SDO HMI 2014-09-07 09:01:21 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.31 | 67.48 | 22.92 | 134.91 | -16.48 | 64.08 | -72.52 | 109.17 | 0.9687 | 180.4 | -44.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.05 | 0.00 | 3.57 | -16.90 | 66.38 | -70.23 | 110.09 | 0.9599 | 571.0 | 508.5 | |
| 4.64 | 37.23 | 8.29 | 67.87 | -16.90 | 65.90 | -70.70 | 109.97 | 0.9621 | 426.4 | 15.6 | |
| 3.39 | -2.00 | 6.04 | -2.00 | -16.48 | 65.88 | -70.72 | 109.54 | 0.9617 | 544.9 | 999999 | |
| 3.39 | -2.00 | 6.25 | -2.00 | -16.68 | 65.31 | -71.29 | 109.62 | 0.9644 | -16.1 | 999999 | |
| 0.00 | 8.04 | 0.00 | 14.83 | -16.11 | 65.22 | -71.38 | 109.02 | 0.9643 | -104.0 | -70.7 | |
| 0.00 | 1.07 | 0.00 | 2.06 | -16.73 | 64.66 | -71.94 | 109.53 | 0.9672 | -124.0 | -140.8 | |
| 0.00 | 2.32 | 0.00 | 4.65 | -17.01 | 63.96 | -72.64 | 109.66 | 0.9703 | 21.0 | -51.7 | |
| 0.00 | 0.98 | 0.00 | 2.09 | -16.73 | 63.03 | -73.58 | 109.19 | 0.9737 | -250.0 | -142.8 | |
| 0.00 | 0.27 | 0.00 | 0.54 | -15.88 | 63.65 | -72.95 | 108.47 | 0.9706 | 175.0 | 77.0 | |
| 0.00 | 0.71 | 0.00 | 1.54 | -16.50 | 62.81 | -73.79 | 108.92 | 0.9743 | -348.0 | -337.6 | |
| 0.00 | 0.80 | 0.00 | 2.00 | -16.70 | 61.02 | -75.59 | 108.76 | 0.9806 | -329.0 | -307.7 | |
| 0.00 | 5.71 | 0.00 | 13.79 | -16.06 | 61.25 | -75.35 | 108.16 | 0.9794 | -566.0 | -459.4 | |
| 0.89 | 2.41 | 2.34 | 6.31 | -16.30 | 60.30 | -76.30 | 108.23 | 0.9826 | 9.9 | 43.5 | |
| 0.00 | 5.89 | 0.00 | 15.66 | -15.95 | 60.05 | -76.55 | 107.83 | 0.9832 | 145.0 | 99.1 | |
| 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. | |