SDO HMI 2014-10-14 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.37 | 462.90 | 41.43 | 261.46 | -20.95 | 17.29 | 10.11 | 200.01 | 0.4816 | 885.7 | 342.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.54 | -18.07 | 20.06 | 12.88 | 207.69 | 0.4581 | 617.0 | 468.7 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -18.39 | 19.99 | 12.81 | 207.21 | 0.4621 | 685.0 | 567.2 | |
| 0.00 | 1.66 | 0.00 | 0.92 | -18.00 | 19.83 | 12.65 | 207.34 | 0.4555 | 776.0 | 676.2 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -19.28 | 19.80 | 12.62 | 205.97 | 0.4728 | 660.0 | 566.1 | |
| 0.00 | 2.27 | 0.00 | 1.26 | -18.41 | 17.93 | 10.75 | 203.34 | 0.4486 | -847.0 | -665.5 | |
| 30.87 | 445.95 | 17.47 | 251.92 | -21.06 | 17.72 | 10.54 | 200.69 | 0.4851 | 1184.8 | 365.2 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -18.40 | 17.35 | 10.17 | 202.22 | 0.4450 | -510.0 | -322.4 | |
| 0.35 | 0.52 | 0.19 | 0.29 | -19.25 | 17.18 | 10.00 | 201.15 | 0.4563 | 924.0 | 803.0 | |
| 42.15 | -6.00 | 23.77 | -6.00 | -20.91 | 17.09 | 9.91 | 199.66 | 0.4797 | 1317.6 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.67 | -17.92 | 16.18 | 9.00 | 200.27 | 0.4313 | -815.0 | -665.6 | |
| 0.00 | 1.40 | 0.00 | 0.77 | -17.91 | 15.99 | 8.81 | 199.88 | 0.4302 | -856.0 | -671.1 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -18.24 | 15.87 | 8.70 | 199.38 | 0.4344 | -632.0 | -487.2 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -23.22 | 15.21 | 8.03 | 194.80 | 0.5046 | 665.0 | 525.7 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -18.81 | 14.98 | 7.80 | 197.10 | 0.4386 | -702.0 | -619.8 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -21.81 | 14.32 | 7.14 | 193.95 | 0.4805 | -752.0 | -508.5 | |
| 0.00 | 1.57 | 0.00 | 0.94 | -28.39 | 5.10 | -2.08 | 176.75 | 0.5667 | -745.0 | -559.0 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -28.03 | 4.25 | -2.92 | 175.39 | 0.5623 | -679.0 | -431.5 | |
| 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. | |