group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
70.88 | 378.32 | 87.21 | 473.02 | 13.73 | 173.85 | 66.39 | 284.01 | 0.9166 | -87.0 | 12.4 |
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back to the solar disc SDO HMI 2010-11-18 13:58:57 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 |
2.92 | 211.43 | 4.22 | 300.69 | 12.84 | 177.52 | 70.06 | 282.78 | 0.9413 | 290.1 | -97.9 | |
31.15 | -1.00 | 44.05 | -1.00 | 12.96 | 176.96 | 69.50 | 282.92 | 0.9381 | -734.2 | 999999 | |
1.37 | -1.00 | 1.89 | -1.00 | 13.34 | 176.42 | 68.96 | 283.36 | 0.9350 | -943.9 | 999999 | |
0.00 | 1.20 | 0.00 | 1.60 | 12.86 | 175.62 | 68.16 | 282.88 | 0.9299 | -548.0 | -492.4 | |
0.00 | 2.49 | 0.00 | 3.17 | 13.21 | 174.45 | 66.99 | 283.31 | 0.9225 | -568.0 | -433.8 | |
0.00 | 3.17 | 0.00 | 3.89 | 13.27 | 173.56 | 66.10 | 283.43 | 0.9166 | 241.0 | -65.9 | |
4.12 | 5.06 | 4.85 | 5.96 | 13.37 | 172.49 | 65.03 | 283.61 | 0.9093 | 292.2 | 131.8 | |
0.00 | 2.23 | 0.00 | 2.58 | 12.75 | 172.04 | 64.58 | 282.96 | 0.9057 | 408.0 | 313.8 | |
3.00 | 3.52 | 3.49 | 4.08 | 13.48 | 172.04 | 64.58 | 283.76 | 0.9061 | 438.3 | 374.7 | |
0.00 | 1.63 | 0.00 | 1.89 | 14.15 | 171.96 | 64.50 | 284.51 | 0.9059 | 196.0 | 151.6 | |
0.00 | 0.60 | 0.00 | 0.64 | 14.33 | 169.64 | 62.18 | 284.90 | 0.8887 | 240.0 | 267.4 | |
3.95 | 5.15 | 4.14 | 5.40 | 14.72 | 168.92 | 61.46 | 285.41 | 0.8833 | 354.7 | 172.4 | |
24.37 | 141.84 | 24.57 | 143.12 | 15.38 | 167.59 | 60.13 | 286.30 | 0.8731 | 830.8 | 251.8 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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 | |
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. |