SDO HMI 2014-03-03 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.77 | 94.64 | 13.84 | 77.65 | 13.12 | 50.03 | -49.07 | 67.44 | 0.7986 | -5.7 | -22.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 6.13 | 0.00 | 4.72 | 12.74 | 53.07 | -46.03 | 66.59 | 0.7673 | -795.0 | -668.5 | |
| 0.00 | 1.38 | 0.00 | 1.06 | 12.51 | 52.86 | -46.24 | 66.96 | 0.7685 | -706.0 | -638.0 | |
| 0.00 | 2.59 | 0.00 | 2.01 | 12.62 | 52.66 | -46.44 | 66.92 | 0.7710 | -760.0 | -590.5 | |
| 2.94 | 9.15 | 2.31 | 7.24 | 13.62 | 52.14 | -46.96 | 65.95 | 0.7801 | -752.0 | -612.6 | |
| 0.00 | 1.73 | 0.00 | 1.35 | 12.69 | 52.33 | -46.77 | 66.99 | 0.7746 | -562.0 | -395.1 | |
| 0.00 | 0.95 | 0.00 | 0.74 | 12.67 | 52.15 | -46.95 | 67.08 | 0.7763 | -575.0 | -557.3 | |
| 0.00 | 0.95 | 0.00 | 0.75 | 12.72 | 51.96 | -47.14 | 67.11 | 0.7784 | -494.0 | -450.2 | |
| 2.85 | 4.58 | 2.26 | 3.62 | 12.88 | 51.65 | -47.45 | 67.05 | 0.7821 | -525.7 | -358.9 | |
| 0.00 | 0.95 | 0.00 | 0.76 | 13.69 | 51.35 | -47.75 | 66.21 | 0.7882 | -454.0 | -405.9 | |
| 0.00 | 1.64 | 0.00 | 1.31 | 13.12 | 51.46 | -47.64 | 66.85 | 0.7850 | -687.0 | -530.9 | |
| 0.00 | 1.90 | 0.00 | 1.50 | 12.26 | 51.58 | -47.52 | 67.83 | 0.7806 | -468.0 | -367.4 | |
| 0.78 | 2.07 | 0.62 | 1.66 | 13.29 | 51.27 | -47.83 | 66.72 | 0.7875 | -577.6 | -489.4 | |
| 0.00 | 1.64 | 0.00 | 1.31 | 13.05 | 51.20 | -47.90 | 67.05 | 0.7873 | -475.0 | -400.9 | |
| 0.00 | 0.86 | 0.00 | 0.69 | 12.54 | 51.24 | -47.87 | 67.64 | 0.7850 | -298.0 | -264.2 | |
| 0.00 | 1.21 | 0.00 | 0.97 | 13.16 | 50.99 | -48.11 | 67.00 | 0.7898 | -423.0 | -343.9 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 13.97 | 50.77 | -48.33 | 66.14 | 0.7950 | -293.0 | -235.9 | |
| 0.00 | 1.73 | 0.00 | 1.38 | 12.84 | 51.02 | -48.08 | 67.36 | 0.7883 | -414.0 | -299.5 | |
| 0.00 | 1.73 | 0.00 | 1.39 | 13.37 | 50.84 | -48.26 | 66.82 | 0.7920 | -463.0 | -346.5 | |
| 1.90 | 9.41 | 1.55 | 7.68 | 13.34 | 50.48 | -48.62 | 67.01 | 0.7954 | -538.5 | -315.6 | |
| 0.00 | 3.20 | 0.00 | 2.65 | 13.89 | 49.71 | -49.39 | 66.68 | 0.8047 | 262.0 | 311.2 | |
| 0.00 | 2.07 | 0.00 | 1.75 | 13.91 | 48.85 | -50.25 | 67.01 | 0.8129 | 621.0 | 563.8 | |
| 0.00 | 1.12 | 0.00 | 0.96 | 14.26 | 48.55 | -50.55 | 66.73 | 0.8169 | 346.0 | 320.5 | |
| 0.00 | 2.42 | 0.00 | 2.06 | 14.07 | 48.56 | -50.54 | 66.95 | 0.8161 | 645.0 | 569.8 | |
| 1.73 | 4.66 | 1.43 | 3.87 | 11.86 | 48.98 | -50.12 | 69.36 | 0.8047 | 741.7 | 584.7 | |
| 0.00 | 1.04 | 0.00 | 0.87 | 12.70 | 48.71 | -50.39 | 68.48 | 0.8101 | 644.0 | 592.2 | |
| 1.30 | 4.40 | 1.11 | 3.77 | 13.71 | 48.38 | -50.72 | 67.44 | 0.8166 | 751.5 | 681.1 | |
| 0.00 | 1.47 | 0.00 | 1.23 | 12.49 | 48.63 | -50.47 | 68.76 | 0.8102 | 615.0 | 520.9 | |
| 0.00 | 0.69 | 0.00 | 0.59 | 13.98 | 48.15 | -50.95 | 67.21 | 0.8196 | 386.0 | 335.2 | |
| 0.00 | 1.81 | 0.00 | 1.52 | 11.99 | 48.61 | -50.49 | 69.35 | 0.8087 | 603.0 | 538.7 | |
| 0.00 | 0.95 | 0.00 | 0.82 | 13.34 | 48.00 | -51.10 | 68.02 | 0.8189 | 436.0 | 419.9 | |
| 0.00 | 1.73 | 0.00 | 1.50 | 14.07 | 47.63 | -51.47 | 67.32 | 0.8246 | 432.0 | 404.6 | |
| 0.43 | 1.21 | 0.37 | 1.03 | 12.36 | 48.08 | -51.02 | 69.12 | 0.8149 | 606.8 | 500.6 | |
| 0.00 | 1.73 | 0.00 | 1.49 | 13.27 | 47.72 | -51.38 | 68.20 | 0.8212 | 612.0 | 545.0 | |
| 0.52 | 2.07 | 0.44 | 1.77 | 12.48 | 47.80 | -51.30 | 69.09 | 0.8179 | 476.3 | 458.1 | |
| 0.00 | 4.84 | 0.00 | 4.17 | 12.75 | 47.58 | -51.52 | 68.85 | 0.8209 | 632.0 | 525.5 | |
| 4.32 | 6.65 | 3.75 | 5.77 | 13.11 | 47.43 | -51.67 | 68.49 | 0.8234 | 441.1 | 269.1 | |
| 0.00 | 1.12 | 0.00 | 0.99 | 13.72 | 46.99 | -52.11 | 67.96 | 0.8293 | 434.0 | 312.2 | |
| 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. | |