SDO HMI 2014-03-01 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.59 | 76.72 | 10.26 | 40.05 | -7.27 | 149.29 | 18.38 | 268.74 | 0.3145 | 401.3 | 299.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.70 | 50.56 | 5.63 | 26.59 | -7.58 | 150.89 | 19.98 | 267.68 | 0.3404 | 1028.2 | 573.8 | |
| 5.95 | -1.00 | 3.13 | -1.00 | -7.28 | 150.43 | 19.52 | 268.62 | 0.3329 | 1065.0 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -6.55 | 149.36 | 18.44 | 271.00 | 0.3157 | 669.0 | 533.7 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -6.50 | 148.95 | 18.03 | 271.22 | 0.3090 | 928.0 | 812.8 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -6.36 | 148.82 | 17.90 | 271.71 | 0.3070 | 647.0 | 544.5 | |
| 0.00 | 2.24 | 0.00 | 1.16 | -4.73 | 146.87 | 15.95 | 278.05 | 0.2779 | -489.0 | -433.7 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -5.36 | 146.79 | 15.87 | 275.84 | 0.2750 | -799.0 | -636.2 | |
| 0.52 | 6.21 | 0.27 | 3.20 | -5.63 | 146.76 | 15.85 | 274.87 | 0.2740 | -1025.7 | -721.0 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -9.12 | 146.42 | 15.50 | 261.92 | 0.2678 | 819.0 | 697.3 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -8.51 | 145.71 | 14.79 | 264.00 | 0.2551 | 778.0 | 599.5 | |
| 0.00 | 2.33 | 0.00 | 1.19 | -9.63 | 145.29 | 14.37 | 259.42 | 0.2501 | 917.0 | 689.2 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -7.76 | 145.12 | 14.21 | 266.92 | 0.2447 | -634.0 | -508.8 | |
| 2.42 | 4.23 | 1.23 | 2.16 | -7.95 | 144.76 | 13.84 | 266.10 | 0.2386 | -1031.8 | -804.7 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -5.61 | 144.48 | 13.56 | 276.06 | 0.2358 | -855.0 | -704.6 | |
| 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. | |