How Linear Are Typical CCDs?

The typical linearity achievable with CCDs was questioned at the previous ESO Optical Detector Workshop in 1993. This paper describes the efforts at CTIO since then to develop a technique for measuring linearity accurately, and rapidly enough to make the exploration of CCD operating parameters practical. A simple circuit has been adopted which stabilizes the intensity of a pulsed LED. It is compact enough to be installed behind the shutter so that linearity can be monitored at the telescope while the dome lights are on. Methods are described for verifying the linearity and stability of the measurement system itself. These requirements are very stringent, since CCD gain variations have typically been measured to be 0.2% or less over most of the operating range. Methods are proposed for reducing non-linearity further, and for generating each new linearity curve from a single exposure, after having taken several calibration exposures. Several discrepancies have been seen between linearity of point sources and linearity measured with flat illumination: the amplitudes were similar but the gain variations had opposite slopes over the central part of the curve, and a more pronounced signal deficit has been noted at low light levels for point sources, which is equivalent to the subtraction of few electrons from every pixel.     

A record of the upper Cochiti polarity transition from the Southern Hemisphere (FIJI)

We sampled the upper Cochiti polarity transition recorded in the Suva Marl in Fiji (18° S, 178° E). The Suva Marl accumulated at an average rate of 83.2 m/m.y. and provides a unique opportunity to address the question of whether present-day overprints bias the transition records. Fiji has undergone a 30° counterclockwise rotation since the deposition of the Suva Marl and hence a present day overprint onto the transitions would bias the VGPs toward the east of the site. Replicate transition records yield VGPs over both Asia and the Americas. Progressive demagnetization reveals a normal polarity overprint which was acquired prior to the rotation of Fiji, and therefore does not produce an easterly bias to the transition data even after correction for the rotation. We collected an oriented block sample across a portion of the transitional interval in the upper Cochiti reversal. Subsampling of this block into 1.0 cm thick wafers cut parallel to bedding provides considerably greater detail during the transition. These detailed data suggest that the oscillatory movement of the VGPs in these sections may be a result of the averaging caused by standard, detailed minicoring and not by the sediments or the remanence acquisition process.     

Ducted whistler-mode signals received at two widely spaced locations

Whistler-mode signals from a single VLF transmitter that have propagated in the same duct, have been observed simultaneously at Faraday, Antarctica (65°S, 64°W) and Dunedin, New Zealand (46°S, 171°E). The signals received have group-delay times that differ in the order of 10 ms, which can be explained by the differences in southern-hemisphere sub-ionospheric propagation time from duct exit region to receiver for the two sites. This difference has been used to determine the location of the duct exit region, with confirmation provided by arrival-bearing information from both sites. The whistler-mode signals typically occur one or two days after geomagnetic activity, with K_p\geq5. The sub-ionospheric-propagation model, LWPC, is used to estimate the whistler-mode power radiated from the duct exit region. These results are then combined with estimated loss values for ionospheric and ducted transmission to investigate the role of wave-particle amplification or absorption. On at least half of the events studied, plasmaspheric amplification of the signals appears to be needed to explain the observed whistler-mode signal strengths.     

XVIIIth International Congress of Photogrammetry and Remote Sensing

The XVIIIth International Congress of Photogrammetry and Remote Sensing was held in the Austria Center, Vienna from 9th to 19th July, 1996. Reports on the Technical Commission Activities, on the Congress Exhibition and on the General Assembly were given at a meeting of the Photogrammetric Society on 7th October, 1996. Papers from the Congress were published in the International Archives of Photogrammetry and Remote Sensing, 31.     

An intercomparison of ESR and uranium series ages for quaternary speleothem calcites

Equivalent dose (ED) estimates for speleothem calcite derived by ESR measurements of the g = 2.0005 signal have a typical precision of ±7% (minimum ±2%), and depend on the signal strength, radiation sensitivity and the presence of interfering signals. Underestimation of ED will occur if the crushing signal at g = 2.0001 is not removed by acid etching, while overestimation may be caused if the short-lived radiation induced interfering signal at g = 2.0020 is not removed by annealing. Quoted errors for ESR ages are rarely better than ±10% and are typically ±15% because of uncertainties in ED, calibration of dosimeters and gamma source, and in the a-value. Serial analyses along the growth axis of single speleothems, and between speleothems interbedded in a sequence demonstrate excellent stratigraphic concordance. Intercomparison of ESR and uranium series ages for samples derived from 11 geographically diverse sites show good agreement with no indication of systematic error. Although validation is more difficult for samples beyond the limit of dating, the results appear encouraging, but recrystallisation and changes in the external radiation dose may cause problems.     

The rise and fall of the estuarine intertidal zone

Water level records from two study sites in Indian River Lagoon, along Florida’s Atlantic Coast, are used to characterize the vertical displacement of the estuarine intertidal zone in response to subtidal frequency forcing. A 22-year water level record indicates that the seasonal cycle has a range approximately one-quarter greater than the mean tidal range. The intertidal zone thus rises and falls to such an extent that over time scales in excess of several weeks there is no layer which consistently experiences an alternating exposure and inundation. Six-year sets of high and low tide extremes from the second study site are expressed in the form of cummulative histograms to determine the probabilities with which high tide and low tide levels lying outside of median values will occur in response to the interaction of tidal constituents and low-frequency forcing. High and low water values are then stratified by month, and probability distributions are recomputed for each subset. In this study area, unpredictable, low-frequency water level fluctuations perturb the intertidal zone to such an extent that the probabilities of extreme high and low water levels, in addition to mean high and low water, must be determined to characterize the stuarine intertidal zone adequately. *** DIRECT SUPPORT *** A01BY034 00002