | 102.31 | 0.8130 | 697.8 | 521.6 | |
| 0.00 | 0.99 | 0.00 | 0.85 | -11.60 | 61.11 | -54.13 | 103.01 | 0.8169 | 238.0 | 241.4 | |
| 0.00 | 0.90 | 0.00 | 0.77 | -11.26 | 61.20 | -54.03 | 102.61 | 0.8156 | 483.0 | 418.4 | |
| 0.00 | 0.72 | 0.00 | 0.62 | -11.47 | 60.93 | -54.30 | 102.83 | 0.8185 | 132.0 | 201.4 | |
| 0.00 | 0.72 | 0.00 | 0.63 | -11.61 | 60.41 | -54.83 | 102.94 | 0.8237 | 202.0 | 129.2 | |
| 0.00 | 1.26 | 0.00 | 1.13 | -12.80 | 59.43 | -55.81 | 104.24 | 0.8343 | -736.0 | -613.1 | |
| 6.31 | 13.96 | 5.71 | 12.63 | -12.69 | 58.85 | -56.39 | 104.03 | 0.8396 | -553.0 | -431.8 | |
| 0.00 | 1.62 | 0.00 | 1.46 | -12.07 | 58.99 | -56.24 | 103.32 | 0.8376 | -344.0 | -362.8 | |
| 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. | |