PubMed HealthSearch

PubMed · 6815752

Density-dependent airflow and ventilatory control during exercise.

Abstract

The influence of respired gas density on ventilatory control during cycle-ergometer exercise was investigated in six healthy subjects. They underwent constant-load exercise for 10 min both at 50% and 90% of the anaerobic threshold, inhaling air for the first 5 min followed abruptly by 80% helium-20% oxygen (He-O2) for the remaining 5 min (and vice versa). The He-O2 breathing elicited no discernible effect on ventilation (VI) or mean alveolar PCO2 (PACO2) at rest or at the lower work rate. However, at the higher work rate, He-O2 breathing resulted in a clear and sustained hyperventilation in all subjects. A compensatory response to the hypocapnia, consequent to the helium-induced hyperventilation, was not evident even though all subjects demonstrated a normal ventilatory responsiveness to inhaled CO2 while in this condition. These observations suggest that turbulent airflow normally imposes a constraint on the magnitude of the hyperpnea of high-intensity exercise.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

S A Ward, B J Whipp, C S Poon. 1982. Density-dependent airflow and ventilatory control during exercise.. https://doi.org/10.1016/0034-5687(82)90116-5

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related citations

A possible high-temperature origin for the carbonates in the martian meteorite ALH84001.

The meteorite Allan Hills (ALH) 84001, commonly accepted to be of martian origin, is unique among known martian meteorites in containing abundant, zoned, pre-terrestrial carbonate minerals. Previous studies of the oxygen isotope compositions of these minerals have suggested that they precipitated from a low-temperature (0-80 degrees C) aqueous fluid in the martian crust--perhaps in a near-surface hydrothermal system. Here we report analyses of the major-element compositions of the carbonates, which provide an independent constraint on the composition and temperature of the fluid from which they formed. We argue that the most likely explanation for the observed compositions, and for the absence of co-existing hydrons minerals, is that the carbonates were formed by reactions between hot (> 650 degrees C), CO2-rich fluids and the ultramatic host rock during an impact event. Impact processes on the martian surface can produce both the hot, CO2-rich fluid (by volatilization of surface carbonates or other CO2 sources) and--by brecciation--the condults through which it flowed. Impact metasomatism is also consistent with the observed oxygen isotope disequillbrium, sequence of mineral formation, and carbonate mineral zoning, reflecting carbonate formation during rapid cooling from high temperatures rather than prolonged exposure to low-temperature fluids.

Carbon Dioxide

Differential D1 dephosphorylation in functional and photodamaged photosystem II centers. Dephosphorylation is a prerequisite for degradation of damaged D1.

Light dependence and kinetics of reversible phosphorylation of the D1 reaction center protein of Photosystem II was studied in pumpkin leaves. At growth light, maximal phosphorylation of D1 was observed after illumination of 1 h, with higher phosphorylation rates at stronger irradiances. 70-85% of D1 became phosphorylated, corresponding to the proportion of the protein in appressed thylakoid membranes. Comparison of the kinetics of D1 phosphorylation and photoinactivation of Photosystem II revealed that D1 phosphorylation became saturated before any significant photoinhibition of Photosystem II could be detected. Dephosphorylation of D1 in both dim light and darkness was determined in leaves preilluminated with high light for various periods. Similar rates of D1 dephosphorylation were observed after short preillumination conditions that induce no significant loss of functional Photosystem II centers. In contrast, photodamage to Photosystem II centers significantly decreased the dephosphorylation rate of D1 in darkness, and no dephosphorylation occurred in leaves containing mainly damaged Photosystem II centers. Darkness also blocked the degradation of damaged D1 after photoinhibitory preillumination. Degradation of damaged D1 could be prevented even in dim light by sodium fluoride, an inhibitor of protein phosphatases, indicating that dephosphorylation is a prerequisite for D1 proteolysis. We conclude that in higher plants (i) high light induced photodamage to Photosystem II occurs in the centers containing phosphorylated D1. (ii) Dephosphorylation of phosphorylated and photodamaged D1 is associated with the repair cycle of inactivated Photosystem II and is a light-dependent reaction in vivo. (iii) Dephosphorylation of D1 in functional Photosystem II centers, however, occurs rapidly and independent of light. We suggest that two reversible phosphorylation cycles with spatially segregated protein phosphatases are involved in dephosphorylation of functional and damaged phosphorylated D1, respectively.

Carbon Dioxide