SDO HMI 2014-10-06 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.39 | 283.30 | 31.39 | 180.56 | -1.52 | 155.23 | 38.13 | 259.44 | 0.6300 | 821.4 | 320.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.45 | 253.86 | 22.02 | 162.39 | -1.56 | 155.56 | 38.46 | 259.49 | 0.6346 | 1119.3 | 329.8 | |
| 3.95 | -1.00 | 2.50 | -1.00 | -1.63 | 154.84 | 37.74 | 259.14 | 0.6252 | 1051.3 | 999999 | |
| 0.00 | 1.76 | 0.00 | 1.12 | -3.83 | 154.57 | 37.47 | 255.62 | 0.6289 | 642.0 | 439.5 | |
| 7.56 | 10.28 | 4.74 | 6.45 | -1.73 | 154.12 | 37.02 | 258.72 | 0.6159 | 917.5 | 681.3 | |
| 0.00 | 1.23 | 0.00 | 0.76 | -0.13 | 153.61 | 36.51 | 261.14 | 0.6044 | 740.0 | 586.7 | |
| 3.43 | 5.80 | 2.13 | 3.60 | -0.42 | 153.50 | 36.40 | 260.62 | 0.6037 | 898.1 | 737.5 | |
| 0.00 | 1.58 | 0.00 | 0.96 | 0.36 | 151.84 | 34.74 | 261.37 | 0.5785 | 607.0 | 370.4 | |
| 0.00 | 2.37 | 0.00 | 1.44 | -0.15 | 151.80 | 34.70 | 260.49 | 0.5794 | 808.0 | 654.3 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -0.93 | 151.62 | 34.52 | 259.12 | 0.5792 | -373.0 | -388.2 | |
| 0.00 | 2.11 | 0.00 | 1.27 | -0.66 | 151.15 | 34.05 | 259.40 | 0.5718 | -782.0 | -610.7 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -1.11 | 151.12 | 34.02 | 258.62 | 0.5727 | -742.0 | -620.9 | |
| 0.00 | 1.76 | 0.00 | 1.05 | -0.38 | 150.60 | 33.50 | 259.67 | 0.5632 | -600.0 | -569.5 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -1.66 | 148.41 | 31.31 | 256.46 | 0.5364 | -659.0 | -484.7 | |
| 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. | |