SDO HMI 2011-11-13 22:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.85 | 273.72 | 62.89 | 534.94 | 19.04 | 106.47 | 75.63 | 288.90 | 0.9685 | -237.2 | -176.8 | |
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back to the solar disc SDO HMI 2011-11-13 22:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.77 | 128.06 | 19.81 | 287.78 | 19.06 | 108.49 | 77.66 | 288.86 | 0.9767 | 359.0 | 61.5 | |
| 14.28 | -1.00 | 31.01 | -1.00 | 19.09 | 107.95 | 77.11 | 288.90 | 0.9747 | -475.6 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.69 | 18.91 | 106.47 | 75.63 | 288.76 | 0.9690 | -474.0 | -391.3 | |
| 0.00 | 5.07 | 0.00 | 9.86 | 19.33 | 106.27 | 75.43 | 289.19 | 0.9682 | -586.0 | -412.8 | |
| 2.24 | 109.65 | 4.07 | 186.40 | 18.57 | 105.17 | 74.33 | 288.44 | 0.9634 | -427.7 | -457.8 | |
| 4.56 | -5.00 | 8.00 | -5.00 | 18.54 | 104.55 | 73.71 | 288.43 | 0.9606 | -657.0 | 999999 | |
| 0.00 | 0.77 | 0.00 | 1.31 | 18.78 | 103.94 | 73.11 | 288.72 | 0.9578 | -602.0 | -600.7 | |
| 0.00 | 8.08 | 0.00 | 14.65 | 21.32 | 104.98 | 74.14 | 291.31 | 0.9631 | -503.0 | -378.7 | |
| 0.00 | 2.06 | 0.00 | 3.38 | 19.89 | 103.17 | 72.33 | 289.92 | 0.9543 | -619.0 | -525.3 | |
| 0.00 | 12.21 | 0.00 | 19.52 | 20.54 | 102.67 | 71.83 | 290.63 | 0.9521 | -323.0 | -311.3 | |
| 0.00 | 5.07 | 0.00 | 7.74 | 20.18 | 101.76 | 70.92 | 290.30 | 0.9473 | -89.0 | -44.6 | |
| 0.00 | 1.55 | 0.00 | 2.14 | 19.65 | 99.65 | 68.81 | 289.89 | 0.9354 | 481.0 | 414.3 | |
| 0.00 | 0.34 | 0.00 | 0.47 | 22.41 | 98.95 | 68.11 | 292.90 | 0.9328 | 300.0 | 291.5 | |
| 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. | |