SDO HMI 2014-09-23 07:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.96 | 0.00 | 9.64 | -13.82 | 285.82 | -0.64 | 178.54 | 0.3793 | 781.6 | 619.7 | |
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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 | 0.97 | 0.00 | 0.52 | -10.33 | 300.06 | 13.60 | 218.11 | 0.3764 | 772.0 | 623.9 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -9.73 | 299.94 | 13.48 | 218.88 | 0.3676 | 756.0 | 648.7 | |
| 0.00 | 1.51 | 0.00 | 0.80 | -9.41 | 299.87 | 13.41 | 219.27 | 0.3629 | 855.0 | 612.5 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -15.14 | 288.34 | 1.88 | 184.80 | 0.3801 | 765.0 | 612.2 | |
| 0.00 | 1.77 | 0.00 | 1.02 | -23.89 | 285.08 | -1.38 | 177.54 | 0.5163 | 733.0 | 602.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -7.45 | 284.42 | -2.05 | 171.94 | 0.2535 | 756.0 | 596.2 | |
| 0.00 | 0.35 | 0.00 | 0.18 | -8.08 | 284.05 | -2.41 | 170.90 | 0.2649 | 812.0 | 612.0 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -16.81 | 283.07 | -3.39 | 172.02 | 0.4095 | 797.0 | 692.0 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -10.38 | 282.22 | -4.24 | 166.32 | 0.3088 | 936.0 | 802.4 | |
| 0.00 | 2.13 | 0.00 | 1.16 | -17.38 | 281.92 | -4.54 | 169.63 | 0.4214 | 738.0 | 489.8 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -17.81 | 281.66 | -4.80 | 169.24 | 0.4289 | 575.0 | 468.7 | |
| 0.00 | 1.77 | 0.00 | 0.94 | -12.87 | 280.82 | -5.64 | 164.24 | 0.3545 | 885.0 | 738.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -10.61 | 278.55 | -7.91 | 155.87 | 0.3322 | 768.0 | 614.7 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -10.91 | 276.25 | -10.21 | 150.36 | 0.3536 | 794.0 | 593.4 | |
| 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. | |