Photosynthetic photon flux density, red:far-red ratio, and minimum light requirement for survival of Gaultheriashallon in western red cedar–western hemlock stands in coastal British Columbia

1989 ◽  
Vol 19 (11) ◽  
pp. 1470-1477 ◽  
Author(s):  
Christian Messier ◽  
Terry W. Honer ◽  
James P. Kimmins

Measurements of photosynthetic photon flux density (PPFD; global, diffuse, and direct: 400–700 nm) and red:far-red ratio (660:730 nm) were made above and below an understory of salal (Gaultheriashallon Pursh) within three western red cedar (Thujaplicata Donn)–western hemlock (Tsugaheterophylla (Raf.) Sarg.) stands on the northern end of Vancouver Island, British Columbia. These stands were chosen to represent a wide range of canopy closure and understory salal cover. The measurements were repeated under both clear and overcast sky conditions. Within each stand, the percent cover, height, number of stems per hectare, and leaf morphology of the salal were measured. As expected, there was a decrease in both the salal cover and in the global PPFD and red:far-red ratio measured directly above salal as the percent tree cover increased. Salal leaf thickness and specific leaf weight decreased, whereas its leaf area increased, as global PPFD and red:far-red ratio decreased. The results indicate that the minimum light requirement for salal survival is between 3.9 and 11.1 μmol•m−2•s−1 (1.2 to 3.3% of global PPFD measured in an adjacent clearing) and 4.5 and 27.2 μmol•m−2•s−1 (0.3 to 1.8% of global PPFD measured in the clearing) under overcast and clear sky conditions, respectively. The global PPFD and red:far-red ratio measured 30 cm above the forest floor (beneath the salal) did not vary widely among the three stands. At this level, global PPFD values were very low, ranging from 0.15 to 0.35% and 0.58 to 0.75% of the global PPFD measured in the clearing under clear and overcast sky conditions, respectively. Red:far-red ratios at the forest floor level varied from 0.13 to 0.25 and 0.40 to 0.58 under clear and overcast sky conditions, respectively. The silvicultural implications of the results are discussed.

2019 ◽  
Vol 11 (8) ◽  
pp. 932
Author(s):  
Megumi Yamashita ◽  
Mitsunori Yoshimura

A knowledge of photosynthetic photon flux density (PPFD: μmol m−2 s−1) is crucial for understanding plant physiological processes in photosynthesis. The diffuse component of the global PPFD on a short timescale is required for the accurate modeling of photosynthesis. However, because the PPFD is difficult to determine, it is generally estimated from incident solar radiation (SR: W m−2), which is routinely observed worldwide. To estimate the PPFD from the SR, photosynthetically active radiation (PAR: W m−2) is separated from the SR using the PAR fraction (PF; PAR/SR: unitless), and the PAR is then converted into the PPFD using the quanta-to-energy ratio (Q/E: μmol J−1). In this procedure, PF and Q/E are considered constant values; however, it was reported recently that PF and Q/E vary under different sky conditions. Moreover, the diffuse ratio (DR) is needed to distinguish the diffuse component in the global PAR, and it is known that the DR varies depending on sky conditions. Ground-based whole-sky images can be used for sky-condition monitoring, instead of human-eye interpretation. This study developed a methodology for estimating the global and diffuse PPFD using whole-sky images. Sky-condition factors were derived through whole-sky image processing, and the effects of these factors on the PF, the Q/E of global and diffuse PAR, and the DR were examined. We estimated the global and diffuse PPFD with instantaneous values using the sky-condition factors under various sky conditions, based on which the detailed effects of the sky-condition factors on PF, Q/E, and DR were clarified. The results of the PPFD estimations had small bias errors of approximately +0.3% and +3.8% and relative root mean square errors of approximately 27% and 20% for the global and diffuse PPFD, respectively.


2005 ◽  
Vol 60 (6) ◽  
pp. 1161-1163
Author(s):  
Jun-ichi MOGAMI ◽  
Takashi HIRANO ◽  
Ryuichi HIRATA ◽  
Satoshi KITAOKA ◽  
Takayoshi KOIKE ◽  
...  

1996 ◽  
Vol 26 (1) ◽  
pp. 151-154 ◽  
Author(s):  
Sylvain Parent ◽  
Christian Messier

This study presents a new, simple, and efficient method for estimating microsite light availability in the understory of a forest. The percentage of above-canopy photosynthetic photon flux density (%PPFD) transmitted above 16 microsites in the understory of a mixed conifer–broadleaf forest was measured every minute between 07:00 and 19:00 for both a completely overcast and a cloudless day. Instantaneous measures of %PPFD were also taken at different times on 3 overcast days. The instantaneous measures of %PPFD were strongly and directly related (P < 0.001) among themselves and with mean daily %PPFD values. These results demonstrate the usefulness of using an instantaneous measure of %PPFD taken under overcast sky conditions for estimating the mean daily %PPFD at any microsite under a forest canopy.


