scholarly journals Data-derived optimization of sensitivity requirements for upcoming auroral imaging missions

2017 ◽  
Vol 122 (9) ◽  
pp. 9358-9370
Author(s):  
Eric Donovan ◽  
Vadim M. Uritsky ◽  
Craig Unick ◽  
Vladimir Troyan
Keyword(s):  
2009 ◽  
Vol 27 (4) ◽  
pp. 1457-1467 ◽  
Author(s):  
R. G. Michell ◽  
K. A. Lynch ◽  
C. J. Heinselman ◽  
H. C. Stenbaek-Nielsen

Abstract. Observations of naturally enhanced ion acoustic lines (NEIALs) taken with the Poker Flat Incoherent Scatter Radar (PFISR) using a mode with very high time resolution are presented. The auroral event took place over Poker Flat, Alaska on 8 February 2007 at 09:35 UT (~22:00 MLT), and the radar data are complemented by common-volume high-resolution auroral imaging. The NEIALs occurred during only one of the standard 15-s integration periods. The raw data of this time show very intermittent NEIALs which occur only during a few very short time intervals (≤1 s) within the 15-s period. The time sampling of the raw data, ~19 ms on average, allows study of the time development of the NEIALs, though there are indications that even finer time resolution would be of interest. The analysis is based on the assumption that the NEIAL returns are the result of Bragg scattering from ion-acoustic waves that have been enhanced significantly above thermal levels. The spectra of the raw data indicate that although the up- and down-shifted shoulders can both become enhanced at the same time, (within 19 ms), they are most often enhanced individually. The overall power in the up-and down-shifted shoulders is approximately equal throughout the event, with the exception of one time, when very large up-shifted power was observed with no corresponding down-shifted power. This indicates that during the 480 μs pulse, the strongly enhanced ion-acoustic waves were only traveling downward and not upward. The exact time that the NEIALs occurred was when the radar beam was on the boundary of a fast-moving (~10 km/s), bright auroral structure, as seen in the high resolution auroral imaging of the magnetic zenith. When viewed with high time resolution, the occurrence of NEIALs is associated with rapid changes in auroral luminosity within the radar field of view due to fast-moving auroral fine structures.


1981 ◽  
Author(s):  
J. B. Kumer ◽  
R. D. Sears ◽  
J. E. Evans ◽  
S. E. Harris ◽  
R. M. Nadile

2007 ◽  
Vol 25 (4) ◽  
pp. 1001-1009 ◽  
Author(s):  
A. T. Y. Lui ◽  
Y. Zheng ◽  
Y. Zhang ◽  
V. Angelopoulos ◽  
G. K. Parks ◽  
...  

Abstract. A close conjunction of several satellites (LANL, GOES, Polar, Geotail, and Cluster) distributed from the geostationary altitude to about 16 RE downstream in the tail occurred during substorm activity as indicated by global auroral imaging and ground-based magnetometer data. This constellation of satellites resembles what is planned for the THEMIS (Time History of Events and Macroscopic Interactions during Substorms) mission to resolve the substorm controversy on the location of the substorm expansion onset region. In this article, we show in detail the dipolarization and dynamic changes seen by these satellites associated with two onsets of substorm intensification activity. In particular, we find that dipolarization at ~16 RE downstream in the tail can occur with dawnward electric field and without plasma flow, just like some near-Earth dipolarization events reported previously. The spreading of substorm disturbances in the tail coupled with complementary ground observations indicates that the observed time sequence on the onsets of substorm disturbances favors initiation in the near-Earth region for this THEMIS-like conjunction.


1982 ◽  
Vol 2 (7) ◽  
pp. IN7-105
Author(s):  
C.D. Anger
Keyword(s):  

2008 ◽  
Vol 16 (20) ◽  
pp. 15623 ◽  
Author(s):  
Fred Sigernes ◽  
Jeffrey Morgan Holmes ◽  
Margit Dyrland ◽  
Dag Arne Lorentzen ◽  
Trond Svenøe ◽  
...  
Keyword(s):  

Author(s):  
B. J. Jackel ◽  
C. Unick ◽  
M. T. Syrjäsuo ◽  
N. Partamies ◽  
J. A. Wild ◽  
...  

Abstract. Color mosaic CCDs use a matrix of different wide-band micro-filters in order to produce images with several (often three) color channels. These devices are increasingly employed in auroral studies to provide time sequences of two dimensional luminosity maps, but the color information is typically only used for qualitative analysis. In this study we use Backus–Gilbert linear inversion techniques to obtain quantitative measures of effective spectral resolution for multi-channel color mosaic CCDs. These techniques also allow us to explore the possibility of further improvements by modifying or combining multiple detectors. We consider two spectrally calibrated commercial color CCDs (Sony ICX285AQ and ICX429AKL) in order to determine effective wavelength resolution of each device individually, together, and with additional filters. From these results we develop methods to enhance the utility of existing data sets, and propose ways to improve the next generation of low-cost color auroral imaging systems.


1997 ◽  
Author(s):  
G. Germany ◽  
P. Richards ◽  
G. Parks ◽  
M. Brittnacher ◽  
G. Germany ◽  
...  
Keyword(s):  

2009 ◽  
Vol 114 (A1) ◽  
pp. n/a-n/a ◽  
Author(s):  
S. B. Mende ◽  
H. U. Frey ◽  
J. McFadden ◽  
C. W. Carlson ◽  
V. Angelopoulos ◽  
...  

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