Payloads coming/which came down:
MMS team needs to know within 24 hours if you would like them to download data. E-mail Drew Turner or Allison Jaynes if you would like them to collect data in a specific region/time for conjunction studies.
the L-shell of BARREL and the neighboring inner magnetosphere (L> ~3)
for the context of possible conjunctions with this BARREL campaign.
Within these fast survey intervals, thye also trigger particle and wave
bursts to capture high-frequency waves (whistler-mode).
This special data collection scheme is implemented on the three inner
probes for Aug. 10-25 (starting from Aug. 11 for TH-D), based on the
estimated interval of this BARREL campaign.
Swedish Institute of Space Physics: Kiruna Magnetometer: http://www.irf.
ACE Solar wind speed:
ACE Solar proton density:
69 and Sunspot AR2571 is rotating off the disk. Sunspot regions 2574, 2575, and 2576 are still rotating around but do not currently look complex enough to likely produce a CME.
GOES Flare activity:
kp = 2 with a 24 hour max of kp = 3
ACE SW magnetic field:
Coronal hole news
The high speed stream has reached the Earth and the solar wind velocity is expected to stay high until about August 12th according to the WSA-ENLIL models. However we can already see that the velocity is dropping.