SDO HMI 2011-09-06 19:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.53 | 23.19 | 4.85 | 19.63 | -18.96 | 257.73 | 48.09 | 240.26 | 0.8121 | 133.3 | 121.8 | |
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back to the solar disc SDO HMI 2011-09-06 19:59:07 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 |
| 4.55 | 11.69 | 3.99 | 10.22 | -19.41 | 259.18 | 49.54 | 240.45 | 0.8271 | 497.8 | 590.5 | |
| 0.98 | -1.00 | 0.86 | -1.00 | -19.55 | 258.94 | 49.31 | 240.18 | 0.8257 | 540.5 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.86 | -20.11 | 258.83 | 49.19 | 239.51 | 0.8270 | 406.0 | 304.7 | |
| 0.00 | 0.71 | 0.00 | 0.62 | -19.58 | 258.56 | 48.92 | 239.97 | 0.8225 | 636.0 | 529.9 | |
| 0.00 | 1.16 | 0.00 | 1.00 | -19.16 | 258.34 | 48.70 | 240.33 | 0.8189 | 764.0 | 631.9 | |
| 0.00 | 0.62 | 0.00 | 0.53 | -19.10 | 258.08 | 48.44 | 240.28 | 0.8163 | 538.0 | 462.6 | |
| 0.00 | 0.98 | 0.00 | 0.81 | -18.42 | 256.91 | 47.27 | 240.48 | 0.8032 | -398.0 | -359.9 | |
| 0.00 | 0.71 | 0.00 | 0.60 | -20.31 | 256.40 | 46.76 | 238.10 | 0.8070 | -314.0 | -201.9 | |
| 0.00 | 1.52 | 0.00 | 1.24 | -19.27 | 255.73 | 46.09 | 238.91 | 0.7963 | -587.0 | -534.8 | |
| 0.00 | 0.80 | 0.00 | 0.66 | -19.65 | 255.87 | 46.23 | 238.56 | 0.7993 | -232.0 | -221.7 | |
| 0.00 | 1.52 | 0.00 | 1.21 | -18.22 | 255.17 | 45.53 | 239.83 | 0.7864 | -524.0 | -458.9 | |
| 0.00 | 2.50 | 0.00 | 1.88 | -15.29 | 253.27 | 43.63 | 242.28 | 0.7542 | -761.0 | -565.5 | |
| 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. | |