SDO HMI 2014-05-30 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.36 | 173.97 | 13.19 | 87.16 | -9.12 | 24.83 | 0.56 | 184.37 | 0.1479 | 769.2 | 443.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.72 | 144.90 | 0.36 | 72.54 | -8.94 | 25.97 | 1.70 | 191.87 | 0.1428 | 1044.9 | 469.8 | |
| 25.64 | -1.00 | 12.83 | -1.00 | -9.06 | 25.54 | 1.27 | 188.79 | 0.1436 | 1276.6 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.36 | -8.11 | 23.76 | -0.51 | 175.92 | 0.1257 | 767.0 | 592.9 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -10.07 | 23.63 | -0.64 | 176.01 | 0.1598 | 748.0 | 619.0 | |
| 0.00 | 2.71 | 0.00 | 1.36 | -8.96 | 23.51 | -0.76 | 174.62 | 0.1409 | 782.0 | 704.3 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -9.39 | 23.23 | -1.04 | 173.04 | 0.1488 | 1061.0 | 860.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -9.73 | 23.17 | -1.10 | 172.91 | 0.1547 | 1109.0 | 882.2 | |
| 0.00 | 8.03 | 0.00 | 4.03 | -10.07 | 23.07 | -1.20 | 172.60 | 0.1607 | 845.0 | 633.8 | |
| 0.00 | 1.81 | 0.00 | 0.90 | -9.55 | 23.05 | -1.23 | 171.97 | 0.1518 | 1087.0 | 856.8 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -9.82 | 22.95 | -1.32 | 171.63 | 0.1568 | 979.0 | 746.1 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -14.18 | 20.01 | -4.27 | 162.53 | 0.2413 | 746.0 | 549.5 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -9.05 | 20.03 | -4.24 | 152.63 | 0.1596 | -899.0 | -744.5 | |
| 0.00 | 1.81 | 0.00 | 0.90 | -8.19 | 19.64 | -4.63 | 147.66 | 0.1501 | -903.0 | -727.7 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -8.25 | 19.33 | -4.94 | 146.20 | 0.1539 | -873.0 | -764.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -2.27 | 15.41 | -8.87 | 98.61 | 0.1565 | 872.0 | 696.7 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -11.86 | 13.00 | -11.28 | 134.76 | 0.2707 | -896.0 | -725.6 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -4.86 | 10.81 | -13.47 | 106.52 | 0.2431 | -771.0 | -541.9 | |
| 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. | |