SDO HMI 2014-09-10 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.12 | 182.53 | 22.72 | 109.16 | -15.85 | 66.29 | -25.19 | 132.99 | 0.5611 | 522.2 | 299.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.85 | 0.00 | 1.62 | -14.80 | 71.67 | -19.81 | 138.32 | 0.4949 | 29.0 | 90.0 | |
| 0.00 | 1.16 | 0.00 | 0.67 | -13.81 | 68.66 | -22.82 | 132.87 | 0.5160 | 727.0 | 520.8 | |
| 0.00 | 0.45 | 0.00 | 0.26 | -14.86 | 68.34 | -23.14 | 133.97 | 0.5300 | 785.0 | 644.8 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -15.76 | 67.89 | -23.59 | 134.67 | 0.5437 | 714.0 | 634.5 | |
| 0.27 | 155.27 | 0.16 | 92.31 | -15.70 | 67.31 | -24.17 | 133.89 | 0.5490 | 1081.7 | 392.0 | |
| 5.16 | -5.00 | 3.06 | -5.00 | -15.57 | 67.16 | -24.32 | 133.54 | 0.5495 | 1275.6 | 999999 | |
| 0.36 | -5.00 | 0.21 | -5.00 | -16.11 | 66.98 | -24.50 | 134.06 | 0.5565 | 648.2 | 999999 | |
| 6.50 | -5.00 | 3.86 | -5.00 | -15.85 | 66.92 | -24.57 | 133.63 | 0.5547 | 1020.4 | 999999 | |
| 0.71 | -5.00 | 0.42 | -5.00 | -16.12 | 66.74 | -24.74 | 133.79 | 0.5592 | 645.4 | 999999 | |
| 20.57 | -5.00 | 12.22 | -5.00 | -15.63 | 66.74 | -24.75 | 133.13 | 0.5545 | 1137.4 | 999999 | |
| 0.27 | -5.00 | 0.16 | -5.00 | -16.06 | 66.64 | -24.84 | 133.60 | 0.5596 | 589.7 | 999999 | |
| 1.25 | -5.00 | 0.74 | -5.00 | -15.69 | 66.21 | -25.27 | 132.61 | 0.5606 | 700.4 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.53 | -14.06 | 65.76 | -25.72 | 129.84 | 0.5504 | 760.0 | 605.2 | |
| 0.00 | 1.78 | 0.00 | 1.08 | -16.17 | 64.64 | -26.85 | 131.55 | 0.5818 | 523.0 | 413.4 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -15.94 | 64.67 | -26.81 | 131.28 | 0.5793 | 681.0 | 526.7 | |
| 0.00 | 1.96 | 0.00 | 1.19 | -15.75 | 64.63 | -26.85 | 130.97 | 0.5780 | 695.0 | 560.4 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -15.29 | 62.53 | -28.95 | 128.25 | 0.5968 | -477.0 | -417.9 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -21.11 | 61.17 | -30.31 | 134.26 | 0.6597 | 679.0 | 526.8 | |
| 0.00 | 1.16 | 0.00 | 0.73 | -17.07 | 61.84 | -29.64 | 129.95 | 0.6190 | -676.0 | -562.6 | |
| 0.00 | 1.25 | 0.00 | 0.78 | -16.25 | 61.84 | -29.64 | 128.88 | 0.6122 | -757.0 | -594.6 | |
| 3.03 | 4.90 | 1.89 | 3.06 | -16.03 | 61.69 | -29.79 | 128.45 | 0.6119 | -982.0 | -752.6 | |
| 0.00 | 1.25 | 0.00 | 0.80 | -18.08 | 61.10 | -30.38 | 130.55 | 0.6350 | -801.0 | -635.3 | |
| 0.00 | 1.25 | 0.00 | 0.78 | -16.15 | 61.42 | -30.06 | 128.35 | 0.6158 | -667.0 | -537.8 | |
| 0.00 | 1.51 | 0.00 | 0.97 | -17.86 | 60.45 | -31.04 | 129.68 | 0.6399 | -774.0 | -539.6 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -19.68 | 59.69 | -31.79 | 131.25 | 0.6621 | -683.0 | -597.0 | |
| 0.00 | 2.23 | 0.00 | 1.45 | -18.43 | 59.47 | -32.01 | 129.53 | 0.6543 | -779.0 | -622.9 | |
| 0.00 | 0.80 | 0.00 | 0.52 | -18.05 | 59.10 | -32.38 | 128.75 | 0.6552 | -668.0 | -612.2 | |
| 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. | |