SDO HMI 2014-10-05 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.54 | 311.13 | 35.26 | 184.77 | -1.42 | 155.10 | 32.49 | 257.41 | 0.5522 | 924.6 | 355.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.20 | 274.61 | 22.75 | 163.54 | -1.47 | 155.44 | 32.82 | 257.47 | 0.5572 | 1270.5 | 358.8 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 1.61 | 154.94 | 32.33 | 262.79 | 0.5410 | 524.0 | 364.2 | |
| 0.26 | -1.00 | 0.16 | -1.00 | -1.37 | 154.83 | 32.22 | 257.37 | 0.5483 | 1296.0 | 999999 | |
| 4.48 | -1.00 | 2.65 | -1.00 | -1.52 | 154.69 | 32.08 | 257.05 | 0.5468 | 1150.4 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.72 | 0.34 | 153.98 | 31.36 | 260.12 | 0.5303 | 419.0 | 390.9 | |
| 11.33 | 14.75 | 6.64 | 8.65 | -1.81 | 153.95 | 31.34 | 256.19 | 0.5374 | 939.9 | 637.9 | |
| 5.27 | 11.59 | 3.06 | 6.74 | -0.36 | 153.48 | 30.87 | 258.63 | 0.5254 | 992.6 | 765.1 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -1.65 | 153.36 | 30.74 | 256.18 | 0.5283 | 704.0 | 618.5 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 0.01 | 151.92 | 29.31 | 258.63 | 0.5013 | 646.0 | 611.0 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -0.79 | 151.65 | 29.03 | 256.94 | 0.5002 | -490.0 | -420.7 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -1.10 | 151.17 | 28.56 | 256.10 | 0.4944 | -602.0 | -456.6 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -0.54 | 150.93 | 28.31 | 257.07 | 0.4886 | -770.0 | -657.4 | |
| 0.00 | 1.58 | 0.00 | 0.90 | -1.54 | 150.90 | 28.29 | 255.09 | 0.4922 | -723.0 | -588.4 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -1.64 | 148.38 | 25.76 | 253.31 | 0.4555 | -597.0 | -483.6 | |
| 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. | |