SDO HMI 2014-11-30 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.56 | 64.32 | 11.95 | 34.00 | -18.97 | 108.14 | 4.50 | 192.18 | 0.3511 | 272.7 | 85.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.02 | 19.22 | 2.13 | 10.21 | -19.29 | 109.99 | 6.35 | 196.80 | 0.3629 | 1071.1 | 674.4 | |
| 8.12 | -1.00 | 4.31 | -1.00 | -19.41 | 109.71 | 6.07 | 196.00 | 0.3635 | 1115.7 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -19.73 | 109.47 | 5.83 | 195.16 | 0.3674 | 748.0 | 593.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -19.28 | 109.36 | 5.72 | 195.22 | 0.3600 | -302.0 | -271.2 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -19.38 | 109.27 | 5.63 | 194.92 | 0.3611 | 665.0 | 603.0 | |
| 0.00 | 3.25 | 0.00 | 1.72 | -19.28 | 108.67 | 5.03 | 193.46 | 0.3572 | 420.0 | 537.0 | |
| 7.52 | 16.74 | 3.98 | 8.85 | -19.06 | 108.25 | 4.61 | 192.53 | 0.3521 | 1091.5 | 644.2 | |
| 2.90 | 7.86 | 1.53 | 4.13 | -18.05 | 107.57 | 3.93 | 191.33 | 0.3336 | -1058.5 | -629.7 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -18.05 | 107.11 | 3.47 | 190.01 | 0.3322 | -1011.0 | -780.2 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -18.02 | 106.79 | 3.16 | 189.14 | 0.3308 | 850.0 | 720.7 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -17.77 | 106.51 | 2.87 | 188.45 | 0.3260 | 799.0 | 478.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -18.74 | 106.34 | 2.70 | 187.54 | 0.3415 | -609.0 | -334.2 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -18.80 | 105.68 | 2.04 | 185.70 | 0.3412 | -920.0 | -746.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -18.90 | 105.40 | 1.76 | 184.90 | 0.3423 | -812.0 | -576.2 | |
| 0.00 | 2.39 | 0.00 | 1.26 | -19.34 | 105.19 | 1.55 | 184.20 | 0.3493 | -1006.0 | -786.8 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -18.80 | 105.09 | 1.45 | 184.05 | 0.3404 | -901.0 | -588.2 | |
| 0.00 | 2.82 | 0.00 | 1.49 | -18.99 | 105.06 | 1.42 | 183.93 | 0.3434 | -931.0 | -758.3 | |
| 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. | |