SDO HMI 2014-03-15 23:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.85 | 127.91 | 47.28 | 269.65 | 11.18 | 9.94 | 74.47 | 283.40 | 0.9722 | 10.1 | -59.0 | |
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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 |
| 6.34 | 30.07 | 16.26 | 77.81 | 11.85 | 12.41 | 76.94 | 283.64 | 0.9819 | -101.6 | -19.6 | |
| 0.00 | 1.30 | 0.00 | 2.95 | 11.00 | 11.03 | 75.56 | 283.02 | 0.9767 | -490.0 | -469.7 | |
| 1.13 | 13.03 | 2.55 | 29.67 | 11.51 | 10.94 | 75.47 | 283.55 | 0.9767 | -365.5 | -315.2 | |
| 0.00 | 1.30 | 0.00 | 3.14 | 12.36 | 11.54 | 76.08 | 284.30 | 0.9794 | -194.0 | -140.3 | |
| 0.00 | 6.60 | 0.00 | 14.16 | 11.33 | 10.19 | 74.73 | 283.50 | 0.9738 | -459.0 | -485.2 | |
| 0.00 | 0.70 | 0.00 | 1.43 | 10.65 | 9.71 | 74.24 | 282.90 | 0.9714 | -173.0 | -202.1 | |
| 0.00 | 2.61 | 0.00 | 5.20 | 10.26 | 9.34 | 73.87 | 282.58 | 0.9696 | -198.0 | -203.9 | |
| 0.00 | 0.87 | 0.00 | 1.74 | 10.52 | 9.39 | 73.93 | 282.82 | 0.9700 | -200.0 | -186.0 | |
| 0.00 | 1.13 | 0.00 | 2.22 | 10.73 | 9.09 | 73.62 | 283.09 | 0.9690 | -307.0 | -282.5 | |
| 5.74 | 64.74 | 10.60 | 120.97 | 10.34 | 8.21 | 72.74 | 282.86 | 0.9648 | 481.8 | 100.5 | |
| 3.82 | -10.00 | 7.21 | -10.00 | 10.83 | 8.41 | 72.94 | 283.32 | 0.9661 | -48.2 | 999999 | |
| 2.09 | -10.00 | 4.00 | -10.00 | 11.13 | 8.60 | 73.14 | 283.59 | 0.9672 | -439.0 | 999999 | |
| 0.00 | 2.43 | 0.00 | 4.80 | 11.64 | 8.95 | 73.49 | 284.04 | 0.9691 | -492.0 | -491.8 | |
| 2.17 | -10.00 | 3.88 | -10.00 | 10.76 | 7.54 | 72.07 | 283.41 | 0.9622 | 488.2 | 999999 | |
| 1.56 | 3.13 | 2.78 | 5.56 | 11.47 | 7.28 | 71.81 | 284.19 | 0.9616 | 272.6 | 154.7 | |
| 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. | |