SDO HMI 2011-05-07 06:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.01 | 365.84 | 44.05 | 204.36 | 16.55 | 49.10 | 18.55 | 318.51 | 0.4606 | -327.0 | -149.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.53 | 19.09 | 55.29 | 24.74 | 313.83 | 0.5504 | 708.0 | 538.7 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 16.71 | 52.36 | 21.81 | 313.88 | 0.4956 | 385.0 | 358.1 | |
| 0.00 | 2.59 | 0.00 | 1.48 | 16.83 | 52.07 | 21.52 | 314.44 | 0.4937 | -156.0 | -96.0 | |
| 6.26 | 248.93 | 3.54 | 140.27 | 16.30 | 51.50 | 20.95 | 314.38 | 0.4820 | -994.8 | -380.0 | |
| 1.61 | -4.00 | 0.91 | -4.00 | 16.53 | 51.39 | 20.84 | 314.87 | 0.4831 | -721.4 | 999999 | |
| 0.45 | -4.00 | 0.25 | -4.00 | 16.65 | 51.20 | 20.65 | 315.32 | 0.4824 | -399.8 | 999999 | |
| 29.71 | -4.00 | 16.71 | -4.00 | 16.29 | 50.92 | 20.37 | 315.14 | 0.4756 | -1183.6 | 999999 | |
| 0.89 | -4.00 | 0.50 | -4.00 | 16.00 | 50.66 | 20.11 | 315.05 | 0.4696 | -1054.6 | 999999 | |
| 12.17 | -4.00 | 6.85 | -4.00 | 16.70 | 50.63 | 20.08 | 316.18 | 0.4769 | -917.4 | 999999 | |
| 4.74 | -4.00 | 2.65 | -4.00 | 16.24 | 50.15 | 19.60 | 316.15 | 0.4667 | -1076.0 | 999999 | |
| 0.00 | 1.79 | 0.00 | 1.00 | 15.56 | 49.88 | 19.33 | 315.47 | 0.4565 | -745.0 | -674.0 | |
| 0.00 | 1.34 | 0.00 | 0.75 | 15.91 | 49.61 | 19.06 | 316.41 | 0.4574 | -510.0 | -476.9 | |
| 2.24 | 2.68 | 1.24 | 1.49 | 15.52 | 49.51 | 18.96 | 315.95 | 0.4521 | -983.3 | -888.0 | |
| 0.00 | 1.43 | 0.00 | 0.80 | 16.26 | 49.55 | 19.00 | 317.06 | 0.4606 | -860.0 | -687.6 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 18.10 | 49.34 | 18.79 | 320.08 | 0.4790 | -648.0 | -531.5 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 15.67 | 48.99 | 18.44 | 316.97 | 0.4482 | -920.0 | -719.9 | |
| 0.00 | 1.25 | 0.00 | 0.70 | 16.54 | 48.78 | 18.23 | 318.64 | 0.4556 | -848.0 | -695.4 | |
| 0.00 | 1.34 | 0.00 | 0.76 | 18.93 | 48.32 | 17.77 | 322.74 | 0.4789 | -766.0 | -517.3 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 19.88 | 48.23 | 17.68 | 324.13 | 0.4893 | -554.0 | -415.2 | |
| 1.43 | 3.13 | 0.81 | 1.76 | 18.92 | 48.09 | 17.54 | 323.10 | 0.4767 | -965.1 | -774.5 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 19.22 | 48.02 | 17.47 | 323.59 | 0.4795 | -759.0 | -639.0 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 18.89 | 47.88 | 17.33 | 323.37 | 0.4743 | -815.0 | -649.9 | |
| 0.00 | 1.16 | 0.00 | 0.66 | 19.34 | 47.83 | 17.28 | 324.05 | 0.4794 | -740.0 | -526.2 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 18.71 | 47.43 | 16.88 | 323.85 | 0.4681 | -731.0 | -553.3 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 17.89 | 44.94 | 14.39 | 326.97 | 0.4356 | 675.0 | 573.4 | |
| 0.00 | 2.24 | 0.00 | 1.21 | 16.08 | 44.66 | 14.11 | 324.96 | 0.4098 | 874.0 | 649.2 | |
| 0.00 | 2.06 | 0.00 | 1.12 | 17.07 | 44.58 | 14.03 | 326.54 | 0.4219 | 614.0 | 503.2 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 17.68 | 44.13 | 13.58 | 328.18 | 0.4261 | 795.0 | 594.5 | |
| 19.51 | 72.57 | 10.59 | 39.43 | 16.55 | 44.02 | 13.47 | 326.87 | 0.4102 | 1160.4 | 567.9 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 17.84 | 44.08 | 13.53 | 328.48 | 0.4278 | 882.0 | 737.7 | |
| 0.00 | 3.13 | 0.00 | 1.72 | 18.07 | 44.07 | 13.52 | 328.80 | 0.4307 | 890.0 | 759.2 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.45 | 43.86 | 13.30 | 328.40 | 0.4207 | 746.0 | 563.7 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 17.16 | 43.70 | 13.15 | 328.30 | 0.4156 | 828.0 | 640.4 | |
| 0.00 | 2.06 | 0.00 | 1.12 | 17.02 | 43.21 | 12.66 | 329.10 | 0.4096 | 737.0 | 759.4 | |
| 0.00 | 1.34 | 0.00 | 0.73 | 17.83 | 43.17 | 12.62 | 330.21 | 0.4203 | 709.0 | 552.1 | |
| 0.00 | 2.15 | 0.00 | 1.18 | 19.35 | 42.00 | 11.45 | 334.23 | 0.4327 | 808.0 | 600.8 | |
| 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. | |