Good Morning
There was a CME on Saturday, but it looks more certain that it may have been too far north to be very geo-effective.
Payloads up:
SANAE IV: 1T
Halley 6: 1H, 1I, 1A
Payloads coming down:
1I and 1H are starting to (or have already) dipped below 27 km and may be terminated in the next few days.
Conjunctions:
Feb 9 2013
Sat. A 0430 UT - 1100 UT
Sat. B 0730 UT - 1350 UT
Feb 8 2013
Sat. A 0200 UT - 0800 UT
Sat. B 0600 UT - 1100 UT
Feb 5 2013
Sat. A 0130 UT - 0845 UT
Sat. B 0355 UT - 1130 UT
Feb 4 2013
Sat. B 0045 UT - 0810 UT
Feb 3-4 2013
Sat. A 2220 UT on February 3rd to 0545 on February 4th
Sat. A 0420 UT - 1200 UT
Sat. B 0640 UT - 1420 UT
Jan 30 2013-partially cancelled
Sat. A 0140 UT - 0555 UT
Sat. B 0335 UT - 1050 UT
Sat. A 0735 UT - 1515 UT
Sat. B 0025 UT - 0740 UT
Sat. B 0915 UT - 1650 UT
Jan 28-29 2013
Sat. A 2250 UT Jan 28 - 0605 UT Jan 29
Jan 28 2013
Sat. A 0450 UT - 1210 UT
Sat. B 0625 UT - 1345 UT
Jan 27 2013
Sat. A 0220 UT - 0910 UT
Sat. A 1114 UT - 1815 UT
Sat. B 0330 UT - 1020 UT
Sat. B 1215 UT - 1940 UT
Halley Bay :
quiet
GOES Electron Flux:
Have continued to be at normal to moderate levels and are expected to be the same for the next three days.
GOES Proton Flux:
Has stayed at background levels for the lat 24 hours and is expected to be the same over the next three days
Solar wind speed is 352.4 km/s
Solar proton density 0.6 cm^(-3)
45 sunspots are now visible. NOAA has the likelihood of a M class flare at 10% and a 1% chance of an X class flare.
Kp is quiet kp = 0 with a 24 max of kp = 1
Bz = 2.2 nT north
Btotal = 5.2 nT
The third and final coronal hole from this last bunch is now on the western limb but may be too far south to be geo-effective. If we see solar winds from this hole, they are expected to reach us on Feb. 12th.
From Kyoto:
AE: small amounts of activity
Dst: quiet.
Have a good day!
No comments:
Post a Comment