SDO HMI 2014-11-17 19:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.78 | 79.69 | 19.06 | 63.16 | -13.24 | 225.24 | -49.19 | 109.27 | 0.7823 | -108.6 | -100.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.77 | -10.16 | 232.03 | -42.40 | 107.45 | 0.6982 | -548.0 | -372.9 | |
| 0.00 | 1.03 | 0.00 | 0.76 | -13.29 | 228.86 | -45.57 | 110.51 | 0.7444 | 636.0 | 547.1 | |
| 0.00 | 1.37 | 0.00 | 1.01 | -12.95 | 228.76 | -45.67 | 110.04 | 0.7444 | 726.0 | 476.2 | |
| 3.52 | 10.30 | 2.63 | 7.72 | -12.76 | 228.06 | -46.37 | 109.55 | 0.7515 | 781.4 | 524.5 | |
| 0.00 | 1.03 | 0.00 | 0.77 | -11.26 | 227.96 | -46.47 | 107.58 | 0.7482 | 604.0 | 450.4 | |
| 0.00 | 1.72 | 0.00 | 1.31 | -13.18 | 227.29 | -47.14 | 109.83 | 0.7611 | 415.0 | 269.5 | |
| 0.00 | 1.03 | 0.00 | 0.78 | -12.88 | 227.28 | -47.16 | 109.43 | 0.7603 | 460.0 | 326.6 | |
| 0.00 | 0.86 | 0.00 | 0.65 | -11.50 | 227.38 | -47.05 | 107.70 | 0.7553 | 125.0 | 231.6 | |
| 0.00 | 2.40 | 0.00 | 1.87 | -14.69 | 226.46 | -47.97 | 111.45 | 0.7743 | -702.0 | -582.6 | |
| 0.00 | 0.94 | 0.00 | 0.72 | -11.97 | 226.87 | -47.57 | 108.15 | 0.7621 | 518.0 | 419.2 | |
| 0.00 | 0.52 | 0.00 | 0.39 | -11.79 | 226.86 | -47.57 | 107.91 | 0.7617 | 459.0 | 406.5 | |
| 0.00 | 1.46 | 0.00 | 1.13 | -13.09 | 226.50 | -47.93 | 109.45 | 0.7692 | -706.0 | -549.3 | |
| 6.35 | 17.17 | 5.03 | 13.53 | -14.90 | 225.75 | -48.68 | 111.46 | 0.7822 | -755.5 | -538.5 | |
| 0.00 | 0.69 | 0.00 | 0.54 | -14.59 | 225.85 | -48.59 | 111.11 | 0.7803 | -415.0 | -392.1 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -13.21 | 225.59 | -48.84 | 109.31 | 0.7790 | 274.0 | 256.0 | |
| 4.55 | 10.73 | 3.57 | 8.42 | -12.66 | 225.60 | -48.83 | 108.62 | 0.7774 | 850.3 | 465.8 | |
| 0.43 | 1.12 | 0.34 | 0.88 | -12.88 | 225.40 | -49.03 | 108.84 | 0.7801 | 311.0 | 254.6 | |
| 0.00 | 0.94 | 0.00 | 0.75 | -10.81 | 224.32 | -50.11 | 105.95 | 0.7862 | -298.0 | -365.4 | |
| 0.00 | 1.12 | 0.00 | 0.91 | -13.06 | 223.59 | -50.84 | 108.53 | 0.7989 | -785.0 | -701.5 | |
| 3.52 | 7.30 | 2.91 | 6.05 | -13.17 | 223.17 | -51.26 | 108.55 | 0.8034 | -780.9 | -514.3 | |
| 0.00 | 1.29 | 0.00 | 1.07 | -12.66 | 222.93 | -51.50 | 107.86 | 0.8045 | -530.0 | -490.7 | |
| 0.00 | 1.55 | 0.00 | 1.30 | -13.29 | 222.49 | -51.94 | 108.50 | 0.8103 | -206.0 | -178.2 | |
| 0.69 | 1.72 | 0.58 | 1.44 | -12.76 | 222.55 | -51.88 | 107.88 | 0.8085 | -744.9 | -689.6 | |
| 0.00 | 0.77 | 0.00 | 0.65 | -13.08 | 222.21 | -52.22 | 108.17 | 0.8126 | -302.0 | -247.4 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -11.97 | 222.43 | -52.00 | 106.89 | 0.8079 | -507.0 | -532.7 | |
| 4.72 | 10.99 | 4.00 | 9.32 | -12.66 | 222.04 | -52.40 | 107.62 | 0.8133 | -615.4 | -202.0 | |
| 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. | |