SDO HMI 2014-09-30 03:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.33 | 0.00 | 7.50 | -18.37 | 200.96 | 4.68 | 190.83 | 0.4592 | -349.6 | -224.5 | |
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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 |
| 0.00 | 2.12 | 0.00 | 1.22 | -18.16 | 214.13 | 17.86 | 214.99 | 0.5102 | 742.0 | 642.3 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -8.56 | 211.36 | 15.09 | 224.66 | 0.3678 | -828.0 | -642.4 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -25.48 | 207.64 | 11.37 | 198.52 | 0.5627 | 612.0 | 508.5 | |
| 0.00 | 0.62 | 0.00 | 0.37 | -25.26 | 207.59 | 11.32 | 198.57 | 0.5596 | 778.0 | 607.4 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -16.34 | 202.66 | 6.39 | 195.25 | 0.4079 | -856.0 | -672.6 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -14.82 | 200.78 | 4.51 | 191.67 | 0.3771 | -742.0 | -553.6 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -18.99 | 197.03 | 0.75 | 181.64 | 0.4367 | -756.0 | -612.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -7.10 | 192.95 | -3.32 | 166.50 | 0.2475 | -807.0 | -601.5 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -13.23 | 191.48 | -4.79 | 166.63 | 0.3528 | -734.0 | -535.0 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -23.69 | 190.38 | -5.90 | 169.48 | 0.5172 | -702.0 | -600.7 | |
| 0.00 | 1.15 | 0.00 | 0.74 | -30.96 | 183.10 | -13.17 | 162.22 | 0.6423 | -553.0 | -423.5 | |
| 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. | |