SDO HMI 2011-02-25 21:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.62 | 43.02 | 7.55 | 49.94 | 16.57 | 178.19 | -60.87 | 67.83 | 0.9055 | 57.2 | 126.1 | |
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back to the solar disc SDO HMI 2011-02-25 21:58:58 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 |
| 0.52 | 2.07 | 0.58 | 2.30 | 17.18 | 179.57 | -59.49 | 66.75 | 0.8977 | -303.3 | -247.2 | |
| 0.00 | 0.86 | 0.00 | 1.01 | 18.76 | 178.42 | -60.64 | 65.45 | 0.9091 | -471.0 | -448.8 | |
| 1.98 | 16.35 | 2.16 | 17.88 | 15.42 | 179.72 | -59.34 | 68.59 | 0.8926 | 794.0 | 530.8 | |
| 1.20 | 1.89 | 1.34 | 2.10 | 16.10 | 179.33 | -59.73 | 67.99 | 0.8969 | 423.0 | 417.4 | |
| 0.34 | -3.00 | 0.38 | -3.00 | 15.61 | 179.44 | -59.61 | 68.48 | 0.8950 | 661.8 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.92 | 15.61 | 179.13 | -59.92 | 68.57 | 0.8972 | 222.0 | 155.6 | |
| 1.98 | 7.57 | 2.33 | 8.98 | 17.37 | 177.95 | -61.11 | 67.06 | 0.9092 | -519.8 | -297.6 | |
| 0.00 | 1.03 | 0.00 | 1.31 | 18.83 | 176.44 | -62.61 | 65.98 | 0.9218 | -232.0 | -230.8 | |
| 0.00 | 2.07 | 0.00 | 2.41 | 16.29 | 177.90 | -61.16 | 68.22 | 0.9073 | 292.0 | 293.7 | |
| 0.60 | 2.15 | 0.76 | 2.72 | 18.61 | 176.38 | -62.67 | 66.23 | 0.9217 | -407.0 | -292.1 | |
| 0.00 | 1.12 | 0.00 | 1.30 | 15.97 | 177.87 | -61.19 | 68.56 | 0.9068 | 577.0 | 551.4 | |
| 0.00 | 0.60 | 0.00 | 0.76 | 16.91 | 175.80 | -63.26 | 68.17 | 0.9221 | -495.0 | -468.7 | |
| 0.00 | 4.82 | 0.00 | 6.26 | 17.26 | 175.23 | -63.83 | 67.96 | 0.9263 | -188.0 | -80.4 | |
| 0.00 | 0.77 | 0.00 | 0.99 | 16.38 | 175.42 | -63.64 | 68.83 | 0.9235 | -257.0 | -247.7 | |
| 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. | |