SDO HMI 2011-12-12 12:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.58 | 32.01 | 12.81 | 65.22 | 21.26 | 299.50 | -74.65 | 67.88 | 0.9693 | -168.7 | 24.5 | |
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back to the solar disc SDO HMI 2011-12-12 12:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.92 | 4.68 | 6.24 | 7.46 | 19.98 | 303.64 | -70.51 | 68.74 | 0.9520 | -404.6 | -316.2 | |
| 0.00 | 2.13 | 0.00 | 3.55 | 20.18 | 302.84 | -71.31 | 68.64 | 0.9560 | -244.0 | -160.1 | |
| 0.00 | 0.94 | 0.00 | 1.52 | 19.77 | 303.29 | -70.86 | 69.01 | 0.9536 | -313.0 | -210.0 | |
| 0.00 | 1.02 | 0.00 | 1.73 | 19.87 | 302.48 | -71.67 | 69.00 | 0.9575 | -186.0 | -174.0 | |
| 3.66 | 6.47 | 6.57 | 11.63 | 20.38 | 301.47 | -72.68 | 68.59 | 0.9625 | -196.9 | -31.7 | |
| 0.00 | 1.53 | 0.00 | 2.47 | 18.76 | 303.25 | -70.90 | 70.06 | 0.9531 | -414.0 | -374.1 | |
| 0.00 | 1.62 | 0.00 | 3.03 | 20.68 | 300.77 | -73.37 | 68.36 | 0.9656 | 289.0 | 329.2 | |
| 0.00 | 1.53 | 0.00 | 2.78 | 19.98 | 301.20 | -72.94 | 69.04 | 0.9634 | -105.0 | -107.3 | |
| 0.00 | 6.56 | 0.00 | 18.57 | 23.49 | 295.43 | -78.71 | 66.01 | 0.9852 | 310.0 | 132.3 | |
| 0.00 | 1.87 | 0.00 | 3.35 | 19.60 | 301.44 | -72.71 | 69.41 | 0.9622 | -182.0 | -145.6 | |
| 0.00 | 0.85 | 0.00 | 1.56 | 19.76 | 301.03 | -73.12 | 69.28 | 0.9640 | 25.0 | -0.1 | |
| 0.00 | 1.02 | 0.00 | 2.21 | 21.46 | 298.58 | -75.56 | 67.79 | 0.9746 | 377.0 | 319.8 | |
| 0.00 | 1.79 | 0.00 | 5.36 | 22.33 | 294.72 | -79.43 | 67.23 | 0.9869 | 245.0 | 106.0 | |
| 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. | |