| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88.89 | 404.21 | 107.20 | 499.37 | -19.81 | 81.97 | -63.96 | 112.45 | 0.9148 | 60.4 | 34.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-27 13:00:25 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 |
| 45.69 | 230.58 | 49.78 | 256.85 | -19.73 | 85.36 | -60.57 | 113.02 | 0.8927 | 553.8 | 137.3 | |
| 0.00 | 0.68 | 0.00 | 0.77 | -20.28 | 84.60 | -61.33 | 113.46 | 0.8990 | -326.0 | -352.9 | |
| 5.73 | -1.00 | 6.53 | -1.00 | -19.98 | 84.01 | -61.93 | 113.00 | 0.9027 | 220.6 | 999999 | |
| 1.11 | -1.00 | 1.29 | -1.00 | -20.09 | 83.45 | -62.48 | 113.00 | 0.9066 | 294.5 | 999999 | |
| 4.36 | -1.00 | 5.18 | -1.00 | -20.23 | 82.87 | -63.07 | 113.03 | 0.9108 | 146.6 | 999999 | |
| 0.00 | 2.91 | 0.00 | 3.33 | -19.01 | 83.72 | -62.22 | 111.88 | 0.9032 | -340.0 | -274.1 | |
| 0.00 | 0.60 | 0.00 | 0.70 | -19.43 | 83.16 | -62.78 | 112.23 | 0.9077 | -341.0 | -338.6 | |
| 0.00 | 0.26 | 0.00 | 0.29 | -18.63 | 83.69 | -62.24 | 111.47 | 0.9029 | 289.0 | 235.0 | |
| 1.97 | 6.93 | 2.46 | 8.67 | -20.95 | 81.66 | -64.28 | 113.57 | 0.9196 | 233.4 | -58.7 | |
| 0.00 | 0.26 | 0.00 | 0.31 | -19.44 | 82.73 | -63.20 | 112.15 | 0.9106 | -440.0 | -448.0 | |
| 0.00 | 1.63 | 0.00 | 2.01 | -20.19 | 81.67 | -64.26 | 112.75 | 0.9185 | -396.0 | -324.1 | |
| 0.00 | 2.40 | 0.00 | 2.91 | -19.26 | 82.08 | -63.86 | 111.84 | 0.9147 | 49.0 | -23.8 | |
| 0.00 | 1.88 | 0.00 | 2.45 | -20.60 | 80.44 | -65.49 | 112.96 | 0.9267 | -321.0 | -377.7 | |
| 0.00 | 1.28 | 0.00 | 1.57 | -18.74 | 81.73 | -64.20 | 111.20 | 0.9163 | -489.0 | -402.6 | |
| 0.00 | 0.26 | 0.00 | 0.31 | -18.39 | 81.76 | -64.17 | 110.84 | 0.9157 | -294.0 | -355.0 | |
| 1.28 | 7.02 | 1.65 | 9.03 | -19.58 | 80.58 | -65.35 | 111.90 | 0.9246 | 334.3 | 196.2 | |
| 0.00 | 0.43 | 0.00 | 0.55 | -19.26 | 80.67 | -65.26 | 111.58 | 0.9237 | -125.0 | -144.2 | |
| 1.11 | 5.05 | 1.58 | 7.15 | -21.18 | 78.56 | -67.37 | 113.25 | 0.9382 | -632.1 | -565.9 | |
| 1.80 | 3.34 | 2.29 | 4.25 | -18.26 | 80.60 | -65.34 | 110.49 | 0.9230 | -554.7 | -476.4 | |
| 0.00 | 1.54 | 0.00 | 2.08 | -19.77 | 79.42 | -66.52 | 111.89 | 0.9318 | -552.0 | -482.0 | |
| 2.48 | 26.44 | 3.58 | 38.95 | -20.88 | 78.01 | -67.93 | 112.83 | 0.9410 | -468.3 | 124.6 | |
| 0.00 | 0.26 | 0.00 | 0.34 | -18.46 | 79.83 | -66.10 | 110.58 | 0.9280 | -289.0 | -302.0 | |
| 13.35 | 103.01 | 18.84 | 145.65 | -19.85 | 78.36 | -67.57 | 111.81 | 0.9380 | -543.4 | -73.4 | |
| 1.11 | -23.00 | 1.60 | -23.00 | -20.15 | 78.01 | -67.92 | 112.06 | 0.9402 | -188.8 | 999999 | |
| 3.25 | -23.00 | 4.41 | -23.00 | -18.79 | 79.09 | -66.84 | 110.81 | 0.9327 | -574.6 | 999999 | |
| 1.20 | 2.65 | 1.78 | 3.95 | -20.64 | 77.29 | -68.65 | 112.46 | 0.9446 | 48.9 | 16.2 | |
| 0.86 | -23.00 | 1.19 | -23.00 | -19.02 | 78.66 | -67.27 | 110.99 | 0.9355 | -536.7 | 999999 | |
| 3.59 | -23.00 | 5.04 | -23.00 | -19.06 | 78.38 | -67.55 | 110.98 | 0.9371 | -414.5 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.98 | -18.08 | 77.53 | -68.40 | 109.81 | 0.9410 | 285.0 | 236.8 | |
| 0.00 | 0.60 | 0.00 | 0.91 | -18.85 | 76.68 | -69.26 | 110.50 | 0.9463 | -369.0 | -317.7 | |
| 0.00 | 1.03 | 0.00 | 1.59 | -18.08 | 76.02 | -69.92 | 109.60 | 0.9491 | -95.0 | -107.3 | |
| 0.00 | 1.80 | 0.00 | 2.77 | -17.30 | 76.07 | -69.86 | 108.79 | 0.9483 | -356.0 | -338.0 | |
| 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. |
||
| 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. |
||
| 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. | |