SDO HMI 2014-05-17 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.47 | 293.15 | 24.76 | 156.38 | -23.97 | 191.91 | 2.23 | 185.59 | 0.3714 | 838.7 | 370.9 | |
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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 | 1.17 | 0.00 | 0.61 | -19.97 | 195.56 | 5.89 | 197.70 | 0.3184 | -845.0 | -661.7 | |
| 15.64 | 279.21 | 8.33 | 148.90 | -23.90 | 192.33 | 2.66 | 186.59 | 0.3706 | 1349.9 | 421.2 | |
| 0.27 | -2.00 | 0.14 | -2.00 | -23.54 | 192.26 | 2.58 | 186.53 | 0.3646 | 1375.0 | 999999 | |
| 3.15 | -2.00 | 1.67 | -2.00 | -23.57 | 192.09 | 2.42 | 186.11 | 0.3649 | 1303.4 | 999999 | |
| 18.06 | -2.00 | 9.64 | -2.00 | -24.16 | 191.93 | 2.26 | 185.55 | 0.3741 | 1181.1 | 999999 | |
| 9.35 | -2.00 | 4.98 | -2.00 | -23.83 | 191.93 | 2.26 | 185.63 | 0.3688 | 1450.4 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.19 | -22.53 | 191.42 | 1.74 | 184.67 | 0.3469 | 843.0 | 589.5 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -21.44 | 191.14 | 1.47 | 184.19 | 0.3286 | -837.0 | -749.9 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -22.86 | 190.66 | 0.99 | 182.61 | 0.3514 | -48.0 | -178.7 | |
| 0.00 | 1.80 | 0.00 | 0.96 | -23.60 | 187.59 | -2.08 | 174.74 | 0.3648 | -604.0 | -620.9 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -27.39 | 185.64 | -4.03 | 171.59 | 0.4289 | -691.0 | -603.8 | |
| 0.00 | 3.59 | 0.00 | 1.96 | -26.49 | 185.64 | -4.04 | 171.23 | 0.4148 | -693.0 | -707.4 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -26.99 | 185.52 | -4.16 | 171.18 | 0.4229 | -914.0 | -833.8 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -27.55 | 185.15 | -4.52 | 170.67 | 0.4327 | -655.0 | -598.6 | |
| 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. | |