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 your
estimated interval of this BARREL campaign.
Swedish Institute of Space Physics: Kiruna Magnetometer: http://www.irf.
riometry mode (38 MHz) throughout this time period and will continue to do
so for the remainder of the campaign.
high-speed multi-beam, multi-frequency riometry and various other
monitoring diagnostics. This will continue for a week at least.
ACE Solar wind speed:
ACE Solar proton density:
61 Sunspot regions 2574, 2575, and 2576 are Earthward facing but do not currently look complex enough to likely produce a CME.
GOES Flare activity:
kp = 1 with a 24 hour max of kp = 2
ACE SW magnetic field:
Coronal hole news
The next coronal hole is expected to come after Aug. 18th maybe around the 20th. We should be able to get a 10 heads up from Stereo A. Stereo A will also give us an idea about the magnetic field orientation.