The solar wind environment at the ACE satellite indicated fairly nominal
conditions through about 06/0320 UTC. Wind speeds averaged about 450
km/s, IMF total field (Bt) ranged from 4-7 nT while the Bz component did
not vary much beyond +/- 5 nT. The phi angle was highly variable between
a negative (towards) and a positive (away) sector. After 05/0320 UTC,
phi rotated to a steady negative sector, wind speeds gradually increased
to near 475 km/s, Bt sharply increased to near 20 nT and Bz varied
between +16 nT to -6 nT. EPAM low energy particles also showed a gradual
increase indicating the possible arrival of a co-rotating interaction
region in advance of an anticipated negative polarity coronal hole high
speed stream (CH HSS).
The solar wind environment at ACE was modestly enhanced. Wind speed
hovered near 500 km/s. Phi was variable but predominantly negative. Bt
ranged from around 7 to 11 nT. Bz was mostly neutral or positive, with
-6 nT representing the maximum southern excursion.
Solar wind speed at the ACE spacecraft exhibited a gradual increasing
trend from about 385 km/s to near 460 km/s at period’s end. The IMF
total field (Bt) generally ranged from 8-11 nT. The Bz component was
variable between +9 to -8 nT through about 30/2100 UTC when the field
remained mostly north to about +5 nT. The Phi angle remained in a
predominately negative (towards) orientation. Low energy particles
detected by the EPAM instrument began rising slowly during the past 24
hours, perhaps signaling the approach of a co-rotating interaction
region in advance of an anticipated coronal hole high speed stream (CH
Solar wind parameters indicated a nominal solar environment. Total
field ranged from 4 nT to 11 nT while the Bz component was variable
between +10 nT and -7 nT. Wind speed averaged about 360 km/s with a
peak of 430 km/s at 27/1938 UTC. The phi angle was in a predominately
negative (towards) sector with some positive (away) variability between
The anticipated sector change and high speed stream has not materialized
yet. Solar wind was nominal at the ACE spacecraft, with speeds in the
mid 300 km/s range. Phi remained mostly positive and Bt was at or below
6 nT. Bz was mostly negative, dipping as low as -5 nT.
Solar wind parameters, measured at ACE, were indicative of waning
coronal hole high speed stream (CH HSS) influence. Solar wind speed
varied between 360 km/s and 480 km/s to begin the period, but eventually
settle down to consistently average near 380 km/s. Total field was
fairly steady between 6 nT to 7 nT, while the Bz component was mostly
negative, ranging between +4 nT and -7 nT. Phi angle remained mostly
positive (away) throughout the period.
Solar wind parameters continued to be slightly enhanced through the
period, likely under weak coronal hole high speed stream (CH HSS)
influence. Solar wind speeds began the period near 360 km/s, but began a
gradual, yet unsteady climb just after the beginning of the new UT day.
Speeds reached a peak of 477 km/s at 23/0351 UTC, and averaged near 410
km/s for the second half of the period. Total field varied slightly
between 5 nT and 9 nT, while the Bz component was variable between +5 nT
and -7 nT. Phi angle was mostly oriented in a positive (away) sector.
Solar wind parameters were indicative of coronal hole high speed stream
(CH HSS) influence. Solar wind speeds began the period near 610 km/s
before reaching a high speed of 706 km/s at 16/0556 UTC. It began to
decrease slowly just after that peak, ending the period at an average
speed near 450 km/s. After beginning the period near 8 nT, the IMF total
field relaxed and saw an average of near 5 nT to end the period. IMF Bz
component was variable between +5 and -7 nT, while Phi angle was
consistently positive (away) through the period. Conditions have begun
to settle down as a weak transition from CH HSS influence from positive
polarity CH09 transition through weak negative fields before
reconnecting with positive polarity CH10, located near central solar
Solar wind parameters indicated continued elevated ambient solar wind
conditions. The IMF total field strength averaged near 6 nT while Bz
remained mostly positive, with intermittent negative deviations. Solar
wind speeds began the period near 570 km/s, but decreased to end of
period speeds near 460 km/s. Phi angle remained in a negative (towards)
sector throughout the period.
Early solar wind parameters indicated the continued influence of the 07
Nov CME combined with coronal hole high speed stream (CH HSS) effects.
The IMF total field strength began the period near 12 nT, then slowly
decreased to average near 10 nT for the majority of the period. The Bz
component was mostly positive, seeing isolated southern deviations as
low as -9 nT. Solar wind speeds remained near 500 km/s, dropping for a
brief period to average near 450 km/s. Phi angle was mostly oriented in
a negative (towards) sector.