J. M. Forbes, E. K. Sutton, R. S. Nerem Department of Aerospace Engineering Sciences, University of...
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J. M. Forbes, E. K. Sutton, R. S. Nerem
Department of Aerospace Engineering Sciences, University of Colorado, Boulder, Colorado, USA
Sean Bruinsma, CNESToulouse, France
Thermosphere Density and Wind Responses to Solar and Geomagnetic Activity
GRACE-A & GRACE-B• launched in March 2002• 3.12 m x 1.94 m x 0.78 m • 500 km altitude• near-circular (89.5°) orbits • GRACE-B ≈ 220 km behind GRACE-A
Supported by NSF Space Weather Grant ATM-0208482
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The CHAMP satellite was launched in July 2000 at 450 km altitude in a near-circular orbit
with an inclination of 87.3°
The physical parameters of the CHAMP satellite are:• Total Mass 522 kg • Height 750 mm• Length (with 4044mm Boom) 8333 mm • Width 1621 mm• Area to Mass Ratio 0.00138 m²kg
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CHAMP is in a 13:20/01:20 LT orbit during the Super Storms
Local time precession rate of CHAMP is about 24 hours/133 days
The GRACE satellites are in a 16:00/04:00 LT orbit during the Super Storms
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The “Halloween 2003” Intense Solar Events
Active region 10486, already under close scrutiny by several instruments on SOHO and other satellites, as well as numerous ground observatories, started up a spectacular two-part show in the morning on Tuesday 28 October 2003. An X 17.2 flare, the second largest flare observed by SOHO, was setting off a strong high energy proton event and a fast-moving Coronal Mass Ejection, hitting Earth early on Wednesday 29 October. The one-two punch was a done deal on Wednesday afternoon, when an X 10.0 flare set off another round of particles and another fast-moving CME.
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Thermosphere Density Response
~200-300%
Second CME
arrives
First CME
arrives
Oct 27
Oct 28
EUV flare
arrives
~200%
19 hrs
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Vic Winter, Warrensburg Missouri, Oct 30: The first wave of aurora appeared between 01 and 02 hours UT. A second wave hit about 04 hours UT and had many red spikes with green curtains below."
Barry Kierstein, Lyndeborough, New Hampshire , Oct. 30
Aurora during theHalloween Storms
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Thermosphere Wind Response to the October/November 2003 Storms from CHAMP
Accelerometer Measurements
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Westward winds during quiet period
Westward intensification during disturbed periods
Daytime (LST ~ 13:20) Zonal Winds at the Equator
Note: longitude also changing @ 360°/day
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CHAMP ~ 0 to -50 m/s during quiet period
HWM93 ~ 50 to 100 m/s during quiet period
CHAMP strong westward intensification during disturbed periods
Nighttime (LST ~ 01:20) Zonal Winds at the Equator
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Suggests enhanced eastward electric field, vertical drifts, and vertical redistribution of equatorial plasma -- reduction or increase in east-west drag at 410 km?
TEC asymmetry possibly imply northward wind?
Equatorial plasma depletion reduces ion drag?
Reduction in O/N2 ratio or transport effect?
TEC Measurements Suggest a Possible Combination of Electrodynamic, Dynamical and Chemical Effects at the Equator
Credit: International GPS Service - http://igscb.jpl.nasa.gov
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X17flare301
Oct 28X28flare308
Nov 4
302, 303Oct 29, 30
324Nov 20
(days)
The Isolated Magnetic Storm of November 20, 2003
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(days)
V2
Bz
ap
Dst
Oct25
Oct30
Oct20
Nov20
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Day of Year, 2003 Day of Year, 2003
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Smoothed densities, using a 150-sec (~1200 km) window, along the orbital tracks of GRACE (left) and CHAMP (right) on dayside (top) and nightside (bottom) beginning during the quiet period early on day 324, and ending during the quiet period early on day 325. The dotted black curves are beginning orbits and the solid black curves are ending orbits while the color rainbow spectrum (from dark blue to red) represents the sequence of orbits during the storm.
Large-Scale Wave Structures during the Storm
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Traveling Atmospheric Disturbances during the 15-24 April 2002 Magnetically Active Interval
waves launched
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~800 ms-1
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