SDO HMI 2014-03-22 17:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.57 | 416.00 | 45.86 | 257.22 | -13.66 | 169.78 | -36.72 | 103.62 | 0.5997 | 676.1 | 320.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.35 | 0.00 | 1.34 | -15.82 | 177.69 | -28.80 | 109.97 | 0.4952 | -482.0 | -557.6 | |
| 33.58 | 264.33 | 20.45 | 161.43 | -14.33 | 170.99 | -35.51 | 104.93 | 0.5846 | 1235.1 | 357.1 | |
| 0.96 | -2.00 | 0.58 | -2.00 | -13.90 | 170.88 | -35.62 | 104.17 | 0.5853 | 899.7 | 999999 | |
| 0.00 | 2.88 | 0.00 | 1.75 | -12.01 | 171.04 | -35.45 | 100.97 | 0.5801 | 763.0 | 675.3 | |
| 0.96 | -2.00 | 0.59 | -2.00 | -14.83 | 170.40 | -36.10 | 105.64 | 0.5936 | 381.5 | 999999 | |
| 0.00 | 1.66 | 0.00 | 1.01 | -11.51 | 170.78 | -35.72 | 100.07 | 0.5832 | 862.0 | 806.3 | |
| 13.95 | -2.00 | 8.58 | -2.00 | -14.19 | 170.29 | -36.20 | 104.54 | 0.5938 | 810.9 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -11.20 | 170.71 | -35.78 | 99.54 | 0.5838 | 679.0 | 590.3 | |
| 0.00 | 1.48 | 0.00 | 0.91 | -11.33 | 170.43 | -36.07 | 99.73 | 0.5879 | 677.0 | 662.4 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -15.31 | 169.38 | -37.12 | 106.18 | 0.6083 | -708.0 | -605.4 | |
| 23.90 | 108.92 | 14.89 | 67.91 | -12.58 | 168.97 | -37.53 | 101.63 | 0.6093 | 1110.6 | 384.4 | |
| 0.00 | 1.13 | 0.00 | 0.71 | -14.15 | 168.52 | -37.98 | 104.12 | 0.6175 | 595.0 | 469.5 | |
| 1.22 | 2.27 | 0.77 | 1.43 | -13.77 | 168.24 | -38.25 | 103.45 | 0.6206 | 581.6 | 385.2 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -13.57 | 168.00 | -38.49 | 103.09 | 0.6234 | 476.0 | 364.6 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -13.17 | 167.92 | -38.57 | 102.44 | 0.6240 | 523.0 | 355.5 | |
| 0.00 | 2.97 | 0.00 | 1.88 | -12.96 | 167.61 | -38.89 | 102.06 | 0.6279 | 617.0 | 459.1 | |
| 0.00 | 2.09 | 0.00 | 1.34 | -13.81 | 167.24 | -39.25 | 103.36 | 0.6338 | -788.0 | -573.8 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -15.28 | 166.93 | -39.57 | 105.59 | 0.6402 | 484.0 | 329.4 | |
| 0.00 | 2.35 | 0.00 | 1.52 | -12.47 | 166.23 | -40.27 | 101.11 | 0.6455 | 615.0 | 421.7 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -15.46 | 165.38 | -41.12 | 105.57 | 0.6603 | -652.0 | -466.6 | |
| 0.00 | 1.83 | 0.00 | 1.20 | -13.54 | 165.65 | -40.85 | 102.70 | 0.6541 | -852.0 | -647.2 | |
| 0.00 | 0.44 | 0.00 | 0.29 | -13.67 | 165.42 | -41.08 | 102.87 | 0.6572 | -905.0 | -812.4 | |
| 0.00 | 1.40 | 0.00 | 0.92 | -13.72 | 165.24 | -41.25 | 102.92 | 0.6595 | -648.0 | -603.0 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -9.78 | 165.07 | -41.42 | 96.92 | 0.6591 | 597.0 | 489.1 | |
| 0.00 | 0.44 | 0.00 | 0.29 | -9.06 | 163.96 | -42.54 | 95.83 | 0.6734 | 668.0 | 567.2 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -10.01 | 163.77 | -42.73 | 97.23 | 0.6759 | 665.0 | 530.5 | |
| 0.00 | 1.92 | 0.00 | 1.28 | -8.30 | 163.90 | -42.59 | 94.70 | 0.6743 | 621.0 | 440.5 | |
| 0.00 | 1.57 | 0.00 | 1.06 | -11.80 | 163.23 | -43.26 | 99.86 | 0.6832 | -577.0 | -495.7 | |
| 0.00 | 1.22 | 0.00 | 0.83 | -11.70 | 163.04 | -43.45 | 99.69 | 0.6856 | -469.0 | -374.1 | |
| 0.00 | 1.22 | 0.00 | 0.83 | -10.08 | 162.84 | -43.66 | 97.33 | 0.6876 | 698.0 | 611.1 | |
| 0.00 | 1.13 | 0.00 | 0.84 | -19.14 | 158.60 | -47.90 | 109.53 | 0.7461 | -385.0 | -368.9 | |
| 0.00 | 1.31 | 0.00 | 0.94 | -12.35 | 159.69 | -46.81 | 100.44 | 0.7265 | -611.0 | -558.3 | |
| 0.00 | 1.57 | 0.00 | 1.16 | -11.48 | 158.16 | -48.34 | 99.21 | 0.7440 | -594.0 | -584.6 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -10.63 | 158.35 | -48.15 | 98.05 | 0.7417 | -660.0 | -615.8 | |
| 0.00 | 2.01 | 0.00 | 1.50 | -10.71 | 157.64 | -48.86 | 98.16 | 0.7498 | -544.0 | -508.5 | |
| 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. | |