Abstract
| Original language | English |
|---|---|
| Journal | Proceedings of the XXXIII annual conference of the Finnish Physical Society |
| Publication status | Published - 1999 |
| Event | Finnish Physical Society - Turku, Finland Duration: 1 Jan 1999 → … |
Conference
| Conference | Finnish Physical Society |
|---|---|
| City | Turku, Finland |
| Period | 01/01/1999 → … |
Cite this
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First results of the Auroral Turbulance II rocket experiment. / Danielides, M.A.; Ranta, A.; Ivchenco, N.; Marklund, G.; Poetrowski, D.; Lynch, K.A.; Torbert, R.B.; Primdahl, Fritz.
In: Proceedings of the XXXIII annual conference of the Finnish Physical Society, 1999.Research output: Contribution to journal › Journal article › Research
TY - JOUR
T1 - First results of the Auroral Turbulance II rocket experiment
AU - Danielides, M.A.
AU - Ranta, A.
AU - Ivchenco, N.
AU - Marklund, G.
AU - Poetrowski, D.
AU - Lynch, K.A.
AU - Torbert, R.B.
AU - Primdahl, Fritz
PY - 1999
Y1 - 1999
N2 - The Auroral Turbulance II sounding rocket was launched on February 11, 1997 into moderately active nightside aurora from the Poker Flat Research Range, Alaska, US. The experiment consisted of three independent, completely instrumented payloads launched by a single vehicle. The aim of the experiment was to study the fine structure of an active auroral arc. Ground based observations were done by a chain all-sky cameras, a photometer and a magnetometer at Poker Flat. The satellite coverage was obtained by POLAR UV imager and GOES 8 and 9 magnetometer. The three point measurement allows the distinction of spatial and temporal variations. The first results of the magnetic, [1,2], electric and particle data analysis are compared with optical observations [2] of auroral structures.
AB - The Auroral Turbulance II sounding rocket was launched on February 11, 1997 into moderately active nightside aurora from the Poker Flat Research Range, Alaska, US. The experiment consisted of three independent, completely instrumented payloads launched by a single vehicle. The aim of the experiment was to study the fine structure of an active auroral arc. Ground based observations were done by a chain all-sky cameras, a photometer and a magnetometer at Poker Flat. The satellite coverage was obtained by POLAR UV imager and GOES 8 and 9 magnetometer. The three point measurement allows the distinction of spatial and temporal variations. The first results of the magnetic, [1,2], electric and particle data analysis are compared with optical observations [2] of auroral structures.
M3 - Journal article
JO - Proceedings of the XXXIII annual conference of the Finnish Physical Society
JF - Proceedings of the XXXIII annual conference of the Finnish Physical Society
ER -