SDO HMI 2014-03-28 08:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.00 | 328.87 | 35.69 | 175.26 | 10.17 | 145.62 | 13.30 | 322.12 | 0.3698 | -345.0 | -195.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.62 | 10.11 | 150.45 | 18.14 | 312.82 | 0.4196 | -811.0 | -651.7 | |
| 0.00 | 4.64 | 0.00 | 2.51 | 11.04 | 148.21 | 15.90 | 318.20 | 0.4051 | -895.0 | -630.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 10.84 | 148.14 | 15.82 | 318.02 | 0.4021 | -738.0 | -577.2 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 10.71 | 147.94 | 15.63 | 318.15 | 0.3984 | -748.0 | -633.2 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 10.78 | 147.06 | 14.75 | 319.91 | 0.3900 | -765.0 | -611.2 | |
| 34.95 | 255.65 | 18.65 | 136.63 | 9.65 | 146.85 | 14.53 | 318.36 | 0.3740 | -1276.1 | -276.9 | |
| 2.98 | -6.00 | 1.60 | -6.00 | 10.83 | 146.78 | 14.47 | 320.55 | 0.3878 | -514.7 | 999999 | |
| 1.49 | -6.00 | 0.80 | -6.00 | 11.08 | 146.73 | 14.42 | 321.06 | 0.3904 | 386.6 | 999999 | |
| 7.44 | -6.00 | 3.98 | -6.00 | 10.26 | 146.59 | 14.28 | 319.95 | 0.3788 | -1001.5 | 999999 | |
| 1.75 | -6.00 | 0.94 | -6.00 | 11.01 | 146.50 | 14.19 | 321.38 | 0.3873 | 721.0 | 999999 | |
| 3.77 | -6.00 | 2.02 | -6.00 | 11.01 | 146.22 | 13.91 | 321.93 | 0.3843 | 1088.4 | 999999 | |
| 1.14 | -6.00 | 0.61 | -6.00 | 10.80 | 145.74 | 13.43 | 322.58 | 0.3770 | 819.5 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.33 | 11.15 | 145.73 | 13.41 | 323.17 | 0.3813 | -578.0 | -525.3 | |
| 0.00 | 2.45 | 0.00 | 1.31 | 10.83 | 145.43 | 13.12 | 323.27 | 0.3743 | -909.0 | -736.8 | |
| 1.31 | 5.25 | 0.70 | 2.79 | 10.38 | 145.06 | 12.75 | 323.31 | 0.3650 | -941.1 | -811.5 | |
| 0.61 | 2.10 | 0.33 | 1.12 | 10.50 | 144.85 | 12.54 | 323.97 | 0.3645 | -1003.7 | -781.4 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 10.09 | 144.68 | 12.37 | 323.67 | 0.3574 | -950.0 | -799.5 | |
| 0.53 | 1.49 | 0.28 | 0.79 | 10.29 | 144.13 | 11.81 | 325.24 | 0.3549 | -1044.5 | -887.6 | |
| 0.00 | 1.49 | 0.00 | 0.78 | 9.53 | 142.21 | 9.90 | 328.65 | 0.3274 | 893.0 | 757.8 | |
| 4.20 | 11.04 | 2.21 | 5.79 | 10.55 | 141.14 | 8.82 | 332.97 | 0.3333 | -1027.8 | -674.3 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 9.84 | 140.32 | 8.00 | 334.23 | 0.3169 | 758.0 | 561.6 | |
| 0.00 | 2.45 | 0.00 | 1.27 | 9.03 | 140.05 | 7.74 | 333.82 | 0.3028 | 771.0 | 719.2 | |
| 0.00 | 1.66 | 0.00 | 0.87 | 9.62 | 140.07 | 7.75 | 334.63 | 0.3118 | 777.0 | 622.9 | |
| 0.00 | 2.01 | 0.00 | 1.05 | 10.03 | 139.95 | 7.64 | 335.50 | 0.3171 | 706.0 | 599.1 | |
| 0.00 | 0.53 | 0.00 | 0.28 | 10.62 | 139.66 | 7.35 | 337.07 | 0.3241 | 696.0 | 626.3 | |
| 0.00 | 2.36 | 0.00 | 1.24 | 10.77 | 139.57 | 7.26 | 337.50 | 0.3260 | 774.0 | 573.2 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 10.99 | 139.52 | 7.21 | 337.92 | 0.3290 | 753.0 | 608.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 11.21 | 139.31 | 7.00 | 338.74 | 0.3310 | 484.0 | 403.3 | |
| 0.35 | 2.63 | 0.18 | 1.37 | 10.45 | 139.14 | 6.82 | 338.37 | 0.3183 | 1003.2 | 875.0 | |
| 0.35 | -29.00 | 0.18 | -29.00 | 10.42 | 139.04 | 6.73 | 338.60 | 0.3173 | 1037.8 | 999999 | |
| 3.50 | 5.69 | 1.83 | 2.98 | 10.86 | 138.93 | 6.62 | 339.41 | 0.3234 | 1058.9 | 797.1 | |
| 1.23 | 2.98 | 0.64 | 1.57 | 11.71 | 138.95 | 6.64 | 340.26 | 0.3367 | 1016.4 | 840.8 | |
| 1.40 | 5.96 | 0.74 | 3.14 | 12.40 | 138.78 | 6.47 | 341.39 | 0.3466 | 1006.1 | 820.8 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 10.48 | 138.71 | 6.40 | 339.64 | 0.3162 | 939.0 | 750.6 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 12.72 | 138.64 | 6.33 | 342.07 | 0.3507 | 842.0 | 653.8 | |
| 0.00 | 4.64 | 0.00 | 2.43 | 10.82 | 138.35 | 6.04 | 341.06 | 0.3195 | 1000.0 | 856.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 10.10 | 138.12 | 5.81 | 340.98 | 0.3069 | 848.0 | 677.4 | |
| 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. | |