SDO HMI 2011-11-14 11:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.20 | 239.39 | 19.17 | 138.23 | 28.21 | 42.35 | 18.63 | 326.76 | 0.5153 | -814.7 | -401.2 | |
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back to the solar disc SDO HMI 2011-11-14 11:58:58 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 |
| 0.00 | 0.86 | 0.00 | 0.52 | 32.61 | 44.95 | 21.23 | 328.50 | 0.5861 | -526.0 | -406.4 | |
| 13.76 | 225.46 | 7.94 | 130.31 | 27.99 | 42.61 | 18.89 | 326.12 | 0.5149 | -1340.1 | -419.7 | |
| 10.32 | -2.00 | 5.97 | -2.00 | 28.38 | 42.65 | 18.93 | 326.55 | 0.5198 | -1083.0 | 999999 | |
| 3.70 | -2.00 | 2.13 | -2.00 | 28.10 | 42.24 | 18.52 | 326.75 | 0.5130 | -1318.5 | 999999 | |
| 1.81 | -2.00 | 1.04 | -2.00 | 28.39 | 42.22 | 18.50 | 327.13 | 0.5164 | -933.3 | 999999 | |
| 3.61 | -2.00 | 2.09 | -2.00 | 28.59 | 42.18 | 18.47 | 327.41 | 0.5184 | -829.8 | 999999 | |
| 0.00 | 2.58 | 0.00 | 1.49 | 28.99 | 41.65 | 17.93 | 328.60 | 0.5190 | -555.0 | -488.5 | |
| 0.00 | 2.58 | 0.00 | 1.46 | 26.84 | 41.11 | 17.39 | 326.77 | 0.4887 | -772.0 | -592.3 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 29.64 | 40.52 | 16.80 | 330.89 | 0.5184 | -650.0 | -605.0 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 29.34 | 40.40 | 16.68 | 330.74 | 0.5138 | -805.0 | -670.7 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 29.32 | 39.65 | 15.93 | 331.78 | 0.5081 | -896.0 | -721.2 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 27.09 | 36.73 | 13.01 | 333.96 | 0.4584 | 788.0 | 654.1 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 26.67 | 36.65 | 12.93 | 333.64 | 0.4521 | 702.0 | 591.1 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 26.90 | 36.43 | 12.71 | 334.25 | 0.4538 | 969.0 | 713.8 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 27.16 | 36.43 | 12.71 | 334.54 | 0.4573 | 601.0 | 382.0 | |
| 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. | |