SDO HMI 2014-09-29 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 |
| 1.33 | 36.62 | 0.66 | 18.13 | 7.87 | 207.52 | -1.94 | 108.36 | 0.0425 | 31.7 | 255.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.52 | 7.35 | 210.69 | 1.23 | 293.54 | 0.0233 | -1016.0 | -792.2 | |
| 0.00 | 1.76 | 0.00 | 0.87 | 7.53 | 210.15 | 0.68 | 316.43 | 0.0172 | -901.0 | -692.0 | |
| 0.00 | 1.24 | 0.00 | 0.61 | 7.71 | 210.09 | 0.62 | 325.33 | 0.0190 | -965.0 | -756.1 | |
| 0.00 | 1.76 | 0.00 | 0.87 | 7.41 | 209.57 | 0.11 | 349.89 | 0.0105 | -1185.0 | -901.5 | |
| 0.00 | 4.06 | 0.00 | 2.01 | 7.17 | 208.03 | -1.44 | 76.10 | 0.0258 | -1178.0 | -957.8 | |
| 0.00 | 1.24 | 0.00 | 0.61 | 6.45 | 207.97 | -1.50 | 103.88 | 0.0269 | -703.0 | -476.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 5.97 | 207.94 | -1.53 | 119.19 | 0.0305 | 829.0 | 689.8 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 7.05 | 207.82 | -1.65 | 81.89 | 0.0290 | -864.0 | -715.0 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 8.73 | 207.12 | -2.35 | 50.52 | 0.0528 | 825.0 | 695.2 | |
| 0.62 | 7.85 | 0.31 | 3.89 | 7.95 | 206.94 | -2.53 | 65.63 | 0.0482 | 1018.3 | 686.9 | |
| 0.00 | 3.09 | 0.00 | 1.53 | 8.64 | 206.84 | -2.63 | 54.88 | 0.0556 | 866.0 | 730.4 | |
| 0.00 | 5.91 | 0.00 | 2.93 | 8.19 | 206.63 | -2.84 | 63.89 | 0.0548 | 988.0 | 1004.8 | |
| 0.71 | 4.68 | 0.35 | 2.32 | 8.70 | 206.54 | -2.93 | 56.92 | 0.0606 | 1125.6 | 916.9 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 7.65 | 206.48 | -2.98 | 74.23 | 0.0539 | 915.0 | 807.3 | |
| 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. | |