SDO HMI 2011-11-14 04:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.90 | 191.62 | 68.85 | 482.41 | 19.06 | 106.40 | 78.86 | 288.86 | 0.9802 | -157.9 | -93.0 | |
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back to the solar disc SDO HMI 2011-11-14 04:58:58 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 |
| 8.86 | 93.70 | 25.87 | 277.55 | 19.12 | 108.33 | 80.79 | 288.89 | 0.9865 | 399.0 | 167.8 | |
| 10.41 | -1.00 | 28.95 | -1.00 | 19.05 | 107.79 | 80.25 | 288.83 | 0.9850 | -330.8 | 999999 | |
| 0.00 | 4.99 | 0.00 | 12.77 | 18.88 | 106.74 | 79.20 | 288.67 | 0.9819 | -485.0 | -410.7 | |
| 0.00 | 3.53 | 0.00 | 8.62 | 19.41 | 106.20 | 78.65 | 289.21 | 0.9802 | -416.0 | -398.0 | |
| 6.63 | 57.47 | 14.03 | 120.02 | 18.48 | 104.24 | 76.70 | 288.29 | 0.9732 | -655.2 | -406.3 | |
| 0.00 | 2.15 | 0.00 | 4.41 | 18.88 | 103.72 | 76.18 | 288.72 | 0.9712 | -509.0 | -494.8 | |
| 0.00 | 12.91 | 0.00 | 25.88 | 19.49 | 103.40 | 75.86 | 289.36 | 0.9700 | -651.0 | -507.6 | |
| 0.00 | 0.95 | 0.00 | 1.93 | 20.20 | 103.65 | 76.11 | 290.08 | 0.9711 | -505.0 | -477.1 | |
| 0.00 | 3.53 | 0.00 | 7.92 | 21.37 | 105.01 | 77.47 | 291.24 | 0.9763 | -415.0 | -327.0 | |
| 0.00 | 2.24 | 0.00 | 4.32 | 20.24 | 102.80 | 75.26 | 290.16 | 0.9677 | -443.0 | -386.3 | |
| 0.00 | 5.76 | 0.00 | 11.04 | 20.66 | 102.64 | 75.10 | 290.60 | 0.9671 | -393.0 | -347.1 | |
| 0.00 | 4.39 | 0.00 | 7.95 | 20.08 | 101.71 | 74.17 | 290.03 | 0.9630 | -26.0 | 27.4 | |
| 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. | |