SDO HMI 2014-10-08 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.19 | 208.36 | 33.19 | 140.35 | -14.89 | 121.94 | 37.25 | 239.78 | 0.6790 | 344.7 | 209.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.98 | -15.55 | 124.15 | 39.46 | 240.37 | 0.7067 | 210.0 | 285.8 | |
| 16.66 | 60.07 | 11.42 | 41.25 | -14.41 | 123.46 | 38.77 | 241.42 | 0.6930 | 907.3 | 218.9 | |
| 6.75 | 25.70 | 4.66 | 17.75 | -15.47 | 123.49 | 38.80 | 240.07 | 0.6992 | 921.3 | 551.9 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -15.93 | 123.11 | 38.42 | 239.25 | 0.6977 | 254.0 | 392.3 | |
| 0.00 | 2.89 | 0.00 | 1.98 | -15.52 | 122.78 | 38.09 | 239.57 | 0.6918 | 294.0 | 393.8 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -15.09 | 122.61 | 37.92 | 240.01 | 0.6875 | 151.0 | 78.8 | |
| 5.52 | 44.02 | 3.72 | 29.71 | -14.46 | 122.33 | 37.64 | 240.65 | 0.6807 | 843.9 | 486.8 | |
| 0.00 | 1.75 | 0.00 | 1.19 | -15.56 | 122.43 | 37.75 | 239.29 | 0.6883 | 242.0 | 332.0 | |
| 4.12 | -7.00 | 2.78 | -7.00 | -14.74 | 122.23 | 37.54 | 240.22 | 0.6812 | 958.0 | 999999 | |
| 0.44 | -7.00 | 0.30 | -7.00 | -15.16 | 122.31 | 37.62 | 239.72 | 0.6846 | -178.0 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.90 | -16.27 | 122.51 | 37.83 | 238.43 | 0.6933 | 749.0 | 588.2 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -14.05 | 121.93 | 37.25 | 240.94 | 0.6740 | 742.0 | 603.6 | |
| 1.40 | 2.98 | 0.94 | 2.00 | -14.43 | 121.93 | 37.24 | 240.43 | 0.6762 | 913.5 | 730.2 | |
| 1.67 | 3.95 | 1.10 | 2.61 | -13.76 | 121.38 | 36.69 | 240.98 | 0.6660 | 849.1 | 642.8 | |
| 4.21 | 9.38 | 2.81 | 6.26 | -14.87 | 121.32 | 36.63 | 239.45 | 0.6719 | 871.0 | 581.7 | |
| 0.79 | 3.68 | 0.52 | 2.44 | -14.53 | 121.10 | 36.41 | 239.75 | 0.6674 | 836.8 | 692.7 | |
| 0.00 | 1.40 | 0.00 | 0.93 | -14.34 | 121.06 | 36.37 | 239.99 | 0.6659 | 781.0 | 671.7 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -16.22 | 121.44 | 36.75 | 237.77 | 0.6816 | -239.0 | -144.0 | |
| 0.53 | 3.16 | 0.35 | 2.09 | -14.71 | 120.82 | 36.13 | 239.33 | 0.6654 | 894.0 | 749.4 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -15.68 | 121.02 | 36.33 | 238.18 | 0.6736 | -15.0 | -92.7 | |
| 0.00 | 0.96 | 0.00 | 0.63 | -14.20 | 120.38 | 35.70 | 239.72 | 0.6574 | -279.0 | -222.0 | |
| 0.00 | 1.32 | 0.00 | 0.87 | -15.77 | 120.49 | 35.81 | 237.70 | 0.6684 | -581.0 | -400.1 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -16.03 | 120.55 | 35.86 | 237.39 | 0.6707 | -738.0 | -637.2 | |
| 0.00 | 1.93 | 0.00 | 1.26 | -14.25 | 120.16 | 35.48 | 239.50 | 0.6552 | -87.0 | -111.3 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -15.17 | 119.69 | 35.00 | 237.92 | 0.6557 | -369.0 | -213.0 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -14.03 | 118.32 | 33.63 | 238.47 | 0.6327 | -211.0 | -326.0 | |
| 0.96 | 20.96 | 0.63 | 13.57 | -15.90 | 118.62 | 33.93 | 236.15 | 0.6487 | -563.9 | -615.0 | |
| 0.00 | 2.37 | 0.00 | 1.53 | -15.42 | 118.53 | 33.84 | 236.73 | 0.6444 | -381.0 | -521.5 | |
| 4.65 | -27.00 | 3.01 | -27.00 | -16.05 | 118.38 | 33.70 | 235.77 | 0.6471 | -805.0 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.19 | -15.49 | 118.20 | 33.52 | 236.38 | 0.6413 | -779.0 | -632.2 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -14.09 | 117.85 | 33.16 | 238.02 | 0.6278 | -642.0 | -488.6 | |
| 1.49 | 5.70 | 0.95 | 3.65 | -15.15 | 117.88 | 33.19 | 236.59 | 0.6353 | -485.8 | -420.2 | |
| 0.00 | 1.14 | 0.00 | 0.73 | -15.43 | 117.71 | 33.02 | 236.08 | 0.6353 | -734.0 | -621.9 | |
| 0.00 | 1.49 | 0.00 | 0.93 | -13.87 | 116.90 | 32.21 | 237.58 | 0.6153 | -759.0 | -563.2 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -14.97 | 115.98 | 31.29 | 235.30 | 0.6126 | -762.0 | -610.3 | |
| 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. | |