SDO HMI 2014-05-28 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.35 | 88.84 | 6.60 | 48.53 | -12.71 | 64.82 | 21.77 | 240.18 | 0.4190 | 373.0 | 352.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 8.75 | 0.71 | 4.94 | -13.40 | 69.07 | 26.02 | 243.27 | 0.4798 | -849.6 | -717.3 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -14.80 | 69.21 | 26.16 | 240.74 | 0.4905 | 783.0 | 648.0 | |
| 0.63 | 3.52 | 0.35 | 1.96 | -11.86 | 68.28 | 25.24 | 245.70 | 0.4597 | 813.1 | 664.1 | |
| 0.00 | 2.80 | 0.00 | 1.55 | -11.08 | 68.14 | 25.09 | 247.18 | 0.4534 | 853.0 | 708.2 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -8.57 | 67.40 | 24.35 | 252.11 | 0.4303 | 661.0 | 520.1 | |
| 1.08 | 2.08 | 0.60 | 1.15 | -12.76 | 67.72 | 24.67 | 243.42 | 0.4572 | 941.3 | 817.9 | |
| 0.00 | 7.04 | 0.00 | 3.89 | -11.27 | 67.44 | 24.39 | 246.24 | 0.4444 | 1007.0 | 718.3 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -11.46 | 67.19 | 24.14 | 245.64 | 0.4418 | 785.0 | 680.0 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -11.21 | 67.17 | 24.12 | 246.15 | 0.4401 | 1121.0 | 924.4 | |
| 0.00 | 2.71 | 0.00 | 1.49 | -11.09 | 66.99 | 23.94 | 246.26 | 0.4368 | 807.0 | 810.6 | |
| 0.00 | 1.89 | 0.00 | 1.04 | -11.43 | 66.85 | 23.80 | 245.42 | 0.4367 | 769.0 | 618.0 | |
| 0.00 | 4.96 | 0.00 | 2.74 | -12.42 | 66.87 | 23.82 | 243.36 | 0.4431 | 1009.0 | 830.5 | |
| 0.00 | 2.80 | 0.00 | 1.53 | -10.48 | 66.66 | 23.62 | 247.34 | 0.4287 | 790.0 | 687.5 | |
| 0.00 | 4.51 | 0.00 | 2.48 | -10.94 | 66.70 | 23.65 | 246.36 | 0.4318 | 802.0 | 718.9 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -7.81 | 65.91 | 22.86 | 252.91 | 0.4044 | -683.0 | -459.6 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -17.25 | 66.32 | 23.28 | 233.47 | 0.4716 | 587.0 | 468.2 | |
| 0.00 | 1.80 | 0.00 | 0.99 | -14.61 | 65.09 | 22.04 | 237.09 | 0.4343 | 841.0 | 696.0 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -15.30 | 65.09 | 22.04 | 235.73 | 0.4399 | 651.0 | 427.5 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -12.03 | 64.74 | 21.69 | 242.16 | 0.4106 | 741.0 | 625.5 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -11.97 | 64.37 | 21.32 | 241.91 | 0.4049 | 798.0 | 607.5 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -15.49 | 64.26 | 21.22 | 234.39 | 0.4308 | 639.0 | 471.8 | |
| 0.00 | 1.89 | 0.00 | 1.03 | -12.78 | 63.94 | 20.89 | 239.64 | 0.4047 | 776.0 | 682.1 | |
| 0.00 | 1.89 | 0.00 | 1.02 | -11.57 | 63.84 | 20.79 | 242.25 | 0.3946 | 964.0 | 812.3 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -15.24 | 64.17 | 21.12 | 234.77 | 0.4274 | 739.0 | 586.2 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -11.64 | 63.68 | 20.63 | 241.93 | 0.3928 | 943.0 | 748.0 | |
| 0.00 | 1.99 | 0.00 | 1.07 | -11.85 | 63.53 | 20.48 | 241.27 | 0.3922 | 1015.0 | 753.5 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -12.50 | 63.32 | 20.27 | 239.54 | 0.3940 | 856.0 | 773.4 | |
| 0.54 | 2.71 | 0.29 | 1.45 | -12.41 | 63.01 | 19.96 | 239.39 | 0.3890 | 1024.0 | 843.8 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -18.57 | 61.93 | 18.88 | 225.53 | 0.4317 | 813.0 | 657.5 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -12.86 | 60.09 | 17.04 | 234.39 | 0.3529 | -883.0 | -680.7 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -21.47 | 60.85 | 17.80 | 219.19 | 0.4520 | 786.0 | 625.3 | |
| 1.17 | 2.98 | 0.62 | 1.57 | -11.56 | 59.90 | 16.86 | 237.31 | 0.3390 | -1085.6 | -880.2 | |
| 0.00 | 2.44 | 0.00 | 1.29 | -13.05 | 59.87 | 16.82 | 233.61 | 0.3518 | -800.0 | -726.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -14.86 | 59.94 | 16.89 | 229.66 | 0.3701 | -706.0 | -562.9 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -15.39 | 59.79 | 16.74 | 228.28 | 0.3736 | -608.0 | -449.8 | |
| 7.67 | 10.20 | 4.03 | 5.36 | -14.18 | 57.58 | 14.53 | 227.00 | 0.3340 | -1034.0 | -740.4 | |
| 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. | |