Our results confirm Saunders’ data of Nasonia diapause responses in a full Nanda-Hamner landscape (Saunders 1968, 1974). Our partial Nanda-Hamner protocol was not designed to confirm a positive Nanda-Hamner response showing circadian involvement in photoperiodism. Instead, our comparison between the northern and southern line provides additional evidence that latitudinal adaptation in Nasonia may be caused by differences in properties of the circadian system, resulting in adaptive differences in photoperiodic responses. The northern Nasonia line shows in different T-cycles a positive response and variation in CPP; with longer CPP in longer T-cycles and shorter CPP in short Tcycles. These differences became slightly smaller when plotting the data as a function of critical night length, but still the curves did not superimpose. This may indicate that the photoperiodic system in the northern Nasonia line responds to both day length and night length.
In the southern line clear diapause induction just occurred in T-21 h and T-24 h with different CPP that was longer in T-24 h than in T-21 h but lay on top of each other when plotted as a function of critical night length. This suggests that the southern Nasonia line may measure night length rather than day length. The lack of diapause induction in the southern line at T-18 h, T-27 h and T-30 h may indicate that there was no entrainment (the system is not in ‘resonance’), and that light perceived at all phases of the circadian cycle resulted in effective suppression of diapause. This can be considered as evidence that the system does not respond as an hour glass model, where diapause should have occurred in all T-cycles at short photoperiods.
In his complete Nanda-Hamner study, David Saunders used a Nasonia line originating from Cambridge, United Kingdom (52°12’19.213’’N, 0°7’18.541’’E; Saunders 1968, 1974), an intermediate latitudinal location between Oulu, Finland (65°3’40.16’’N, 25°31’40.80’’E) and Corsica, France (42°22’40.80’’N, 8°44’52.80’’E). Re-plotting Saunders results (Fig. 3) from T-cycles similar to cycle lengths that we used, we find similarities to both our northern and the southern data (Fig. 2A, B & Fig. 3). T-16 h, T-21 h, T-24 h, T-28 h show diapause induction at long photoperiods. T-32 h does not show more than 25% diapause induction, similar to results shown by the southern line (Fig. 2B). We conclude that the results of Saunders also support our conclusion since those data show intermediate diapause induction responses when compared to our northern and southern data, while the geographical origin of the Saunders strain was also intermediate to the strains we used.
Saunders collected large data sets when he applied night interruption experiments (Saunders 1970) and the Nanda-Hamner protocol (Saunders 1974). Both experimental approaches led to the conclusion of a circadian based seasonal timing mechanism. Further, Saunders wanted to determine oscillator properties, especially whether internal or external coincidence model drives seasonal timing. At the time, he interpreted his findings as internal coincidence model based on the position of the ascending and descending slope of the peak of the photoperiodic response curve. “…When the photoperiod was increased from 12 h to 14 or 16 h the ‘descending slope‘ of the peaks remained in the same position (at T = 28–32 and at T = 52–56), but the ‘ascending slope’ moved to longer T values in such a way that the maxima became narrower. …. A similar, but opposite trend was observed when the photoperiod was shortened; the ‘ascending slope’ moved steadily to the left, whereas the ‘descending slope’ remained constant, except with the 4 h photoperiod in which a perceptible movement to left was also apparent.“ (Saunders 1974). He connected the ascending slopes with dusk and the descending slopes with dawn and by that he drew the conclusion of an internal coincidence model with a morning oscillator tracking dawn and an evening oscillator tracking dusk (Saunders 1974).
Here we propose an alternative explanation based upon an external coincidence timing model, similar to the photoperiodic timing mechanism located in the mammalian Pars tuberalis (Dardente et al. 2010, Masumoto et al. 2010). Essential for evaluation of the involvement of circadian components in photoperiodic timing in unusual T-cycles is whether the circadian system is able to entrain or not, especially in absence of photoperiodic response as shown in the southern Nasonia line (Fig. 2B, D). In prior experiments phase response curves were conducted of females of the northern and southern lines to light pulses of the same light intensity as used here, where light pulses of 4 h or more resulted in phase shifts of more than 7 h advance or delay (Floessner et al. 2019). This means that both the northern (tau = 26.33 h) and the southern line (tau = 25.01 h) probably entrained to all T-cycles presented here. Assuming that circadian entrainment indeed occurred in both lines under all Tcycles, we consider the difference in light sensitivity of the northern and southern line as a possible explanation for the difference in diapause response. The higher light sensitivity in the northern line should result in a shallower phase-period relationship under a range of T-cycles than would be the case with the southern line with a lower light sensitivity (Floessner and Hut 2017). This means that with increasing duration of the Tcycle, the southern line would show a stronger effect on phase (more ‘leading’) than the northern line. This indeed seems to be the case when activity profiles for the northern and southern lines are considered for T-20 h, T-24 h and T-28 h LD cycles (Floessner et al. 2019). When this difference in phase-period relationship between the northern and southern line is applied to an external coincidence model, we can construct a graphical representation model that summarizes our results (Fig. 4). In this model we assume that diapause is suppressed when a single light sensitive phase of ~ 7 h duration would be exposed to light. This light sensitive phase would be coupled to the circadian system and is entrained around the middle of the light phase (Floessner et al. 2019). This parsimonious model can explain all diapause responses presented here when lower light sensitivity in the southern line (Floessner et al. 2019) results in a reduced range of entrainment and a wider phase angle of entrainment range (Floessner and Hut 2017) when compared to the northern line (Fig. 4). The narrower range of phase angle of entrainment in the northern line, resulting from their higher light sensitivity, would then lead to a narrower phase distribution of the light sensitive phase, and hence more similar responses in maintaining diapause at shorter photoperiods at all T-cycles applied (Fig. 4). The wider phase distribution in the southern line, due to their lower circadian light sensitivity, would therefore result in maintenance of diapause only in those T-cycles with a period relatively close to the intrinsic circadian period of that line.
Our ‘external coincidence - phase angle of entrainment’ (EX-PA) model seems in line with the interpretation by Vaze and Helfrig-Förster (2016) that a tight range of phase angle of entrainment may indicate either a weak or dampened oscillator that can be easily entrained by light, or a strong oscillator that can be easily entrained because of a high response/sensitivity to light. Under entrained conditions, these two options can only be distinguished by an independent measure of oscillator strength, perhaps through establishing the robustness of activity rhythms, and by measuring the strength of the circadian light responses. Both measures, robustness of activity profiles and strength of circadian light resetting, seem to indicate that Nasonia has a strong circadian oscillator with strong circadian light resetting, especially in the northern line (Floessner et al. 2019). As a next step, it would be interesting to see to what extent our EX-PA model can explain the full extent of the photoperiodic landscape model as measured by Saunders (1974).
To further support our EX-PA model, we would need better confirmation on the phase angle of entrainment under various T-cycles and we would need to increase our understanding of the system using a wider range of photoperiods and T-cycles applied to a wider range of Nasonia strains. Given the results presented here, we draw the preliminary conclusion that the different diapause responses in our northern and southern lines can be explained (at least partly) by an external coincidence timing model while taking into account the higher circadian light sensitivity in the northern line. This interpretation indicates that variation in circadian light sensitivity, together with adaptation in circadian period, may form the basis for latitudinal adaptation in photoperiod driven seasonal diapause response.