SDO HMI 2014-03-29 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.36 | 441.91 | 72.68 | 362.53 | -13.27 | 172.85 | 53.18 | 258.35 | 0.7969 | 480.3 | 229.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.83 | -11.06 | 175.22 | 55.56 | 261.16 | 0.8213 | 431.0 | 306.6 | |
| 0.00 | 0.53 | 0.00 | 0.45 | -10.85 | 174.84 | 55.17 | 261.42 | 0.8175 | 440.0 | 402.2 | |
| 0.00 | 2.98 | 0.00 | 2.53 | -11.01 | 174.46 | 54.79 | 261.23 | 0.8137 | 746.0 | 589.0 | |
| 0.00 | 1.05 | 0.00 | 0.89 | -11.27 | 174.53 | 54.86 | 260.90 | 0.8144 | 418.0 | 339.4 | |
| 22.35 | 95.70 | 18.97 | 81.17 | -11.97 | 174.52 | 54.85 | 260.04 | 0.8143 | 691.0 | 140.3 | |
| 0.79 | 2.54 | 0.66 | 2.13 | -10.78 | 173.92 | 54.25 | 261.51 | 0.8083 | 635.9 | 531.2 | |
| 15.16 | -5.00 | 12.69 | -5.00 | -11.73 | 173.92 | 54.25 | 260.34 | 0.8083 | 906.3 | 999999 | |
| 1.05 | 4.82 | 0.87 | 4.00 | -10.91 | 173.54 | 53.87 | 261.36 | 0.8044 | 749.8 | 575.5 | |
| 0.00 | 1.05 | 0.00 | 0.87 | -11.08 | 173.37 | 53.70 | 261.15 | 0.8027 | 710.0 | 661.2 | |
| 0.00 | 1.05 | 0.00 | 0.87 | -11.27 | 173.22 | 53.55 | 260.90 | 0.8011 | 771.0 | 645.1 | |
| 0.00 | 1.75 | 0.00 | 1.44 | -11.47 | 173.12 | 53.45 | 260.66 | 0.8001 | 524.0 | 561.7 | |
| 37.68 | 250.89 | 31.38 | 209.27 | -13.85 | 173.64 | 53.97 | 257.69 | 0.8059 | 1025.0 | 308.5 | |
| 0.00 | 1.05 | 0.00 | 0.86 | -11.39 | 172.89 | 53.22 | 260.75 | 0.7978 | 676.0 | 590.2 | |
| 3.24 | 11.66 | 2.65 | 9.52 | -14.91 | 172.80 | 53.13 | 256.33 | 0.7979 | 700.7 | 474.3 | |
| 0.00 | 0.79 | 0.00 | 0.64 | -14.68 | 172.26 | 52.59 | 256.58 | 0.7922 | 765.0 | 693.1 | |
| 0.00 | 0.70 | 0.00 | 0.57 | -14.92 | 172.34 | 52.67 | 256.29 | 0.7931 | 358.0 | 382.1 | |
| 4.29 | 7.27 | 3.40 | 5.76 | -12.28 | 171.47 | 51.80 | 259.60 | 0.7829 | 731.4 | 487.3 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -11.56 | 171.07 | 51.41 | 260.52 | 0.7786 | 542.0 | 522.6 | |
| 0.00 | 0.96 | 0.00 | 0.76 | -12.73 | 171.19 | 51.52 | 259.01 | 0.7802 | 215.0 | 208.5 | |
| 0.00 | 2.54 | 0.00 | 2.04 | -15.05 | 171.87 | 52.20 | 256.09 | 0.7884 | 283.0 | 322.3 | |
| 0.00 | 2.10 | 0.00 | 1.65 | -12.84 | 171.07 | 51.40 | 258.88 | 0.7789 | -17.0 | -38.3 | |
| 0.00 | 1.14 | 0.00 | 0.89 | -12.92 | 170.80 | 51.13 | 258.76 | 0.7760 | -581.0 | -410.8 | |
| 0.00 | 1.23 | 0.00 | 0.95 | -12.71 | 170.40 | 50.73 | 259.01 | 0.7716 | 684.0 | 613.0 | |
| 0.00 | 1.40 | 0.00 | 1.12 | -17.10 | 171.76 | 52.09 | 253.49 | 0.7889 | -576.0 | -407.8 | |
| 0.00 | 1.05 | 0.00 | 0.81 | -13.01 | 170.10 | 50.43 | 258.61 | 0.7684 | -360.0 | -256.0 | |
| 0.61 | 1.67 | 0.46 | 1.25 | -12.84 | 168.62 | 48.95 | 258.76 | 0.7519 | 664.3 | 551.1 | |
| 0.70 | 1.84 | 0.52 | 1.37 | -13.39 | 168.25 | 48.58 | 258.01 | 0.7481 | -471.9 | -345.8 | |
| 0.00 | 0.96 | 0.00 | 0.71 | -13.22 | 167.69 | 48.02 | 258.19 | 0.7417 | 676.0 | 628.7 | |
| 0.00 | 0.35 | 0.00 | 0.26 | -13.60 | 167.47 | 47.80 | 257.66 | 0.7394 | -442.0 | -489.8 | |
