SDO HMI 2014-10-10 04:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.44 | 0.00 | 11.61 | -20.34 | 75.04 | 11.26 | 202.44 | 0.4890 | 447.1 | 388.9 | |
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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 | 2.19 | 0.00 | 1.28 | -21.51 | 80.67 | 16.90 | 210.39 | 0.5365 | 745.0 | 577.5 | |
| 0.00 | 2.19 | 0.00 | 1.25 | -19.32 | 79.30 | 15.53 | 210.58 | 0.4985 | 706.0 | 543.9 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -21.40 | 79.52 | 15.74 | 208.78 | 0.5268 | 642.0 | 542.0 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -22.42 | 79.57 | 15.79 | 207.88 | 0.5401 | 669.0 | 559.7 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -19.12 | 79.22 | 15.44 | 210.67 | 0.4953 | 832.0 | 666.8 | |
| 0.00 | 1.67 | 0.00 | 0.92 | -17.36 | 76.41 | 12.63 | 207.70 | 0.4509 | 624.0 | 603.9 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -16.52 | 75.46 | 11.68 | 206.79 | 0.4325 | 543.0 | 407.6 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -16.91 | 75.32 | 11.55 | 206.11 | 0.4370 | 740.0 | 594.1 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -18.83 | 74.71 | 10.93 | 203.06 | 0.4601 | 825.0 | 613.8 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -17.97 | 74.65 | 10.87 | 203.74 | 0.4476 | 822.0 | 601.9 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -18.98 | 74.01 | 10.23 | 201.60 | 0.4581 | 765.0 | 666.9 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -23.69 | 72.91 | 9.14 | 196.30 | 0.5203 | 665.0 | 591.2 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -15.49 | 68.58 | 4.80 | 192.32 | 0.3800 | 712.0 | 576.2 | |
| 0.00 | 1.58 | 0.00 | 0.91 | -23.82 | 67.81 | 4.04 | 187.33 | 0.5066 | -614.0 | -497.3 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -23.71 | 67.48 | 3.70 | 186.76 | 0.5044 | -715.0 | -568.7 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -28.74 | 63.26 | -0.51 | 179.22 | 0.5753 | -807.0 | -692.2 | |
| 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. | |