SDO HMI 2011-05-29 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.39 | 300.81 | 44.37 | 203.31 | 20.82 | 131.63 | 37.57 | 302.91 | 0.6803 | -190.7 | -160.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.69 | 16.43 | 135.53 | 41.47 | 294.94 | 0.7028 | 520.0 | 424.2 | |
| 4.33 | 9.11 | 2.98 | 6.26 | 20.23 | 133.31 | 39.26 | 301.12 | 0.6959 | -731.5 | -496.4 | |
| 1.26 | 199.15 | 0.88 | 137.70 | 21.91 | 133.77 | 39.71 | 303.04 | 0.7094 | -511.6 | -352.8 | |
| 4.96 | -3.00 | 3.47 | -3.00 | 22.14 | 133.54 | 39.49 | 303.46 | 0.7083 | -770.1 | 999999 | |
| 22.65 | -3.00 | 15.69 | -3.00 | 21.54 | 133.18 | 39.12 | 302.90 | 0.7013 | -825.2 | 999999 | |
| 5.41 | -3.00 | 3.72 | -3.00 | 21.04 | 132.77 | 38.71 | 302.49 | 0.6943 | -894.0 | 999999 | |
| 4.60 | -3.00 | 3.15 | -3.00 | 21.33 | 132.44 | 38.38 | 303.07 | 0.6924 | -1031.0 | 999999 | |
| 3.88 | -3.00 | 2.63 | -3.00 | 20.67 | 132.03 | 37.97 | 302.44 | 0.6844 | -948.9 | 999999 | |
| 0.54 | -3.00 | 0.37 | -3.00 | 21.26 | 132.13 | 38.07 | 303.16 | 0.6887 | -907.0 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.52 | 20.05 | 131.73 | 37.67 | 301.79 | 0.6777 | -268.0 | -244.8 | |
| 0.00 | 0.99 | 0.00 | 0.66 | 18.97 | 131.15 | 37.09 | 300.67 | 0.6654 | 569.0 | 389.5 | |
| 0.00 | 1.62 | 0.00 | 1.07 | 18.93 | 130.54 | 36.48 | 300.99 | 0.6583 | 481.0 | 364.8 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 19.65 | 130.56 | 36.50 | 301.95 | 0.6626 | 260.0 | 212.7 | |
| 0.00 | 3.88 | 0.00 | 2.54 | 18.83 | 130.31 | 36.25 | 300.99 | 0.6552 | 479.0 | 545.4 | |
| 1.26 | 1.99 | 0.82 | 1.29 | 18.60 | 129.94 | 35.88 | 300.90 | 0.6496 | 723.4 | 768.4 | |
| 5.50 | 20.48 | 3.59 | 13.36 | 19.25 | 129.90 | 35.84 | 301.82 | 0.6529 | 661.2 | 109.1 | |
| 0.00 | 1.53 | 0.00 | 0.99 | 18.47 | 129.63 | 35.57 | 300.91 | 0.6453 | 746.0 | 648.6 | |
| 0.00 | 1.17 | 0.00 | 0.77 | 19.54 | 129.77 | 35.72 | 302.30 | 0.6531 | 409.0 | 286.8 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 14.38 | 128.51 | 34.45 | 295.58 | 0.6097 | -675.0 | -603.9 | |
| 4.06 | -16.00 | 2.64 | -16.00 | 19.34 | 129.52 | 35.47 | 302.19 | 0.6492 | 726.1 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 19.11 | 129.11 | 35.05 | 302.14 | 0.6431 | 779.0 | 591.6 | |
| 0.00 | 1.71 | 0.00 | 1.11 | 19.34 | 129.13 | 35.07 | 302.44 | 0.6447 | 934.0 | 698.3 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 19.59 | 128.01 | 33.96 | 303.54 | 0.6336 | 703.0 | 554.6 | |
| 0.00 | 0.81 | 0.00 | 0.51 | 17.16 | 127.40 | 33.34 | 300.48 | 0.6115 | -577.0 | -498.7 | |
| 0.00 | 1.53 | 0.00 | 0.99 | 20.96 | 128.20 | 34.14 | 305.30 | 0.6445 | 650.0 | 554.5 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 20.27 | 127.91 | 33.85 | 304.57 | 0.6368 | 585.0 | 495.1 | |
| 1.44 | 3.88 | 0.92 | 2.48 | 20.33 | 127.53 | 33.47 | 304.92 | 0.6330 | 797.6 | 650.0 | |
| 0.99 | 3.07 | 0.63 | 1.96 | 20.49 | 127.26 | 33.20 | 305.34 | 0.6311 | 784.9 | 747.5 | |
| 3.61 | 21.84 | 2.31 | 13.90 | 20.88 | 127.24 | 33.18 | 305.89 | 0.6335 | 787.0 | 684.1 | |
| 0.00 | 2.80 | 0.00 | 1.77 | 19.74 | 126.92 | 32.87 | 304.53 | 0.6223 | 700.0 | 532.9 | |
| 0.00 | 1.89 | 0.00 | 1.18 | 18.15 | 126.42 | 32.36 | 302.61 | 0.6061 | -151.0 | -73.5 | |
| 0.00 | 10.74 | 0.00 | 6.65 | 17.86 | 126.29 | 32.23 | 302.28 | 0.6026 | -503.0 | -506.1 | |
| 0.90 | -29.00 | 0.57 | -29.00 | 20.48 | 126.75 | 32.70 | 305.70 | 0.6254 | 838.0 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 18.21 | 126.21 | 32.15 | 302.86 | 0.6040 | 660.0 | 485.1 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 18.02 | 125.98 | 31.92 | 302.74 | 0.6000 | 533.0 | 404.2 | |
| 0.00 | 1.99 | 0.00 | 1.22 | 17.89 | 125.84 | 31.78 | 302.65 | 0.5975 | 664.0 | 523.1 | |
| 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. | |