| 0.00 | 1.67 | 0.00 | 1.22 | -13.67 | 167.40 | 47.73 | 257.56 | 0.7386 | -581.0 | -465.4 | |
| 0.00 | 1.14 | 0.00 | 0.83 | -13.99 | 167.21 | 47.54 | 257.11 | 0.7367 | -502.0 | -359.8 | |
| 0.00 | 5.52 | 0.00 | 4.01 | -13.58 | 167.00 | 47.34 | 257.65 | 0.7340 | 61.0 | -105.9 | |
| 0.00 | 1.84 | 0.00 | 1.32 | -12.41 | 166.44 | 46.77 | 259.21 | 0.7268 | 658.0 | 517.3 | |
| 1.49 | 4.73 | 1.08 | 3.43 | -13.94 | 166.78 | 47.11 | 257.15 | 0.7317 | -809.6 | -605.3 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -12.97 | 166.35 | 46.68 | 258.44 | 0.7260 | 696.0 | 617.8 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -14.19 | 165.85 | 46.19 | 256.70 | 0.7212 | -540.0 | -446.9 | |
| 0.00 | 1.14 | 0.00 | 0.79 | -13.15 | 164.49 | 44.82 | 258.04 | 0.7040 | -486.0 | -399.2 | |
| 0.00 | 1.49 | 0.00 | 1.04 | -13.61 | 164.47 | 44.80 | 257.38 | 0.7041 | -576.0 | -440.8 | |
| 0.00 | 0.96 | 0.00 | 0.66 | -9.71 | 163.60 | 43.93 | 262.93 | 0.6914 | 111.0 | 217.5 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -9.63 | 163.38 | 43.71 | 263.04 | 0.6886 | 549.0 | 493.0 | |
| 0.00 | 1.23 | 0.00 | 0.84 | -13.67 | 163.62 | 43.95 | 257.19 | 0.6939 | -439.0 | -360.6 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -13.34 | 163.54 | 43.88 | 257.66 | 0.6927 | -564.0 | -502.7 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -13.00 | 163.25 | 43.59 | 258.13 | 0.6888 | -654.0 | -554.3 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -11.74 | 162.70 | 43.03 | 259.92 | 0.6809 | -240.0 | -243.1 | |
| 0.00 | 1.31 | 0.00 | 0.88 | -11.83 | 162.34 | 42.67 | 259.76 | 0.6764 | -446.0 | -302.6 | |
| 0.00 | 1.14 | 0.00 | 0.76 | -14.82 | 161.77 | 42.10 | 255.26 | 0.6725 | -387.0 | -430.4 | |
| 0.00 | 1.31 | 0.00 | 0.87 | -13.48 | 161.43 | 41.76 | 257.22 | 0.6664 | -774.0 | -595.1 | |
| 0.00 | 1.58 | 0.00 | 1.05 | -15.73 | 161.49 | 41.82 | 253.87 | 0.6705 | -544.0 | -475.8 | |
| 0.00 | 0.96 | 0.00 | 0.63 | -14.34 | 160.87 | 41.20 | 255.84 | 0.6605 | -600.0 | -457.4 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -12.73 | 160.49 | 40.82 | 258.23 | 0.6537 | -390.0 | -289.3 | |
| 0.00 | 1.31 | 0.00 | 0.87 | -15.19 | 160.94 | 41.27 | 254.57 | 0.6627 | -572.0 | -513.7 | |
| 0.00 | 0.96 | 0.00 | 0.63 | -14.02 | 160.64 | 40.97 | 256.28 | 0.6571 | -671.0 | -593.5 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -15.17 | 160.73 | 41.06 | 254.55 | 0.6601 | -681.0 | -580.6 | |
| 0.00 | 1.58 | 0.00 | 1.03 | -15.34 | 160.48 | 40.81 | 254.25 | 0.6572 | -620.0 | -494.8 | |
| 0.00 | 1.49 | 0.00 | 0.96 | -12.90 | 159.84 | 40.17 | 257.89 | 0.6454 | -683.0 | -605.4 | |
| 0.00 | 2.02 | 0.00 | 1.30 | -14.01 | 159.50 | 39.83 | 256.11 | 0.6424 | -702.0 | -593.4 | |
| 0.00 | 1.14 | 0.00 | 0.73 | -13.82 | 158.74 | 39.07 | 256.27 | 0.6323 | -767.0 | -601.9 | |
| 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. | |