Auroral Activity on May 19/20, 1996
Event Overview
The period of interest spans from about 17:30 UT on May 19 (day 140)
to about 03:00 UT on May 20 (day 141). After a period of very quiet
aurora on the northern hemisphere, an auroral brightening (17:30 UT)
near the midnight sector spread slowly out into a narrow auroral oval.
This was preceeded by a southward turning of the interplanetary
magnetic field. A second southward turning was followed by
significant auroral activity (20:25 UT). Towards the end of the
period another, even larger activity period started (00:35 UT). During
this entire time the entire aurora borealis was in bright sunlight.
Overview of Available Data
During the 9 hour period between 17:30 UT on May 19
and 02:30 UT on May 20, 1996, the UVI imager on POLAR observed strong
auroral activity. During this time, the WIND satellite was about 100
RE upstream in the solar wind, Interball-Tail was about 25
RE upstream, GEOTAIL was at about X=-7 RE
crossing from the sheath into the magnetosphere, and IMP-8 was X=-20
RE inside the magnetotail. DMSP and NOAA-TIROS particle
data from low altitude (800 km) are also available. Ground based
observations were taken by the Sondestrom IS Radar
for the last few hours of this period. SuperDARN
has data for the entire period. Magnetometer data are available from
CANOPUS
and other other chains. No ground based optical observations could be
made, since the entire northern auroral zone is in bright daylight.
Available Data
- Orbit plots:
- Auroral Images:
- Summary plots with one sample image every 5 minutes (LBH-long filter):
- Energy flux from LBH-long images (in geomagnetic coordinates):
- Energy flux from the images with in situ measurements
from DMSP and NOAA superimposed.
- SuperDARN:
- Ground Based Magnetometers:
- Solar Wind:
- Magnetosphere:
Published Papers
- Lummerzheim, D., M. Brittnacher, D. Evans, G. A. Germany,
G. K. Parks, M. H. Rees, and J. F. Spann, High time resolution
study of the hemispheric power carried by energetic electrons into
the ionosphere during the May 19/20, 1996 auroral activity,
Geophys. Res. Lett., 24, 987, 1997. Summary. Contact
person: Dirk Lummerzheim.
- Germany, G. A., G. K.
Parks, M. Brittnacher, J. Cumnock, D. Lummerzheim, J. F. Spann,
L. Chen, P. G. Richards, and F. J. Rich, Remote determination of
auroral energy characteristics during substorm activity, Geophys.
Res, Lett., 24, 995, 1997. HTML
version. Contact person:
Glynn Germany.
- Doe, R. A., J. D. Kelly, D. Lummerzheim, M. Brittnacher,
G. A. Germany, G. K. Parks, and J. F. Spann, Initial comparison
of POLAR UVI and Sondrestrøm IS radar estimates for auroral
electron energy flux, Geophys. Res, Lett., 24,
999, 1997. Summary. Contact
person: Rick Doe.
Studies in progress
- Alfven modulation of substorm magnetotail transport (paper
submitted to the special ISTP issue of
GRL). Contact person: Ennio
Sanchez. Summary.
- A combined analysis of SuperDARN and UVI image data. Contact
person: Kile Baker.
- Modeling of the hemispheric ionosphere using the AMIE
procedure. Contact person: Dirk Lummerzheim.
The
"official" GGS Event page for the 19/20 May
Other GGS events of interest may be found in the
Catalog of GGS Events
Last updated: 23 January 1997
Questions? Comments? Or would you like to add to this study?
Please send E-mail to Dirk Lummerzheim
lumm@gi.alaska.edu
or Kile Baker baker@jhuapl.edu