SDO HMI 2014-03-29 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.44 | 351.64 | 47.19 | 200.74 | 10.06 | 146.44 | 24.58 | 304.32 | 0.4974 | -455.5 | -267.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.51 | 5.00 | 150.45 | 28.59 | 291.60 | 0.5148 | -627.0 | -535.1 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 4.90 | 149.70 | 27.84 | 291.97 | 0.5037 | -783.0 | -666.6 | |
| 6.31 | 12.70 | 3.69 | 7.42 | 10.45 | 149.04 | 27.18 | 302.15 | 0.5327 | -784.6 | -654.5 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 10.82 | 148.94 | 27.08 | 302.84 | 0.5343 | -595.0 | -457.8 | |
| 1.49 | 2.54 | 0.87 | 1.48 | 10.58 | 148.64 | 26.78 | 302.75 | 0.5288 | -773.6 | -620.8 | |
| 0.00 | 1.40 | 0.00 | 0.81 | 10.56 | 148.26 | 26.40 | 303.10 | 0.5239 | -585.0 | -579.9 | |
| 1.31 | 4.56 | 0.76 | 2.63 | 9.93 | 148.07 | 26.21 | 302.25 | 0.5165 | -594.3 | -446.6 | |
| 0.00 | 2.10 | 0.00 | 1.22 | 10.96 | 148.03 | 26.17 | 303.97 | 0.5242 | -648.0 | -539.9 | |
| 0.00 | 2.10 | 0.00 | 1.22 | 10.74 | 147.94 | 26.08 | 303.70 | 0.5213 | -571.0 | -403.9 | |
| 4.73 | 270.96 | 2.72 | 155.19 | 10.11 | 147.38 | 25.52 | 303.26 | 0.5092 | -776.9 | -331.0 | |
| 35.83 | -10.00 | 20.52 | -10.00 | 9.67 | 147.27 | 25.41 | 302.63 | 0.5043 | -1075.6 | 999999 | |
| 3.77 | 11.56 | 2.17 | 6.66 | 11.27 | 146.67 | 24.81 | 305.91 | 0.5102 | 753.2 | 241.5 | |
| 0.44 | -10.00 | 0.25 | -10.00 | 10.57 | 146.54 | 24.68 | 304.92 | 0.5026 | 485.0 | 999999 | |
| 20.76 | -10.00 | 11.86 | -10.00 | 10.35 | 146.49 | 24.63 | 304.61 | 0.5001 | -665.9 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 11.38 | 146.38 | 24.52 | 306.41 | 0.5076 | 810.0 | 718.4 | |
| 2.37 | -10.00 | 1.35 | -10.00 | 10.63 | 145.78 | 23.92 | 305.87 | 0.4937 | 640.1 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.35 | 10.03 | 145.63 | 23.77 | 305.03 | 0.4867 | -813.0 | -647.0 | |
| 1.14 | 3.33 | 0.64 | 1.86 | 10.02 | 144.21 | 22.35 | 306.72 | 0.4690 | -956.2 | -809.0 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 7.71 | 143.89 | 22.03 | 302.91 | 0.4446 | -705.0 | -640.3 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 9.72 | 143.63 | 21.77 | 306.91 | 0.4590 | -749.0 | -598.2 | |
| 0.00 | 2.19 | 0.00 | 1.22 | 10.53 | 143.06 | 21.20 | 309.07 | 0.4599 | -719.0 | -540.6 | |
| 2.89 | 4.82 | 1.60 | 2.67 | 10.83 | 141.91 | 20.05 | 311.16 | 0.4492 | -862.5 | -719.4 | |
| 0.00 | 2.01 | 0.00 | 1.11 | 10.69 | 141.51 | 19.65 | 311.49 | 0.4431 | -702.0 | -616.3 | |
| 0.70 | 7.36 | 0.38 | 4.02 | 9.99 | 140.50 | 18.64 | 311.79 | 0.4240 | 832.1 | 699.6 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 9.51 | 140.15 | 18.29 | 311.46 | 0.4149 | 951.0 | 817.0 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 9.41 | 139.99 | 18.13 | 311.54 | 0.4119 | 836.0 | 666.3 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 9.62 | 139.81 | 17.95 | 312.21 | 0.4120 | 831.0 | 742.5 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 9.25 | 139.76 | 17.90 | 311.61 | 0.4074 | 825.0 | 654.6 | |
| 0.00 | 1.66 | 0.00 | 0.91 | 10.42 | 139.25 | 17.39 | 314.54 | 0.4141 | 735.0 | 641.0 | |
| 0.00 | 1.75 | 0.00 | 0.95 | 9.96 | 138.81 | 16.95 | 314.48 | 0.4041 | 761.0 | 556.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 11.06 | 138.78 | 16.92 | 316.43 | 0.4161 | 614.0 | 503.7 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 7.29 | 138.55 | 16.69 | 309.75 | 0.3722 | -724.0 | -617.8 | |
| 0.70 | 2.37 | 0.38 | 1.29 | 11.83 | 138.41 | 16.55 | 318.33 | 0.4212 | 956.6 | 746.7 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 12.31 | 138.44 | 16.58 | 319.03 | 0.4271 | 687.0 | 465.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 10.38 | 138.07 | 16.21 | 316.49 | 0.4005 | 811.0 | 708.5 | |
| 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. | |