SDO HMI 2014-05-19 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.58 | 258.83 | 23.44 | 153.21 | -24.50 | 190.71 | 25.30 | 225.42 | 0.5483 | 670.9 | 293.3 | |
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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 |
| 35.71 | 241.28 | 21.16 | 143.00 | -24.40 | 191.05 | 25.64 | 225.92 | 0.5506 | 1233.3 | 355.3 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -20.94 | 190.36 | 24.95 | 230.49 | 0.5127 | -727.0 | -576.8 | |
| 3.87 | -1.00 | 2.28 | -1.00 | -24.12 | 190.54 | 25.13 | 225.81 | 0.5427 | 1172.9 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.18 | -26.03 | 190.67 | 25.26 | 223.25 | 0.5617 | 78.0 | 80.7 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -24.26 | 189.69 | 24.28 | 224.70 | 0.5351 | 906.0 | 696.0 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -24.95 | 186.93 | 21.52 | 220.49 | 0.5141 | -678.0 | -475.3 | |
| 0.00 | 3.24 | 0.00 | 1.87 | -25.98 | 186.29 | 20.88 | 218.29 | 0.5191 | -771.0 | -598.9 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -25.96 | 185.67 | 20.26 | 217.53 | 0.5131 | -807.0 | -705.5 | |
| 0.00 | 2.43 | 0.00 | 1.41 | -26.99 | 185.53 | 20.12 | 216.01 | 0.5234 | -604.0 | -612.9 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -27.43 | 185.11 | 19.70 | 214.91 | 0.5247 | -917.0 | -765.5 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -30.91 | 185.40 | 19.99 | 211.28 | 0.5669 | -630.0 | -463.2 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -27.11 | 184.25 | 18.84 | 214.18 | 0.5137 | -815.0 | -676.1 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -26.95 | 183.61 | 18.20 | 213.51 | 0.5064 | -701.0 | -534.4 | |
| 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. | |