SDO HMI 2014-11-01 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.31 | 100.57 | 24.32 | 75.86 | -4.48 | 84.31 | -48.21 | 99.82 | 0.7567 | 485.6 | 399.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.63 | -4.75 | 86.51 | -46.00 | 100.68 | 0.7319 | 494.0 | 421.4 | |
| 1.65 | 3.38 | 1.21 | 2.48 | -5.54 | 85.83 | -46.69 | 101.57 | 0.7416 | -733.3 | -569.3 | |
| 0.00 | 1.04 | 0.00 | 0.77 | -5.01 | 85.57 | -46.94 | 100.80 | 0.7434 | -543.0 | -478.0 | |
| 3.46 | 18.02 | 2.58 | 13.51 | -5.37 | 85.10 | -47.42 | 101.16 | 0.7496 | -571.4 | 250.8 | |
| 0.00 | 1.21 | 0.00 | 0.91 | -5.74 | 84.92 | -47.60 | 101.60 | 0.7524 | 756.0 | 611.3 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -4.96 | 84.78 | -47.74 | 100.55 | 0.7523 | 303.0 | 281.7 | |
| 3.81 | -4.00 | 2.87 | -4.00 | -5.54 | 84.63 | -47.89 | 101.27 | 0.7552 | 641.5 | 999999 | |
| 1.65 | 70.42 | 1.24 | 53.14 | -4.71 | 84.45 | -48.07 | 100.14 | 0.7556 | 807.6 | 509.2 | |
| 10.65 | -8.00 | 8.01 | -8.00 | -4.32 | 84.44 | -48.08 | 99.63 | 0.7549 | 1029.6 | 999999 | |
| 3.29 | -8.00 | 2.49 | -8.00 | -4.07 | 84.14 | -48.37 | 99.23 | 0.7577 | 809.6 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.72 | -2.93 | 84.04 | -48.47 | 97.72 | 0.7568 | 636.0 | 501.7 | |
| 0.00 | 1.21 | 0.00 | 0.93 | -5.02 | 83.83 | -48.69 | 100.40 | 0.7631 | 552.0 | 364.4 | |
| 7.80 | -8.00 | 5.92 | -8.00 | -3.81 | 83.85 | -48.67 | 98.84 | 0.7606 | 626.9 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -4.36 | 83.71 | -48.81 | 99.52 | 0.7631 | 169.0 | 182.0 | |
| 0.00 | 0.87 | 0.00 | 0.66 | -3.90 | 83.43 | -49.09 | 98.86 | 0.7654 | -206.0 | -160.8 | |
| 0.00 | 1.13 | 0.00 | 0.90 | -5.27 | 81.57 | -50.95 | 100.22 | 0.7881 | 587.0 | 512.0 | |
| 0.00 | 0.95 | 0.00 | 0.82 | -5.61 | 78.51 | -54.01 | 100.00 | 0.8198 | -537.0 | -477.5 | |
| 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. | |