The figure below shows measurements of the solar wind magnetic field at 1 AU over a 24 hour period. Themeasurements are in GSM coordinates and include the vector components of the field as well as the correspondingangles (θ is the polar angle, which correspond to Bz, and φ is the azimuthal angle). Based on the figure, briefly describewhat event occurred between 13 and 14 UT.

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Chapter1: Units, Trigonometry. And Vectors
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The figure below shows measurements of the solar wind magnetic field at 1 AU over a 24 hour period. Themeasurements are in GSM coordinates and include the vector components of the field as well as the correspondingangles (θ is the polar angle, which correspond to Bz, and φ is the azimuthal angle). Based on the figure, briefly describewhat event occurred between 13 and 14 UT.

Bx, By, Bt (gsm)
Bz (gam)
Theta (gsm)
Phi (gam)
ACE RTSW (Estimated) MAG
10
5
0
-5
-10
10
5
0
-5
-10
90
45
0
-45
-90
360
270
180
90
0
I
19
21
start DOY: 120
23 01 03
eaution: ACE maneuver
Begin: 2021-04-30 19:00:00UTC
05 07 09 11
13 15 17 19
UTC(hours) NOAA/SWPC created:2021-05-01 18:45:04UTC
Transcribed Image Text:Bx, By, Bt (gsm) Bz (gam) Theta (gsm) Phi (gam) ACE RTSW (Estimated) MAG 10 5 0 -5 -10 10 5 0 -5 -10 90 45 0 -45 -90 360 270 180 90 0 I 19 21 start DOY: 120 23 01 03 eaution: ACE maneuver Begin: 2021-04-30 19:00:00UTC 05 07 09 11 13 15 17 19 UTC(hours) NOAA/SWPC created:2021-05-01 18:45:04UTC
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