SDO HMI 2014-08-10 01:00:39 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 123.36 | 644.69 | 66.44 | 345.82 | 12.75 | 129.50 | -21.48 | 70.74 | 0.3800 | -155.4 | -143.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-10 01:00:39 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 | 1.26 | 0.00 | 0.67 | 16.30 | 133.43 | -17.55 | 58.49 | 0.3409 | -840.0 | -595.2 | |
| 65.46 | 393.47 | 34.48 | 207.32 | 14.11 | 132.36 | -18.61 | 65.62 | 0.3414 | -1377.6 | -451.3 | |
| 0.27 | -2.00 | 0.14 | -2.00 | 14.03 | 131.77 | -19.20 | 66.43 | 0.3497 | -805.0 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 10.63 | 131.60 | -19.38 | 76.15 | 0.3373 | -704.0 | -503.8 | |
| 0.00 | 7.76 | 0.00 | 4.11 | 13.11 | 131.05 | -19.92 | 69.53 | 0.3558 | -902.0 | -733.7 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 14.18 | 130.93 | -20.05 | 66.80 | 0.3632 | -548.0 | -382.2 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 12.56 | 130.90 | -20.08 | 71.16 | 0.3556 | -701.0 | -505.5 | |
| 0.00 | 1.35 | 0.00 | 0.72 | 12.91 | 129.70 | -21.27 | 71.07 | 0.3754 | 833.0 | 625.7 | |
| 0.00 | 2.44 | 0.00 | 1.30 | 12.42 | 129.71 | -21.26 | 72.34 | 0.3733 | 748.0 | 614.8 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 14.98 | 129.13 | -21.84 | 66.36 | 0.3940 | -619.0 | -556.8 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 8.06 | 126.82 | -24.16 | 84.48 | 0.4088 | 689.0 | 567.4 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 9.88 | 126.69 | -24.28 | 80.07 | 0.4131 | 633.0 | 546.3 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 11.74 | 126.50 | -24.48 | 75.71 | 0.4204 | 765.0 | 652.2 | |
| 0.00 | 4.42 | 0.00 | 2.42 | 12.13 | 126.39 | -24.58 | 74.84 | 0.4231 | 554.0 | 687.8 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 10.18 | 126.43 | -24.55 | 79.44 | 0.4177 | 870.0 | 781.2 | |
| 0.00 | 1.90 | 0.00 | 1.04 | 11.63 | 126.07 | -24.91 | 76.15 | 0.4267 | -612.0 | -416.6 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 11.24 | 125.69 | -25.29 | 77.18 | 0.4314 | 948.0 | 730.8 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 9.78 | 125.82 | -25.16 | 80.53 | 0.4265 | 693.0 | 627.7 | |
| 2.08 | 5.42 | 1.14 | 2.98 | 11.54 | 125.56 | -25.42 | 76.54 | 0.4342 | 827.8 | 534.1 | |
| 1.90 | 212.89 | 1.04 | 117.80 | 10.17 | 125.48 | -25.50 | 79.73 | 0.4324 | 1125.9 | 414.4 | |
| 0.00 | 1.44 | 0.00 | 0.79 | 10.99 | 125.41 | -25.57 | 77.86 | 0.4352 | 645.0 | 586.2 | |
| 2.44 | -20.00 | 1.34 | -20.00 | 10.46 | 125.25 | -25.73 | 79.11 | 0.4365 | 1145.7 | 999999 | |
| 2.71 | -20.00 | 1.49 | -20.00 | 10.18 | 125.17 | -25.81 | 79.77 | 0.4372 | 1034.8 | 999999 | |
| 5.24 | -20.00 | 2.89 | -20.00 | 10.73 | 125.09 | -25.89 | 78.55 | 0.4396 | 1138.8 | 999999 | |
| 4.79 | -20.00 | 2.64 | -20.00 | 10.94 | 125.00 | -25.98 | 78.10 | 0.4414 | 940.0 | 999999 | |
| 11.11 | -20.00 | 6.13 | -20.00 | 10.56 | 124.86 | -26.12 | 78.98 | 0.4427 | 1152.3 | 999999 | |
| 3.07 | -20.00 | 1.70 | -20.00 | 10.21 | 124.55 | -26.43 | 79.85 | 0.4469 | 1053.3 | 999999 | |
| 17.06 | -20.00 | 9.45 | -20.00 | 10.61 | 124.44 | -26.54 | 79.01 | 0.4492 | 970.7 | 999999 | |
| 4.88 | -20.00 | 2.70 | -20.00 | 9.83 | 124.23 | -26.74 | 80.77 | 0.4511 | 1041.4 | 999999 | |
| 2.35 | -20.00 | 1.30 | -20.00 | 10.04 | 124.01 | -26.97 | 80.37 | 0.4548 | 801.4 | 999999 | |
| 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. | |