SDO HMI 2014-04-12 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.45 | 0.00 | 12.27 | -20.10 | 323.77 | 24.99 | 234.07 | 0.4932 | 134.9 | 50.9 | |
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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 | 1.15 | 0.00 | 0.70 | -15.67 | 333.45 | 34.67 | 251.08 | 0.5812 | 397.0 | 359.2 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -15.71 | 332.74 | 33.96 | 250.76 | 0.5718 | 667.0 | 570.6 | |
| 0.00 | 1.77 | 0.00 | 1.07 | -16.87 | 332.89 | 34.11 | 248.85 | 0.5777 | 583.0 | 429.7 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -17.19 | 332.69 | 33.91 | 248.23 | 0.5761 | 562.0 | 513.8 | |
| 0.00 | 2.12 | 0.00 | 1.26 | -17.06 | 331.04 | 32.27 | 247.71 | 0.5538 | 747.0 | 527.5 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -18.59 | 330.61 | 31.83 | 244.83 | 0.5545 | 625.0 | 547.8 | |
| 0.00 | 1.15 | 0.00 | 0.68 | -19.69 | 329.83 | 31.06 | 242.51 | 0.5496 | 290.0 | 278.8 | |
| 0.00 | 1.24 | 0.00 | 0.72 | -16.61 | 328.94 | 30.17 | 247.48 | 0.5234 | 737.0 | 607.6 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -20.12 | 326.57 | 27.80 | 239.56 | 0.5100 | 543.0 | 423.0 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -18.87 | 325.34 | 26.57 | 240.93 | 0.4862 | 739.0 | 630.8 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -23.85 | 317.64 | 18.86 | 223.30 | 0.4329 | -620.0 | -524.3 | |
| 0.00 | 3.35 | 0.00 | 1.81 | -22.07 | 316.05 | 17.28 | 224.18 | 0.3966 | -807.0 | -750.3 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -24.15 | 315.95 | 17.17 | 220.28 | 0.4185 | -926.0 | -822.4 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -24.31 | 315.90 | 17.13 | 219.94 | 0.4198 | -817.0 | -662.1 | |
| 0.00 | 2.38 | 0.00 | 1.27 | -27.54 | 303.41 | 4.64 | 190.98 | 0.3780 | -697.0 | -405.0 | |
| 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. | |