The murine fast PIII ERG component recorded from the isolated aspartate-treated retina to rod-saturating flash stimuli contains a fast “nose”-like component (Heikkinen, Nymark, & Koskelainen,
2008; Nymark, Heikkinen, Haldin, Donner, & Koskelainen,
2005) that is either weak or not present in the fast rod PIII photoresponses of amphibian retinas. The “nose” was first observed by Arden (
1976) in rat rod photoresponses, and it is also present in photoresponses recorded from intact APB-treated (2-amino-4-phosphonobutyrate) cat eyes (Kang Derwent & Linsenmeier,
2001) as well as in APB-treated monkey rod PIII responses (Jamison, Bush, Lei, & Sieving,
2001). It is generally believed that the leading edge of the a-wave of the ERG accurately reflects the changes in the circulating current of rods and cones (Breton, Schueller, Lamb, & Pugh,
1994; Hood & Birch,
1990,
1993; Robson, Saszik, Ahmed, & Frishman,
2003; Smith & Lamb,
1997), thereby giving information on the amplification of phototransduction in rods and cones (Lamb & Pugh,
1992; Pugh & Lamb,
1993). Since the time course of the nose overlaps with the initial part of the saturated and nearly saturated PIII responses, we found it important to clarify the nature and origin of the nose. It is worth noting that although the ionic mechanisms carrying currents across the photoreceptor cell membranes have been extensively characterized in older studies (e.g., Bastian & Fain,
1982; Brown & Pinto,
1974; Fain, Quandt, Bastian, & Gerschenfeld,
1978), it is not at all straightforward to resolve which are the molecular mechanisms involved in creating the radial current dipole (the source/sink pair) that is generated consequent to the closure of cGMP-gated channels and that creates the nose. We therefore chose to use the ERG of the isolated mouse retina that easily allows manipulation of the current generating mechanisms in the rod plasma membrane, and that directly shows when a mechanism in the source/sink pair is affected.