SDO HMI 2014-07-10 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.04 | 311.19 | 43.71 | 283.21 | -19.14 | 254.09 | 53.03 | 244.20 | 0.8405 | 709.6 | 244.1 | |
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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 |
| 0.00 | 3.54 | 0.00 | 3.37 | -19.55 | 255.82 | 54.77 | 244.32 | 0.8561 | -141.0 | -178.9 | |
| 0.00 | 1.27 | 0.00 | 1.29 | -22.81 | 256.97 | 55.91 | 241.11 | 0.8738 | -432.0 | -342.6 | |
| 48.04 | 291.21 | 43.71 | 265.19 | -19.06 | 254.15 | 53.09 | 244.31 | 0.8408 | 892.0 | 256.3 | |
| 0.00 | 0.91 | 0.00 | 0.83 | -20.48 | 253.64 | 52.58 | 242.52 | 0.8408 | 360.0 | 307.0 | |
| 0.00 | 1.09 | 0.00 | 0.95 | -18.64 | 252.43 | 51.37 | 244.18 | 0.8245 | 217.0 | 232.8 | |
| 0.00 | 2.63 | 0.00 | 2.30 | -18.97 | 252.47 | 51.41 | 243.81 | 0.8259 | 521.0 | 496.1 | |
| 0.00 | 1.73 | 0.00 | 1.51 | -19.46 | 252.42 | 51.36 | 243.23 | 0.8271 | 402.0 | 454.6 | |
| 0.00 | 3.81 | 0.00 | 3.44 | -21.15 | 253.00 | 51.95 | 241.53 | 0.8375 | 206.0 | 287.8 | |
| 0.00 | 1.27 | 0.00 | 1.11 | -19.67 | 252.10 | 51.04 | 242.87 | 0.8249 | 356.0 | 291.1 | |
| 0.00 | 0.64 | 0.00 | 0.57 | -21.77 | 252.25 | 51.20 | 240.54 | 0.8333 | -323.0 | -291.6 | |
| 0.00 | 0.64 | 0.00 | 0.57 | -22.00 | 252.05 | 50.99 | 240.20 | 0.8324 | 376.0 | 362.6 | |
| 0.00 | 1.00 | 0.00 | 0.85 | -20.87 | 250.39 | 49.33 | 240.81 | 0.8140 | -473.0 | -408.9 | |
| 0.00 | 1.45 | 0.00 | 1.23 | -20.89 | 250.09 | 49.04 | 240.66 | 0.8115 | -526.0 | -472.8 | |
| 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. | |