2020 ◽  
Vol 10 (22) ◽  
pp. 8007
Author(s):  
Ana García-Rodríguez ◽  
Sol García-Rodríguez ◽  
Montserrat Díez-Mediavilla ◽  
Cristina Alonso-Tristán

Plant growth is directly related to levels of photosynthetic photon flux density, Qp. The improvement of plant-growth models therefore requires accurate estimations of the Qp parameter that is often indirectly calculated on the basis of its relationship with solar irradiation, RS, due to the scarcity of ground measurements of photosynthetic photon flux density. In this experimental campaign in Burgos, Spain, between April 2019 and January 2020, an average value of the Qp/Rs ratio is determined on the basis of measurements at ten-minute intervals. The most influential factor in the Qp/Rs ratio, over and above any daily or seasonal pattern, is the existence of overcast sky conditions. The CIE standard sky classification can be used to establish an unequivocal characterization of the cloudiness conditions of homogeneous skies. In this study, the relation between the CIE standard sky type and Qp/Rs is investigated. Its conclusions were that the Qp/Rs values, the average of which was 1.93±0.15 μmol·J−1, presented statistically significant differences for each CIE standard sky type. The overcast sky types presented the highest values of the ratio, while the clear sky categories presented the lowest and most dispersed values. During the experimental campaign, only two exceptions were noted for covered and partial covered sky-type categories, respectively, sky types 5 and 9. Their values were closer to those of categories classified as clear sky according to the CIE standard. Both categories presented high uniformity in terms of illumination.


Author(s):  
M. Yamashita ◽  
M. Yoshimura

Photosynthetic photon flux density (PPFD:&amp;thinsp;&amp;micro;mol&amp;thinsp;m<sup>&amp;minus;2</sup>&amp;thinsp;s<sup>&amp;minus;1</sup>) is indispensable for plant physiology processes in photosynthesis. However, PPFD is seldom measured, so that PPFD has been estimated by using solar radiation (SR: W&amp;thinsp;m<sup>&amp;minus;2</sup>) measured in world wide. In method using SR, there are two steps: first to estimate photosynthetically active radiation (PAR: W&amp;thinsp;m<sup>&amp;minus;2</sup>) by the fraction of PAR to SR (<i>PF</i>) and second: to convert PAR to PPFD using the ratio of quanta to energy (<i>Q&amp;thinsp;/&amp;thinsp;E</i>: &amp;micro;mol&amp;thinsp;J<sup>&amp;minus;1</sup>). PF and <i>Q/E</i> usually have been used as the constant values, however, recent studies point out that <i>PF</i> and <i>Q&amp;thinsp;/&amp;thinsp;E</i> would not be constants under various sky conditions. In this study, we use the numeric data of sky-conditions factors such cloud cover, sun appearance/hiding and relative sky brightness derived from whole-sky image processing and examine the influences of sky-conditions factors on <i>PF</i> and <i>Q&amp;thinsp;/&amp;thinsp;E</i> of global and diffuse PAR. Furthermore, we discuss our results by comparing with the existing methods.


Plants ◽  
2022 ◽  
Vol 11 (1) ◽  
pp. 143
Author(s):  
Neringa Rasiukevičiūtė ◽  
Aušra Brazaitytė ◽  
Viktorija Vaštakaitė-Kairienė ◽  
Alma Valiuškaitė

The study aimed to evaluate the effect of different photon flux density (PFD) and light-emitting diodes (LED) wavelengths on strawberry Colletotrichum acutatum growth characteristics. The C. acutatum growth characteristics under the blue 450 nm (B), green 530 nm (G), red 660 nm (R), far-red 735 nm (FR), and white 5700 K (W) LEDs at PFD 50, 100 and 200 μmol m−2 s−1 were evaluated. The effect on C. acutatum mycelial growth evaluated by daily measuring until five days after inoculation (DAI). The presence of conidia and size (width and length) evaluated after 5 DAI. The results showed that the highest inhibition of fungus growth was achieved after 1 DAI under B and G at 50 μmol m−2 s−1 PFD. Additionally, after 1–4 DAI under B at 200 μmol m−2 s−1 PFD. The lowest conidia width was under FR at 50 μmol m−2 s−1 PFD and length under FR at 100 μmol m−2 s−1 PFD. Various LED light wavelengths influenced differences in C. acutatum colonies color. In conclusion, different photosynthetic photon flux densities and wavelengths influence C. acutatum growth characteristics. The changes in C. acutatum morphological and phenotypical characteristics could be related to its ability to spread and infect plant tissues. This study’s findings could potentially help to manage C. acutatum by LEDs in controlled environment conditions.


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