Efficient signal collection has been a major problem in the development of observational instrumentation systems since their beginnings. One of the earliest approaches to this problem involves the utilization of photographic techniques. Light sensi tivie emulsions (photographic plates) have been used for recording images at the focal point of a telescope since the middle of the 18th century. Similarly, they have been used for recording the spectra produced by various spectrographs for nearly 75 years. The ion-sensitive photo-plate has been the traditional method for recording mass spectra since Thomson (1) and, particularly, Aston (2) built their first mass spectrographs .Unfortunately, it is not free of a number of problems, as will be shown below. The efforts made to solve some of the shortcomings attending its general use have been discussed by Ahearn (3) and Honig (4).
In principle, the photographic plate is ideally suited for simultaneously detecting and integrating the signal from all ion species over an extended mass range, limited only by the ion optics of the mass analyzer, with good resolution (typically > 100 lines/mm).However, its sensitivity is limited, its use awkward, and the conversion of the image to numerical data is time consuming and costly. The limited sensitivity (it takes from 103 to 10^ ions to produce a measurable line) and its associated lack of dynamic range (typically in the order of 30:1) have severely limited the use of photographic plates in routine applications of mass spectrometry. The search for alternate ion detection systems has resulted in the wide-spread use of electrical detection systems.Modern implementation of these devices drastically shortens the time required to collect both quantitative and qualitative analytical results and greatly simplify the associated data reduction problems.Conventional electrical detection devices are based upon sweeping the resolved ion beam 0-8412-0504-3/79/47-102-291$07.00/0