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3-day Report of Solar and Geophysical Activity
Issued Sep 08 22:00 UTC
Solar Activity Forecast:
Solar activity is expected to remain at very low levels for the next three days (09 - 11 September).
Geophysical Activity Forecast:
The geomagnetic field is expected to be at quiet to unsettled levels for day one (09 September) and mostly quiet for days two and three (10 - 11 September).
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Latest GOES 14 Solar X-ray Image Image See Solar Image References for other solar image sites. |

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SOHO EIT 304 |
SOHO EIT 284 |
Mauna Loa Solar Image |
The sun is constantly monitored for sun spots and coronal mass ejections. EIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore, shows solar material at different temperatures. In the images taken at 304 Angstrom the bright material is at 60,000 to 80,000 degrees Kelvin. In those taken at 171 Angstrom, at 1 million degrees. 195 Angstrom images correspond to about 1.5 million Kelvin, 284 Angstrom to 2 million degrees. The hotter the temperature, the higher you look in the solar atmosphere.

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CURRENT TIME
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Solar Cycle Progression Solar Cycle chart updated using the latest ISES predictions. |
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The Solar Cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Solar minimum occurred in December, 2008. Solar maximum is expected to occur in May, 2013.
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Solar X-ray Flux This plot shows 3-days of 5-minute solar x-ray flux values measured on the SWPC primary and secondary GOES satellites. |
Satellite Environment Plot The Satellite Environment Plot combines satellite and ground-based data to provide an overview of the current geosynchronous satellite environment. |

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Northern Hemi Auroral Map |
Southern Hemi Auroral Map |
Instruments on board the NOAA Polar-orbiting Operational Environmental Satellite (POES) continually monitor the power flux carried by the protons and electrons that produce aurora in the atmosphere. SWPC has developed a technique that uses the power flux observations obtained during a single pass of the satellite over a polar region (which takes about 25 minutes) to estimate the total power deposited in an entire polar region by these auroral particles. The power input estimate is converted to an auroral activity index that ranges from 1 to 10.
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| Asteroid | Date(UT) |
Miss
Distance |
Mag. |
Size |
| 2010 QG2 | Sep 3 |
4.6 LD |
24 |
61 m |
| 2010 RB12 | Sep 4 |
2.5 LD |
27 |
18 m |
| 2010 LY63 | Sep 7 |
56 LD |
18 |
1.2 km |
| 2010 RX30 | Sep 8 |
0.6 LD |
27 |
16 m |
| 2010 RF12 | Sep 8 |
0.2 LD |
28 |
9 m |
| 2009 SH2 | Sep 30 |
7.1 LD |
25 |
45 m |
| 1998 UO1 | Oct 1 |
32.1 LD |
17 |
2.1 km |
| 2005 GE59 | Oct 1 |
77 LD |
18 |
1.1 km |
| 2001 WN5 | Oct 10 |
41.8 LD |
18 |
1.0 km |
| 1999 VO6 | Oct 14 |
34.3 LD |
17 |
1.8 km |
| 1998 TU3 | Oct 17 |
69.1 LD |
15 |
5.3 km |
| 1998 MQ | Oct 23 |
77.7 LD |
17 |
1.9 km |
| 2007 RU17 | Oct 29 |
40.6 LD |
18 |
1.0 km |
| 2003 UV11 | Oct 30 |
5 LD |
19 |
595 m |
| 3838 Epona | Nov 7 |
76.8 LD |
16 |
3.4 km |
| 2005 QY151 | Nov 16 |
77.7 LD |
18 |
1.3 km |
| 2008 KT | Nov 23 |
5.6 LD |
28 |
10 m |
| 2002 EZ16 | Nov 30 |
73.9 LD |
18 |
1.0 km |
| 2000 JH5 | Dec 7 |
47 LD |
17 |
1.5 km |
| 2010 JL33 | Dec 9 |
16.6 LD |
18 |
1.3 km |
| Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach. |
| Source: Space Weather.com |

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