SDO HMI 2011-11-24 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.29 | 53.60 | 8.08 | 30.09 | -15.99 | 267.17 | 21.89 | 229.91 | 0.4720 | 494.4 | 324.8 | |
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back to the solar disc SDO HMI 2011-11-24 23:58:57 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 | 1.28 | 0.00 | 0.72 | -12.10 | 269.50 | 24.21 | 239.52 | 0.4673 | 749.0 | 678.4 | |
| 0.00 | 3.00 | 0.00 | 1.67 | -12.30 | 268.69 | 23.40 | 238.30 | 0.4580 | 778.0 | 531.5 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -12.63 | 268.16 | 22.87 | 237.10 | 0.4536 | 691.0 | 492.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -12.54 | 267.92 | 22.63 | 237.02 | 0.4497 | 644.0 | 508.1 | |
| 0.00 | 1.97 | 0.00 | 1.09 | -12.29 | 267.90 | 22.61 | 237.46 | 0.4475 | 805.0 | 739.0 | |
| 0.00 | 2.74 | 0.00 | 1.51 | -12.38 | 267.71 | 22.42 | 237.08 | 0.4457 | 928.0 | 729.5 | |
| 3.42 | 32.71 | 1.94 | 18.50 | -17.01 | 267.78 | 22.50 | 228.94 | 0.4872 | 946.8 | 564.4 | |
| 10.87 | -7.00 | 6.14 | -7.00 | -16.70 | 267.64 | 22.36 | 229.29 | 0.4827 | 1100.4 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -15.59 | 266.29 | 21.00 | 229.44 | 0.4563 | 797.0 | 649.8 | |
| 0.00 | 1.97 | 0.00 | 1.10 | -17.73 | 264.91 | 19.62 | 224.02 | 0.4623 | -890.0 | -666.9 | |
| 0.00 | 2.57 | 0.00 | 1.43 | -17.54 | 264.72 | 19.44 | 224.05 | 0.4583 | -968.0 | -775.9 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -15.75 | 263.59 | 18.31 | 225.36 | 0.4267 | -688.0 | -521.2 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -19.04 | 263.87 | 18.59 | 220.50 | 0.4659 | -635.0 | -540.7 | |
| 0.00 | 1.37 | 0.00 | 0.75 | -18.47 | 260.48 | 15.20 | 215.86 | 0.4262 | -876.0 | -751.4 | |
| 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. | |