SDO HMI 2011-11-13 07:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.89 | 293.23 | 24.05 | 160.76 | 28.11 | 42.88 | 3.79 | 352.13 | 0.4300 | -770.7 | -397.8 | |
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back to the solar disc SDO HMI 2011-11-13 07:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.12 | 280.41 | 0.61 | 153.68 | 27.92 | 44.04 | 4.95 | 349.71 | 0.4289 | -817.8 | -437.7 | |
| 36.49 | -1.00 | 19.99 | -1.00 | 28.02 | 43.30 | 4.21 | 351.26 | 0.4285 | -1335.2 | 999999 | |
| 5.25 | -1.00 | 2.88 | -1.00 | 28.45 | 42.95 | 3.86 | 352.14 | 0.4344 | -878.0 | 999999 | |
| 1.03 | -1.00 | 0.57 | -1.00 | 28.18 | 42.63 | 3.54 | 352.68 | 0.4296 | -873.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 29.91 | 40.60 | 1.51 | 357.09 | 0.4538 | -663.0 | -541.3 | |
| 0.00 | 1.29 | 0.00 | 0.71 | 28.91 | 40.32 | 1.23 | 357.53 | 0.4380 | -804.0 | -700.7 | |
| 0.00 | 1.46 | 0.00 | 0.80 | 28.12 | 37.45 | -1.64 | 3.41 | 0.4258 | 608.0 | 497.5 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 27.14 | 36.40 | -2.69 | 5.85 | 0.4116 | 685.0 | 579.0 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 25.65 | 36.43 | -2.66 | 6.21 | 0.3878 | 670.0 | 555.2 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 28.05 | 34.76 | -4.33 | 8.97 | 0.4293 | 664.0 | 493.3 | |
| 0.00 | 1.12 | 0.00 | 0.64 | 31.91 | 33.00 | -6.08 | 10.57 | 0.4927 | 796.0 | 695.9 | |
| 0.00 | 2.07 | 0.00 | 1.14 | 28.86 | 32.00 | -7.09 | 13.95 | 0.4503 | 777.0 | 522.7 | |
| 0.00 | 1.29 | 0.00 | 0.74 | 31.26 | 27.95 | -11.13 | 19.24 | 0.5031 | 610.0 | 493.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 28.39 | 27.59 | -11.50 | 22.26 | 0.4649 | 631.0 | 547.4 | |
| 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. | |