SDO HMI 2011-08-21 09:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.67 | 256.06 | 29.17 | 147.28 | -21.07 | 54.27 | -12.26 | 157.15 | 0.5097 | 34.0 | -46.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.89 | 0.00 | 1.04 | -18.59 | 62.28 | -4.26 | 170.71 | 0.4375 | 726.0 | 585.1 | |
| 0.00 | 3.69 | 0.00 | 2.03 | -18.46 | 61.51 | -5.02 | 169.02 | 0.4376 | 745.0 | 561.4 | |
| 0.00 | 1.89 | 0.00 | 1.02 | -15.52 | 60.39 | -6.15 | 164.84 | 0.3961 | 453.0 | 368.9 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -17.07 | 58.90 | -7.63 | 162.59 | 0.4263 | 837.0 | 712.9 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -17.54 | 58.30 | -8.23 | 161.69 | 0.4363 | 830.0 | 623.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -18.22 | 57.82 | -8.72 | 161.21 | 0.4488 | 730.0 | 487.5 | |
| 0.00 | 1.98 | 0.00 | 1.09 | -17.29 | 57.61 | -8.93 | 160.05 | 0.4361 | 782.0 | 687.2 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.46 | 57.31 | -9.23 | 159.59 | 0.4403 | 917.0 | 752.0 | |
| 2.16 | 80.70 | 1.24 | 46.16 | -21.68 | 56.86 | -9.67 | 161.86 | 0.5036 | 698.1 | 439.2 | |
| 12.33 | -9.00 | 7.05 | -9.00 | -21.44 | 56.54 | -9.99 | 161.15 | 0.5017 | 1187.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.02 | 56.44 | -10.09 | 159.17 | 0.4677 | 259.0 | 339.0 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -19.16 | 56.11 | -10.43 | 158.65 | 0.4715 | 656.0 | 472.1 | |
| 1.80 | 2.52 | 1.04 | 1.45 | -21.84 | 55.82 | -10.71 | 160.18 | 0.5109 | 705.7 | 584.6 | |
| 1.98 | 16.46 | 1.13 | 9.40 | -20.39 | 54.70 | -11.83 | 157.15 | 0.4968 | 898.4 | 641.8 | |
| 4.05 | -14.00 | 2.31 | -14.00 | -20.66 | 54.65 | -11.88 | 157.28 | 0.5009 | 807.8 | 999999 | |
| 1.44 | -14.00 | 0.82 | -14.00 | -20.53 | 54.49 | -12.04 | 156.91 | 0.5000 | 708.3 | 999999 | |
| 3.69 | 4.59 | 2.12 | 2.64 | -21.05 | 54.39 | -12.15 | 157.15 | 0.5078 | 708.9 | 454.3 | |
| 0.00 | 2.70 | 0.00 | 1.55 | -21.16 | 54.08 | -12.46 | 156.73 | 0.5111 | 629.0 | 497.3 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -20.48 | 53.74 | -12.80 | 155.58 | 0.5039 | 39.0 | 71.7 | |
| 0.00 | 2.70 | 0.00 | 1.55 | -20.86 | 53.67 | -12.86 | 155.80 | 0.5095 | -715.0 | -507.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -20.67 | 53.15 | -13.38 | 154.78 | 0.5102 | -612.0 | -393.0 | |
| 1.89 | 111.02 | 1.10 | 64.35 | -21.40 | 52.95 | -13.58 | 155.09 | 0.5212 | -762.0 | -529.0 | |
| 0.00 | 3.69 | 0.00 | 2.12 | -20.41 | 52.84 | -13.69 | 154.04 | 0.5086 | 312.0 | 136.6 | |
| 5.76 | -22.00 | 3.33 | -22.00 | -21.20 | 52.70 | -13.83 | 154.52 | 0.5201 | -921.1 | 999999 | |
| 3.87 | -22.00 | 2.25 | -22.00 | -21.35 | 52.28 | -14.25 | 153.99 | 0.5248 | -925.5 | 999999 | |
| 9.18 | -22.00 | 5.32 | -22.00 | -20.98 | 52.15 | -14.38 | 153.45 | 0.5207 | -1219.5 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -21.84 | 51.93 | -14.60 | 153.88 | 0.5336 | -516.0 | -403.9 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -23.03 | 51.80 | -14.73 | 154.71 | 0.5499 | -643.0 | -482.6 | |
| 0.00 | 3.24 | 0.00 | 1.90 | -22.33 | 51.81 | -14.72 | 154.13 | 0.5407 | -611.0 | -545.3 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -22.06 | 51.64 | -14.90 | 153.62 | 0.5383 | -541.0 | -485.2 | |
| 2.52 | -22.00 | 1.46 | -22.00 | -21.00 | 51.55 | -14.98 | 152.51 | 0.5251 | -1007.6 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -20.45 | 51.43 | -15.10 | 151.82 | 0.5188 | -777.0 | -524.1 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -22.01 | 50.96 | -15.57 | 152.57 | 0.5422 | -649.0 | -519.8 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -24.79 | 48.98 | -17.55 | 152.24 | 0.5900 | -631.0 | -510.5 | |
| 0.00 | 1.08 | 0.00 | 0.66 | -24.76 | 48.85 | -17.69 | 152.04 | 0.5905 | -596.0 | -532.2 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -24.49 | 48.46 | -18.07 | 151.30 | 0.5898 | -810.0 | -619.8 | |
| 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. | |