SDO HMI 2014-11-03 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 131.30 | 606.44 | 67.91 | 313.49 | 12.07 | 114.53 | 14.41 | 300.66 | 0.2831 | -192.0 | -59.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.32 | 352.53 | 2.27 | 183.95 | 12.24 | 117.90 | 17.78 | 295.82 | 0.3330 | -947.8 | -446.4 | |
| 4.84 | -1.00 | 2.54 | -1.00 | 12.15 | 117.54 | 17.42 | 296.01 | 0.3271 | -950.4 | 999999 | |
| 13.22 | -1.00 | 6.92 | -1.00 | 12.01 | 117.27 | 17.16 | 295.92 | 0.3222 | -1192.1 | 999999 | |
| 32.93 | -1.00 | 17.18 | -1.00 | 12.11 | 116.71 | 16.59 | 296.92 | 0.3145 | -1417.0 | 999999 | |
| 4.41 | -1.00 | 2.29 | -1.00 | 12.03 | 116.17 | 16.05 | 297.42 | 0.3059 | -1214.2 | 999999 | |
| 3.98 | -1.00 | 2.07 | -1.00 | 12.42 | 116.16 | 16.04 | 298.58 | 0.3087 | -1022.0 | 999999 | |
| 11.41 | -1.00 | 5.92 | -1.00 | 11.40 | 116.06 | 15.95 | 295.65 | 0.3001 | -1150.6 | 999999 | |
| 1.90 | -1.00 | 0.99 | -1.00 | 11.53 | 115.79 | 15.67 | 296.41 | 0.2968 | -1321.5 | 999999 | |
| 3.63 | -1.00 | 1.88 | -1.00 | 11.71 | 115.77 | 15.65 | 296.99 | 0.2978 | -1140.2 | 999999 | |
| 2.59 | -1.00 | 1.34 | -1.00 | 11.33 | 115.46 | 15.34 | 296.22 | 0.2905 | -1079.5 | 999999 | |
| 0.00 | 1.47 | 0.00 | 0.76 | 11.58 | 114.66 | 14.54 | 298.21 | 0.2804 | 728.0 | 585.6 | |
| 0.00 | 2.59 | 0.00 | 1.34 | 12.66 | 114.69 | 14.57 | 301.54 | 0.2893 | 756.0 | 644.5 | |
| 0.00 | 1.99 | 0.00 | 1.03 | 12.49 | 114.52 | 14.40 | 301.28 | 0.2855 | 625.0 | 523.4 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 11.92 | 114.05 | 13.93 | 300.30 | 0.2741 | 708.0 | 556.6 | |
| 1.56 | 6.65 | 0.80 | 3.43 | 12.13 | 114.00 | 13.88 | 301.07 | 0.2751 | 1132.2 | 788.9 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 12.28 | 112.79 | 12.67 | 303.79 | 0.2591 | 634.0 | 457.7 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 11.02 | 112.70 | 12.58 | 299.64 | 0.2471 | 866.0 | 716.9 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 11.89 | 112.61 | 12.50 | 302.84 | 0.2532 | 861.0 | 732.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 12.07 | 112.56 | 12.44 | 303.56 | 0.2540 | 810.0 | 631.3 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 11.54 | 112.19 | 12.08 | 302.47 | 0.2441 | 826.0 | 695.6 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 11.54 | 111.85 | 11.74 | 303.21 | 0.2393 | 802.0 | 543.1 | |
| 3.20 | 232.22 | 1.63 | 118.38 | 12.11 | 111.78 | 11.67 | 305.36 | 0.2436 | 954.7 | 438.4 | |
| 6.14 | -22.00 | 3.13 | -22.00 | 12.15 | 111.57 | 11.45 | 305.96 | 0.2409 | 1270.3 | 999999 | |
| 14.52 | -22.00 | 7.41 | -22.00 | 12.27 | 111.39 | 11.27 | 306.81 | 0.2396 | 1297.9 | 999999 | |
| 21.61 | -22.00 | 11.01 | -22.00 | 12.30 | 111.08 | 10.96 | 307.67 | 0.2358 | 1328.3 | 999999 | |
| 1.04 | -22.00 | 0.53 | -22.00 | 11.70 | 111.05 | 10.94 | 305.61 | 0.2296 | 966.1 | 999999 | |
| 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. | |