SDO HMI 2014-05-23 07:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.38 | 69.63 | 15.17 | 38.35 | -13.67 | 136.16 | 23.12 | 241.13 | 0.4371 | 262.5 | -41.5 | |
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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 |
| 10.09 | 15.77 | 5.62 | 8.77 | -13.41 | 137.73 | 24.69 | 243.20 | 0.4571 | 961.0 | 674.5 | |
| 2.61 | 8.83 | 1.45 | 4.89 | -13.07 | 137.29 | 24.24 | 243.50 | 0.4488 | 1147.5 | 799.8 | |
| 9.64 | 15.23 | 5.36 | 8.46 | -13.94 | 137.28 | 24.24 | 241.73 | 0.4542 | 1015.2 | 537.9 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -14.32 | 137.32 | 24.28 | 241.02 | 0.4573 | 542.0 | 323.3 | |
| 0.27 | -2.00 | 0.15 | -2.00 | -13.17 | 137.09 | 24.05 | 243.13 | 0.4467 | 1111.0 | 999999 | |
| 0.90 | 2.25 | 0.50 | 1.25 | -14.41 | 136.99 | 23.94 | 240.52 | 0.4534 | 763.5 | 647.2 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -13.53 | 135.40 | 22.35 | 240.78 | 0.4254 | -854.0 | -597.2 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -14.06 | 135.21 | 22.17 | 239.48 | 0.4267 | -718.0 | -523.5 | |
| 0.00 | 2.61 | 0.00 | 1.43 | -14.19 | 134.79 | 21.74 | 238.75 | 0.4219 | -145.0 | -268.4 | |
| 0.00 | 2.16 | 0.00 | 1.18 | -13.88 | 134.25 | 21.21 | 238.81 | 0.4123 | -705.0 | -500.2 | |
| 0.45 | 1.71 | 0.24 | 0.93 | -13.48 | 134.15 | 21.10 | 239.56 | 0.4078 | -769.6 | -627.1 | |
| 0.00 | 3.60 | 0.00 | 1.95 | -13.91 | 133.95 | 20.91 | 238.40 | 0.4085 | -1003.0 | -798.2 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -14.44 | 133.87 | 20.83 | 237.17 | 0.4115 | -713.0 | -611.9 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -14.23 | 133.81 | 20.77 | 237.57 | 0.4090 | -907.0 | -740.5 | |
| 3.42 | 12.25 | 1.85 | 6.63 | -13.58 | 133.65 | 20.61 | 238.79 | 0.4018 | -1135.4 | -799.1 | |
| 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. | |