SDO HMI 2014-04-16 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.72 | 307.58 | 38.67 | 152.96 | -9.47 | 245.48 | 1.72 | 200.06 | 0.0859 | 359.0 | 119.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.68 | 0.00 | 0.84 | -8.48 | 248.21 | 4.45 | 236.08 | 0.0930 | -240.0 | -237.3 | |
| 40.36 | 139.76 | 20.09 | 69.54 | -9.33 | 247.83 | 4.06 | 226.52 | 0.0968 | 1339.3 | 470.0 | |
| 0.00 | 1.42 | 0.00 | 0.71 | -9.93 | 247.80 | 4.04 | 222.10 | 0.1040 | 13.0 | 100.8 | |
| 2.57 | -2.00 | 1.28 | -2.00 | -8.73 | 247.48 | 3.72 | 228.99 | 0.0855 | 1115.9 | 999999 | |
| 0.00 | 2.30 | 0.00 | 1.15 | -12.02 | 247.33 | 3.57 | 208.34 | 0.1290 | 840.0 | 688.3 | |
| 2.48 | 11.06 | 1.23 | 5.50 | -8.46 | 246.78 | 3.02 | 225.58 | 0.0733 | 1071.9 | 568.5 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -7.38 | 246.05 | 2.28 | 230.87 | 0.0512 | 826.0 | 572.9 | |
| 0.00 | 2.12 | 0.00 | 1.06 | -10.30 | 246.03 | 2.27 | 205.12 | 0.0922 | -955.0 | -789.5 | |
| 0.00 | 2.21 | 0.00 | 1.10 | -10.36 | 245.69 | 1.93 | 201.53 | 0.0908 | 915.0 | 639.8 | |
| 0.00 | 2.39 | 0.00 | 1.19 | -8.58 | 245.50 | 1.74 | 209.50 | 0.0613 | -822.0 | -609.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -10.33 | 245.39 | 1.63 | 198.48 | 0.0885 | 759.0 | 469.8 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -8.10 | 245.29 | 1.53 | 210.54 | 0.0522 | -947.0 | -804.4 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -8.19 | 245.20 | 1.44 | 208.19 | 0.0528 | -898.0 | -742.3 | |
| 0.00 | 1.77 | 0.00 | 0.88 | -10.42 | 245.08 | 1.32 | 194.91 | 0.0885 | -591.0 | -535.0 | |
| 0.71 | 3.54 | 0.35 | 1.76 | -8.46 | 244.96 | 1.19 | 202.00 | 0.0553 | -989.5 | -784.6 | |
| 0.00 | 1.59 | 0.00 | 0.79 | -8.25 | 244.89 | 1.13 | 202.46 | 0.0515 | -843.0 | -546.0 | |
| 0.00 | 2.30 | 0.00 | 1.14 | -9.28 | 244.71 | 0.95 | 194.12 | 0.0675 | -464.0 | -538.4 | |
| 0.00 | 1.33 | 0.00 | 0.66 | -8.37 | 244.56 | 0.80 | 195.59 | 0.0516 | -1088.0 | -752.2 | |
| 0.80 | 9.29 | 0.40 | 4.62 | -9.46 | 244.50 | 0.74 | 190.55 | 0.0698 | -962.2 | -780.1 | |
| 2.12 | 4.34 | 1.06 | 2.16 | -10.72 | 244.13 | 0.37 | 184.05 | 0.0910 | -1057.1 | -705.2 | |
| 1.68 | 3.63 | 0.84 | 1.80 | -9.94 | 244.07 | 0.31 | 184.00 | 0.0773 | -984.1 | -706.0 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -9.97 | 243.83 | 0.07 | 180.87 | 0.0776 | -722.0 | -501.5 | |
| 2.39 | 5.22 | 1.19 | 2.60 | -10.57 | 243.68 | -0.09 | 179.04 | 0.0882 | -1088.6 | -761.8 | |
| 0.71 | 1.68 | 0.35 | 0.84 | -10.75 | 243.55 | -0.21 | 177.75 | 0.0914 | -970.6 | -746.1 | |
| 10.36 | 13.72 | 5.14 | 6.80 | -8.37 | 243.50 | -0.26 | 174.72 | 0.0499 | 1116.4 | 768.9 | |
| 0.00 | 3.89 | 0.00 | 1.93 | -9.03 | 243.40 | -0.36 | 174.23 | 0.0616 | -1121.0 | -886.0 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -10.69 | 242.63 | -1.13 | 167.86 | 0.0923 | -800.0 | -604.3 | |
| 1.95 | 82.14 | 0.97 | 40.81 | -9.18 | 242.55 | -1.21 | 161.84 | 0.0672 | 987.0 | -74.6 | |
| 3.89 | -28.00 | 1.94 | -28.00 | -10.03 | 242.45 | -1.31 | 164.00 | 0.0818 | -967.3 | 999999 | |
| 2.48 | -28.00 | 1.23 | -28.00 | -9.48 | 242.34 | -1.43 | 160.38 | 0.0734 | 918.0 | 999999 | |
| 5.22 | -28.00 | 2.60 | -28.00 | -10.48 | 242.27 | -1.49 | 163.44 | 0.0903 | -1156.9 | 999999 | |
| 0.00 | 1.68 | 0.00 | 0.84 | -9.09 | 242.09 | -1.67 | 155.14 | 0.0686 | 1078.0 | 893.5 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -11.50 | 241.96 | -1.81 | 163.46 | 0.1090 | 685.0 | 627.9 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -9.21 | 241.91 | -1.85 | 153.55 | 0.0719 | 803.0 | 669.3 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -2.47 | 235.77 | -7.99 | 69.26 | 0.1491 | 713.0 | 591.1 | |
| 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. | |