SDO HMI 2014-08-17 04:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.15 | 355.16 | 49.56 | 210.70 | 16.13 | 24.26 | -32.54 | 70.52 | 0.5486 | -118.9 | -72.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.50 | 15.01 | 29.89 | -26.90 | 70.34 | 0.4660 | -822.0 | -694.2 | |
| 0.27 | 167.87 | 0.15 | 95.55 | 16.09 | 28.56 | -28.23 | 68.86 | 0.4893 | -1187.7 | -450.9 | |
| 1.80 | -2.00 | 1.02 | -2.00 | 16.17 | 28.44 | -28.36 | 68.75 | 0.4914 | -1243.9 | 999999 | |
| 0.99 | -2.00 | 0.56 | -2.00 | 15.86 | 28.49 | -28.31 | 69.33 | 0.4895 | -1243.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 18.33 | 27.71 | -29.08 | 65.02 | 0.5111 | -525.0 | -461.1 | |
| 29.55 | -2.00 | 16.84 | -2.00 | 15.96 | 28.04 | -28.76 | 69.36 | 0.4962 | -1206.5 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 16.63 | 26.73 | -30.06 | 68.72 | 0.5172 | -681.0 | -569.6 | |
| 12.07 | 16.40 | 6.97 | 9.47 | 16.20 | 26.69 | -30.10 | 69.56 | 0.5160 | -906.4 | -495.2 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 15.67 | 26.05 | -30.75 | 70.84 | 0.5232 | -729.0 | -519.3 | |
| 0.00 | 1.44 | 0.00 | 0.84 | 15.65 | 25.72 | -31.07 | 71.01 | 0.5277 | -617.0 | -517.0 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 17.27 | 25.28 | -31.51 | 68.25 | 0.5395 | -692.0 | -620.6 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 15.43 | 25.61 | -31.18 | 71.46 | 0.5285 | -763.0 | -575.3 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 17.36 | 24.78 | -32.02 | 68.31 | 0.5467 | -683.0 | -515.2 | |
| 0.00 | 5.41 | 0.00 | 3.18 | 16.44 | 24.91 | -31.88 | 69.90 | 0.5415 | -661.0 | -599.1 | |
| 0.00 | 2.97 | 0.00 | 1.76 | 17.32 | 24.56 | -32.23 | 68.48 | 0.5494 | -444.0 | -497.8 | |
| 0.00 | 1.80 | 0.00 | 1.07 | 17.04 | 24.54 | -32.25 | 68.99 | 0.5487 | -670.0 | -581.2 | |
| 0.00 | 3.15 | 0.00 | 1.87 | 16.53 | 24.37 | -32.42 | 69.96 | 0.5492 | -628.0 | -424.5 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 18.15 | 22.98 | -33.82 | 67.72 | 0.5737 | -484.0 | -396.6 | |
| 0.00 | 1.89 | 0.00 | 1.13 | 15.57 | 23.42 | -33.37 | 72.00 | 0.5593 | 895.0 | 766.9 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 18.27 | 22.84 | -33.96 | 67.58 | 0.5759 | -659.0 | -482.2 | |
| 0.00 | 1.71 | 0.00 | 1.02 | 15.71 | 23.17 | -33.63 | 71.84 | 0.5632 | 866.0 | 662.4 | |
| 0.00 | 4.42 | 0.00 | 2.70 | 17.50 | 21.53 | -35.26 | 69.38 | 0.5905 | 872.0 | 756.0 | |
| 0.00 | 0.45 | 0.00 | 0.28 | 16.70 | 21.20 | -35.60 | 70.82 | 0.5925 | 739.0 | 634.4 | |
| 0.00 | 4.23 | 0.00 | 2.60 | 16.27 | 21.21 | -35.58 | 71.53 | 0.5911 | 923.0 | 759.5 | |
| 0.00 | 1.44 | 0.00 | 0.88 | 15.70 | 21.05 | -35.74 | 72.53 | 0.5917 | 826.0 | 674.8 | |
| 0.00 | 3.78 | 0.00 | 2.34 | 17.19 | 20.58 | -36.21 | 70.22 | 0.6020 | 907.0 | 771.0 | |
| 6.04 | 8.65 | 3.72 | 5.33 | 15.73 | 20.62 | -36.17 | 72.60 | 0.5976 | 967.0 | 703.1 | |
| 4.69 | 12.34 | 2.91 | 7.67 | 16.60 | 20.16 | -36.64 | 71.31 | 0.6059 | 949.7 | 563.5 | |
| 0.00 | 4.69 | 0.00 | 2.91 | 16.29 | 20.19 | -36.61 | 71.80 | 0.6047 | 880.0 | 756.9 | |
| 0.90 | 44.33 | 0.56 | 27.87 | 16.85 | 19.67 | -37.13 | 71.06 | 0.6130 | 743.1 | 184.4 | |
| 0.00 | 1.71 | 0.00 | 1.07 | 17.25 | 19.57 | -37.22 | 70.45 | 0.6153 | 647.0 | 519.9 | |
| 10.09 | 53.97 | 6.30 | 33.69 | 15.70 | 19.60 | -37.19 | 72.94 | 0.6110 | 1086.2 | 470.7 | |
| 12.16 | -30.00 | 7.63 | -30.00 | 16.55 | 19.41 | -37.38 | 71.61 | 0.6155 | 892.0 | 999999 | |
| 2.25 | -30.00 | 1.42 | -30.00 | 16.95 | 19.32 | -37.47 | 71.00 | 0.6177 | 545.5 | 999999 | |
| 2.34 | -30.00 | 1.48 | -30.00 | 16.33 | 18.94 | -37.85 | 72.09 | 0.6211 | 575.4 | 999999 | |
| 0.00 | 3.69 | 0.00 | 2.32 | 15.72 | 19.04 | -37.75 | 73.04 | 0.6184 | 553.0 | 401.6 | |
| 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. | |