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Spatial and Spectral Characteristics of the Near-Infrared Aurorae of Jupiter
Ist Teil von
Icarus (New York, N.Y. 1962), 1993-03, Vol.102 (1), p.99-106
Ort / Verlag
Legacy CDMS: Elsevier Inc
Erscheinungsjahr
1993
Quelle
Elsevier Journal Backfiles on ScienceDirect (DFG Nationallizenzen)
Beschreibungen/Notizen
We obtained near-infrared images and spectra of the Jovian aurorae using the CRSP (Cryogenic Spectrometer) on the KPNO 2.1-m telescope on January 22, 1992 (UT). The slit of the CRSP was aligned with 63° north and south latitudes in order to study the spatial structure of the auroral emission between 2 and 4μm. The spatial resolution was about 3 arcsec with spectral resolving powers of about 1000 and 700 for 2 and 4 μm, respectively. We obtained spatially resolved emission intensities of (1) H
+
3 fundamental band lines between 3 and 4 μm and (2) the H
2 quadrupole lines of Q
1(1), Q
1(3), and S
1(1), and several H
+
3 lines between 2 and 2.5 μm in the northern auroral region. The northern bright spot as seen in the 2-μm H
2 and H
+
3 emission lines is at nearly the same position as the northern bright spot due to the H
+
3 fundamental band lines. We derived spatially resolved rotational temperatures from the H
+
3 lines in the north polar region and found that temperatures on the bright spot are no greater than those in other auroral regions. This suggests an enhanced abundance of H
+
3 on the bright spot relative to other parts of the auroral zone. We found the southern H
+
3 line intensities to be much lower than those in the northern auroral zone, suggesting a lower level of auroral activity near the south pole at the time of the observations. The continuum near the known H
+
3 lines in the 3.17- to 3.57-μm region shows a significant brightening around the northern bright spot position, implying that the continuum contains many weak unidentified emissions, which are correlated with the auroral activity.