SDO HMI 2011-11-02 18:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 166.33 | 1213.53 | 275.91 | 2078.32 | 18.97 | 105.78 | -72.31 | 71.37 | 0.9493 | -145.5 | 92.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 9.08 | 0.75 | 13.11 | 22.52 | 108.03 | -70.05 | 67.56 | 0.9410 | 177.8 | -341.1 | |
| 0.86 | -1.00 | 1.23 | -1.00 | 22.18 | 108.31 | -69.77 | 67.90 | 0.9393 | 44.0 | 999999 | |
| 3.98 | -1.00 | 5.73 | -1.00 | 22.33 | 108.06 | -70.03 | 67.76 | 0.9407 | -440.2 | 999999 | |
| 20.57 | 933.11 | 26.33 | 1449.79 | 18.37 | 110.71 | -67.37 | 71.85 | 0.9235 | -985.9 | 79.7 | |
| 47.63 | -4.00 | 64.27 | -4.00 | 18.91 | 109.41 | -68.67 | 71.34 | 0.9318 | -580.2 | 999999 | |
| 5.45 | -4.00 | 7.57 | -4.00 | 18.92 | 108.69 | -69.40 | 71.36 | 0.9360 | 156.0 | 999999 | |
| 1.99 | 95.78 | 3.25 | 166.39 | 21.35 | 105.37 | -72.71 | 68.94 | 0.9543 | 235.9 | 351.9 | |
| 4.67 | -4.00 | 6.33 | -4.00 | 17.61 | 109.21 | -68.88 | 72.74 | 0.9326 | -461.1 | 999999 | |
| 8.82 | -4.00 | 12.58 | -4.00 | 18.44 | 108.12 | -69.96 | 71.89 | 0.9392 | -406.1 | 999999 | |
| 1.64 | -7.00 | 2.70 | -7.00 | 20.89 | 105.28 | -72.80 | 69.41 | 0.9547 | -266.0 | 999999 | |
| 7.09 | -4.00 | 10.33 | -4.00 | 18.07 | 107.62 | -70.46 | 72.31 | 0.9419 | -279.1 | 999999 | |
| 6.14 | -4.00 | 9.08 | -4.00 | 18.42 | 107.29 | -70.79 | 71.95 | 0.9438 | 204.8 | 999999 | |
| 0.00 | 13.14 | 0.00 | 17.98 | 16.42 | 108.94 | -69.14 | 74.03 | 0.9339 | -104.0 | -146.0 | |
| 0.00 | 1.38 | 0.00 | 2.43 | 20.71 | 103.93 | -74.15 | 69.66 | 0.9610 | 567.0 | 491.4 | |
| 0.00 | 1.04 | 0.00 | 1.86 | 20.59 | 103.62 | -74.47 | 69.79 | 0.9624 | 235.0 | 206.2 | |
| 0.35 | -4.00 | 0.58 | -4.00 | 19.68 | 104.67 | -73.41 | 70.70 | 0.9574 | -90.8 | 999999 | |
| 3.63 | -4.00 | 6.22 | -4.00 | 19.63 | 104.39 | -73.69 | 70.76 | 0.9587 | 253.5 | 999999 | |
| 2.07 | -4.00 | 4.24 | -4.00 | 21.26 | 101.43 | -76.65 | 69.13 | 0.9715 | 479.6 | 999999 | |
| 3.46 | -4.00 | 5.88 | -4.00 | 18.92 | 104.57 | -73.51 | 71.50 | 0.9578 | 750.7 | 999999 | |
| 0.00 | 1.73 | 0.00 | 4.04 | 22.16 | 99.63 | -78.46 | 68.23 | 0.9781 | 127.0 | 106.4 | |
| 4.58 | -4.00 | 7.45 | -4.00 | 17.82 | 105.36 | -72.73 | 72.64 | 0.9538 | 309.7 | 999999 | |
| 6.57 | -4.00 | 10.58 | -4.00 | 17.61 | 105.57 | -72.52 | 72.85 | 0.9527 | -369.8 | 999999 | |
| 1.38 | -4.00 | 2.32 | -4.00 | 18.12 | 104.71 | -73.38 | 72.34 | 0.9570 | 993.9 | 999999 | |
| 1.73 | 2.59 | 4.79 | 7.20 | 22.07 | 97.47 | -80.62 | 68.32 | 0.9847 | 344.8 | 380.3 | |
| 0.00 | 3.89 | 0.00 | 6.97 | 18.35 | 103.63 | -74.46 | 72.11 | 0.9621 | 507.0 | 453.6 | |
| 4.32 | -4.00 | 8.46 | -4.00 | 19.35 | 102.19 | -75.89 | 71.09 | 0.9684 | 481.9 | 999999 | |
| 0.00 | 1.38 | 0.00 | 2.80 | 18.84 | 101.58 | -76.50 | 71.63 | 0.9708 | 379.0 | 253.5 | |
| 0.00 | 2.16 | 0.00 | 3.97 | 17.23 | 103.16 | -74.92 | 73.29 | 0.9642 | 526.0 | 475.4 | |
| 2.42 | 8.64 | 4.83 | 17.30 | 18.22 | 101.77 | -76.31 | 72.26 | 0.9701 | 525.9 | 429.8 | |
| 12.71 | 132.09 | 30.95 | 367.37 | 19.29 | 99.03 | -79.05 | 71.17 | 0.9801 | 481.1 | -20.4 | |
| 0.00 | 1.04 | 0.00 | 2.47 | 18.51 | 99.23 | -78.85 | 71.96 | 0.9794 | 407.0 | 348.3 | |
| 0.00 | 4.58 | 0.00 | 10.70 | 18.25 | 99.52 | -78.57 | 72.23 | 0.9784 | 368.0 | 367.4 | |
| 0.00 | 1.90 | 0.00 | 3.94 | 17.04 | 101.32 | -76.76 | 73.49 | 0.9718 | 340.0 | 334.8 | |
| 7.35 | -30.00 | 20.58 | -30.00 | 19.20 | 97.36 | -80.72 | 71.24 | 0.9852 | 211.7 | 999999 | |
| 6.40 | -30.00 | 18.88 | -30.00 | 19.13 | 96.89 | -81.20 | 71.29 | 0.9865 | -409.2 | 999999 | |
| 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. | |