SDO HMI 2014-03-18 23:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.27 | 182.35 | 39.31 | 117.98 | -10.92 | 296.16 | 40.24 | 261.37 | 0.6425 | -101.4 | -118.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.66 | -9.75 | 310.24 | 54.32 | 263.08 | 0.8087 | 330.0 | 273.6 | |
| 0.00 | 3.05 | 0.00 | 2.54 | -9.54 | 309.98 | 54.06 | 263.36 | 0.8061 | 478.0 | 435.4 | |
| 0.00 | 2.09 | 0.00 | 1.73 | -9.71 | 309.76 | 53.84 | 263.15 | 0.8038 | 486.0 | 454.1 | |
| 0.00 | 0.96 | 0.00 | 0.74 | -11.16 | 306.28 | 50.36 | 261.36 | 0.7665 | 435.0 | 362.9 | |
| 0.00 | 1.22 | 0.00 | 0.93 | -10.72 | 306.13 | 50.21 | 261.94 | 0.7648 | 611.0 | 537.1 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -8.18 | 298.42 | 42.50 | 265.64 | 0.6730 | -481.0 | -507.4 | |
| 0.00 | 0.87 | 0.00 | 0.58 | -8.52 | 298.34 | 42.42 | 265.14 | 0.6719 | -542.0 | -465.7 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -10.76 | 298.44 | 42.52 | 261.79 | 0.6732 | 284.0 | 247.4 | |
| 0.00 | 2.00 | 0.00 | 1.33 | -10.03 | 298.24 | 42.32 | 262.88 | 0.6704 | 531.0 | 426.9 | |
| 4.18 | 8.18 | 2.77 | 5.42 | -10.29 | 297.99 | 42.07 | 262.48 | 0.6673 | 656.7 | 618.3 | |
| 0.00 | 1.22 | 0.00 | 0.81 | -10.05 | 297.91 | 41.99 | 262.83 | 0.6663 | 482.0 | 453.6 | |
| 13.14 | 18.89 | 8.72 | 12.53 | -11.00 | 298.03 | 42.11 | 261.40 | 0.6680 | 721.5 | 505.2 | |
| 0.00 | 0.44 | 0.00 | 0.29 | -9.86 | 297.72 | 41.80 | 263.13 | 0.6638 | 528.0 | 498.6 | |
| 0.00 | 1.13 | 0.00 | 0.75 | -10.61 | 297.76 | 41.84 | 262.00 | 0.6644 | 677.0 | 676.8 | |
| 7.05 | 10.79 | 4.64 | 7.09 | -10.03 | 297.42 | 41.50 | 262.86 | 0.6599 | 863.0 | 644.3 | |
| 0.00 | 6.96 | 0.00 | 4.58 | -10.69 | 297.41 | 41.49 | 261.85 | 0.6599 | 684.0 | 687.8 | |
| 0.61 | 1.83 | 0.40 | 1.19 | -10.37 | 296.99 | 41.07 | 262.34 | 0.6544 | 672.3 | 550.7 | |
| 0.00 | 1.22 | 0.00 | 0.79 | -9.87 | 296.83 | 40.91 | 263.10 | 0.6522 | 559.0 | 472.1 | |
| 0.00 | 1.13 | 0.00 | 0.73 | -10.81 | 296.34 | 40.41 | 261.63 | 0.6460 | 703.0 | 605.4 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -10.92 | 295.68 | 39.76 | 261.42 | 0.6373 | -404.0 | -308.9 | |
| 0.00 | 1.04 | 0.00 | 0.67 | -11.26 | 295.61 | 39.69 | 260.89 | 0.6367 | -150.0 | -196.7 | |
| 0.00 | 1.22 | 0.00 | 0.78 | -11.22 | 295.29 | 39.37 | 260.92 | 0.6324 | -463.0 | -420.1 | |
| 0.00 | 4.44 | 0.00 | 2.83 | -10.68 | 295.21 | 39.28 | 261.76 | 0.6310 | -648.0 | -378.1 | |
| 1.74 | 100.01 | 1.10 | 62.82 | -10.60 | 294.68 | 38.76 | 261.87 | 0.6239 | -477.5 | -448.4 | |
| 0.00 | 3.92 | 0.00 | 2.48 | -11.61 | 294.84 | 38.92 | 260.26 | 0.6267 | -397.0 | -365.7 | |
| 0.00 | 1.22 | 0.00 | 0.77 | -9.88 | 294.35 | 38.43 | 263.02 | 0.6191 | -633.0 | -504.1 | |
| 4.18 | -24.00 | 2.63 | -24.00 | -10.77 | 294.44 | 38.52 | 261.58 | 0.6207 | -701.1 | 999999 | |
| 4.87 | -24.00 | 3.08 | -24.00 | -11.70 | 294.50 | 38.58 | 260.09 | 0.6222 | -721.7 | 999999 | |
| 0.78 | -24.00 | 0.49 | -24.00 | -11.54 | 294.28 | 38.36 | 260.33 | 0.6191 | -766.2 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.78 | -14.91 | 294.87 | 38.95 | 255.03 | 0.6312 | -548.0 | -518.8 | |
| 0.00 | 1.39 | 0.00 | 0.89 | -14.61 | 294.81 | 38.89 | 255.49 | 0.6298 | -584.0 | -513.7 | |
| 0.00 | 0.52 | 0.00 | 0.33 | -15.96 | 294.99 | 39.07 | 253.40 | 0.6346 | -530.0 | -394.8 | |
| 13.49 | -24.00 | 8.45 | -24.00 | -10.87 | 293.95 | 38.03 | 261.39 | 0.6141 | -941.9 | 999999 | |
| 11.23 | -24.00 | 7.03 | -24.00 | -11.32 | 293.94 | 38.02 | 260.65 | 0.6143 | -869.1 | 999999 | |
| 0.00 | 1.65 | 0.00 | 1.03 | -11.70 | 293.65 | 37.73 | 260.00 | 0.6107 | -752.0 | -580.8 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -11.63 | 292.95 | 37.03 | 260.04 | 0.6011 | -737.0 | -686.0 | |
| 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. | |