SDO HMI 2011-11-14 09:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.92 | 143.14 | 65.79 | 468.00 | 19.11 | 106.31 | 81.50 | 288.89 | 0.9879 | -10.9 | -49.4 | |
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back to the solar disc SDO HMI 2011-11-14 09:58:58 UT
See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.34 | 70.62 | 32.15 | 283.26 | 19.09 | 107.99 | 83.18 | 288.87 | 0.9922 | 453.9 | 205.2 | |
| 6.02 | -1.00 | 21.62 | -1.00 | 19.12 | 107.30 | 82.49 | 288.90 | 0.9908 | -257.3 | 999999 | |
| 0.00 | 0.95 | 0.00 | 3.16 | 18.90 | 106.72 | 81.91 | 288.67 | 0.9894 | -477.0 | -442.0 | |
| 4.56 | 40.51 | 12.02 | 103.43 | 18.54 | 104.36 | 79.55 | 288.32 | 0.9830 | -539.7 | -389.8 | |
| 0.00 | 5.50 | 0.00 | 17.01 | 19.37 | 106.09 | 81.28 | 289.15 | 0.9878 | -390.0 | -330.9 | |
| 0.00 | 1.72 | 0.00 | 4.16 | 18.97 | 103.28 | 78.47 | 288.77 | 0.9796 | -503.0 | -490.9 | |
| 0.00 | 9.81 | 0.00 | 23.80 | 19.57 | 103.35 | 78.54 | 289.38 | 0.9798 | -493.0 | -424.8 | |
| 0.00 | 1.55 | 0.00 | 3.82 | 20.25 | 103.62 | 78.81 | 290.07 | 0.9808 | -505.0 | -463.1 | |
| 0.00 | 1.55 | 0.00 | 3.74 | 20.05 | 103.25 | 78.43 | 289.87 | 0.9795 | -432.0 | -448.1 | |
| 0.00 | 1.29 | 0.00 | 3.56 | 21.39 | 104.95 | 80.13 | 291.21 | 0.9848 | -330.0 | -305.9 | |
| 0.00 | 8.95 | 0.00 | 20.60 | 20.46 | 102.57 | 77.76 | 290.31 | 0.9773 | -354.0 | -374.0 | |
| 0.00 | 0.69 | 0.00 | 1.46 | 20.19 | 101.54 | 76.73 | 290.06 | 0.9735 | 126.0 | 53.9 | |
| 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. | |