Characterization of native pathogenic antigens of Onchocerca volvulus: identification of high molecular mass protein antigens eliciting interstitial keratitis in a guinea pig model.

Sclerosing keratitis is the predominant cause of blindness due to onchocerciasis which is a major human parasitic disease caused by the filarial parasite Onchocerca volvulus. In the present investigation, native pathogenic antigens of O. volvulus which are particularly potent in causing interstitial keratitis were characterized utilizing a guinea pig model. Following demonstration of the protein nature of these antigens using pronase digestion, the crude O. volvulus antigen extract was subjected to stepwise procedures of protein purification. At each stage of purification, pooled antigen fractions were injected into one cornea of presensitized guinea pigs followed by clinical evaluation of stromal inflammation and vascularization at different intervals of time after intrastromal challenge. Initial purification of the pathogenic antigens was carried out in the following order: molecular sieve chromatography on Bio-gel A-5m. anion exchange chromatography on Mono Q followed by DEAE-Sepharose CL-6B and cation exchange chromatography on Mono S. Two out of six different pools from the Mono S column (pool a eluted unbound at 10 mM-NaCl and pool e eluted between 130 mM and 475 mM-NaCl) were found to be most pathogenic. Further purification of Mono S pool a and pool e separately by gel filtration chromatography using Superose 12 demonstrated that the fractions which were most potent in inducing interstitial keratitis contained proteins with approximate molecular masses between 100 and 200 kDa. These results show that minor subfractions of total crude antigens of O. volvulus are largely responsible for induction of experimental interstitial keratitis. We have demonstrated the presence of these antigens in O. volvulus microfilariae by their cross-reactivities with anti-microfilarial antibodies, and hence the relevance of the purified antigens to ocular onchocerciasis in man since sclerosing keratitis is associated with invasion of the cornea by O. volvulus microfilariae. Isolation of these two pathogenic antigen pools represents the practical limits of purification and subsequent animal experiments possible with the available amounts of native parasite material obtained from infected human individuals in the absence of a suitable non-human host or of an in vitro culture system for O. volvulus.

Infiltration of CD4+ T cells into cornea during development of Onchocerca volvulus-induced experimental sclerosing keratitis in mice.

Sclerosing keratitis is the major cause of blindness due to onchocerciasis caused by the parasite Onchocerca volvulus. Although the importance of T cells in the pathogenesis of onchocerciasis has been suggested, their precise role in onchocercal sclerosing keratitis has not yet been defined. Using immunohistological techniques and a murine model of onchocercal sclerosing keratitis, we have performed a temporal analysis of the inflammatory T cells infiltrating into the cornea at Days 4, 7, and 21 following intrastromal challenge with soluble O. volvulus antigens into presensitized mice. The maximum number of CD3+ T cells were observed in the corneal stroma at Day 21 when sclerosing keratitis was most severe. The majority (> 85%) of the CD3+ T cells were CD4+ at all time points. A few infiltrating cells bore IL-2 receptors indicating possible activation of a small fraction of the T cells. These results suggest that CD4+ T cells play an important role in onchocercal sclerosing keratitis.

Immune-mediated Onchocerca volvulus sclerosing keratitis in the mouse.

Sclerosing keratitis is the major cause of blindness due to onchocerciasis; its pathogenesis is poorly understood. We have previously reported an immune-mediated model of experimental interstitial keratitis in guinea pigs following intrastromal challenge with soluble antigens from Onchocerca volvulus. This model system is ideal for evaluation of pathogenicity of multiple purified antigen preparations; however, reagents necessary for detailed immunologic analysis of the inflammatory cellular infiltrate are not yet available for guinea pigs. Because of the ready availability of these reagents for mice, a mouse model has been developed. The inflammatory response observed in this model was analogous to that seen in human onchocercal sclerosing keratitis as well as in the guinea pig model of onchocercal sclerosing keratitis. Granulocytes were present in the acute inflammatory response, whereas the chronic response showed lymphocytes, plasma cells, and histiocytes. Neovascularization and scarring of the corneal stroma was also observed. This model will be helpful in examining the mechanisms of immunopathogenesis and the contribution of the host genetic background to the disease.

Very-Long-Baseline Radio Interferometry: The Mark III System for Geodesy, Astrometry, and Aperture Synthesis.

The Mark III very-long-baseline interferometry (VLBI) system allows recording and later processing of up to 112 megabits per second from each radio telescope of an interferometer array. For astrometric and geodetic measurements, signals from two radio-frequency bands (2.2 to 2.3 and 8.2 to 8.6 gigahertz) are sampled and recorded simultaneously at all antenna sites. From these dual-band recordings the relative group delays of signals arriving at each pair of sites can be corrected for the contributions due to the ionosphere. For many radio sources for which the signals are sufficiently intense, these group delays can be determined with uncertainties under 50 picoseconds. Relative positions of widely separated antennas and celestial coordinates of radio sources have been determined from such measurements with 1 standard deviation uncertainties of about 5 centimeters and 3 milliseconds of arc, respectively. Sample results are given for the lengths of baselines between three antennas in the United States and three in Europe as well as for the arc lengths between the positions of six extragalactic radio sources. There is no significant evidence of change in any of these quantities. For mapping the brightness distribution of such compact radio sources, signals of a given polarization, or of pairs of orthogonal polarizations, can be recorded in up to 28 contiguous bands each nearly 2 megahertz wide. The ability to record large bandwidths and to link together many large radio telescopes allows detection and study of compact sources with flux densities under 1 millijansky.