SDO HMI 2011-02-13 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.05 | 22.28 | 2.94 | 12.68 | -20.06 | 70.21 | 27.06 | 240.15 | 0.4935 | 186.1 | 149.9 | |
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back to the solar disc SDO HMI 2011-02-13 10:58:57 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 |
| 0.00 | 2.91 | 0.00 | 1.69 | -20.10 | 72.75 | 29.60 | 242.12 | 0.5269 | 797.0 | 587.6 | |
| 1.46 | 1.80 | 0.85 | 1.05 | -20.32 | 72.68 | 29.54 | 241.69 | 0.5272 | 704.0 | 605.8 | |
| 3.25 | 4.37 | 1.89 | 2.53 | -20.12 | 72.39 | 29.24 | 241.85 | 0.5223 | 957.4 | 740.3 | |
| 0.00 | 1.28 | 0.00 | 0.74 | -19.49 | 72.15 | 29.01 | 242.83 | 0.5159 | 728.0 | 626.8 | |
| 0.34 | 1.37 | 0.20 | 0.79 | -20.08 | 71.98 | 28.84 | 241.65 | 0.5168 | 939.2 | 798.2 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -20.30 | 71.78 | 28.63 | 241.11 | 0.5154 | 797.0 | 634.1 | |
| 0.00 | 1.46 | 0.00 | 0.84 | -21.16 | 71.27 | 28.12 | 239.21 | 0.5138 | 866.0 | 670.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -18.02 | 69.98 | 26.83 | 244.18 | 0.4788 | 647.0 | 569.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -19.33 | 68.83 | 25.69 | 240.77 | 0.4707 | -688.0 | -473.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -19.28 | 68.62 | 25.47 | 240.70 | 0.4674 | -786.0 | -716.6 | |
| 0.00 | 2.40 | 0.00 | 1.31 | -20.45 | 64.85 | 21.70 | 234.75 | 0.4261 | -854.0 | -685.9 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -20.12 | 64.73 | 21.59 | 235.30 | 0.4220 | -808.0 | -683.5 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -19.88 | 64.53 | 21.38 | 235.57 | 0.4175 | -696.0 | -518.7 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -20.73 | 63.37 | 20.22 | 232.45 | 0.4095 | -758.0 | -543.4 | |
| 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. | |