Diurnal variations of serum erythropoietin at sea level and altitude

1996 ◽  
Vol 72 (4) ◽  
pp. 297-302 ◽  
Author(s):  
Tom Klausen ◽  
Troels Dirch Poulsen ◽  
Niels Fogh-Andersen ◽  
Jean-Paul Richalet ◽  
Ove Juel Nielsen ◽  
...  
Author(s):  
Antonio Viruez-Soto ◽  
Mónica Marlene López-Dávalos ◽  
Gabriel Rada-Barrera ◽  
Alfredo Merino-Luna ◽  
Daniel Molano-Franco ◽  
...  

In the 13 years which have elapsed since Mr. Blanford published his paper on the Winds of Northern India, very great additions have been made to our knowledge of the meteorology of the country. The carefully organised system of observations, commenced in Bengal and the North-Western Provinces, has been extended to include the whole of India, and placed under the direction of Mr. Blanford himself, aided by local officers in all the larger provinces. Verified instruments have been supplied to all the stations, and the elevations of these above sea-level have been determined by connecting them with the lines of spirit-levelling, carried inland from the coast, in various directions, by the officers of the Great Trigonometrical Survey; or, where this was impracticable, by spirit-levelling to some of the trigonometrical stations of the Survey. In this way, trust worthy and intercomparable series of barometric observations, extending over ten years or more, have been obtained for all the more important stations. At the same time, the diurnal variations of the barometer at certain selected stations have been determined by long-continued series of hourly observations, with the object of enabling us to reduce the readings made in the ordinary way (usually at 10 a. m. and 4 p. m.) to time daily means. Simultaneously with the collection of this immense quantity of accurate and reliable barometric data, observations have been made of temperature, humidity, cloud, wind, and rain. Latterly also barometric and wind charts of the Bay of Bengal have been prepared from observations made on board ships navigating those waters. During these 13 years, the winds prevailing over the Indian continent and the Bay of Bengal, and their relations to the distribution of pressure at sea-level, have been discussed from time to time, both in their normal aspects for each month or season and in their abnormal or disturbed conditions during the passage of storms. The latter conditions in particular have been very fully described by Mr. Eliot in his numerous reports on cyclones in the Bay of Bengal, while the former have been noticed in the annual reports on the meteorology of India, in occasional papers appearing in the ‘Indian Meteorological Memoirs,' and latterly in a broad and general review in Mr. Blanford’s great monograph on the Rainfall of India.


Author(s):  
Richard Michler

The total increase of leaf area and the rate of water movement in the stems of Coffea arabica L. and Citrus aurantium sinensis Engler were deter- *) Gekürzte Fassung einer am 18. 12. 1969 von der Naturwissenschaftlichen Fakultat der Universitát Giessen als Dissertation angenommenen Abhandlung. mined in various climatic regions of Columbia. During the rain season the maximum rate of water transport decreased with increasing height above sea level. This effect was observed to be more evident in Citrus than in Coffea. At the end of the dry season however, the maximum rate of water movement was measured in 1250 m (Citrus) and 1850 m (Coffea) above sea level. In case of sunshine the maximum values were higher than in case of clouded sky. The most considerable increase of total leaf area was reached at Coffea in 1850 m and at Citrus in 1250 m respectively. With reference to the water economy the cultivation of Citrus could be forced in sea levels about 1250 m with simultaneous displacement of Coffea cultivation to colder climatic regions. Diurnal variations showed, that if the intensity of radiation increased suddenly, the rate of water movement in the stems of Citrus trees accordingly increased. With Coffea trees different results were obtained. During the morning the rate of water transport in trees always increased. At noon the values either remained high or varied in irregular intervals. Moreover, in the hot climatic regions diurnal variations sometimes showed two maximums of rate of water flow in the stems of Coffea arabica. Above all, the type of observed diurnal variations depended on the sea level distance of the measuring point, the season, the intensity of radiation and the species of plant.


1993 ◽  
Vol 67 (6) ◽  
pp. 545-548 ◽  
Author(s):  
Tom Klausen ◽  
Flemming Dela ◽  
Erik Hippe ◽  
Henrik Galbo

1968 ◽  
Vol 46 (10) ◽  
pp. S825-S827
Author(s):  
M. Kodama ◽  
K. Nagashima

Two pieces of experimental evidence, which are inconsistent with the hypothesis of a one-way solar anisotropy as an interpretation of the cosmic-ray diurnal variation, are presented. The diurnal variation of the temperature-corrected meson component at Deep River was examined and compared with that of the neutron component. Both diurnal variations were averaged for each solar rotation from No. 1762 to No. 1787. If a one-way solar anisotropy is assumed, the time of maximum for neutrons should be about half an hour earlier than that for mesons at Deep River. However, the observations show that the phase difference between the two components is the reverse of that expected. Further evidence is obtained from a comparison of the diurnal variation on Mt. Norikura (2 770 m, 11.4 GeV) to that in Itabashi (20 m, 11.5 GeV). According to theoretical calculations based on a one-way solar anisotropy, the time of maximum at high altitude is earlier than or equal to that at sea level, but observations obtained during Dec. 1966 to Mar. 1967 suggest that the opposite is true.


1985 ◽  
Vol 59 (2) ◽  
pp. 360-364 ◽  
Author(s):  
J. S. Milledge ◽  
P. M. Cotes

Serum immunoreactive erythropoietin (siEp) was estimated in samples collected from members of two scientific and mountaineering expeditions, to Mount Kongur in Western China and to Mount Everest in Nepal. SiEp was increased above sea-level control values 1 and 2 days after arrival at 3,500 m and remained high on ascent to 4,500 m. Thereafter, while subjects remained at or above 4,500 m, siEp declined, and by 22 days after the ascent to 4,500 m was at control values but increased on ascent to higher altitude. Thus siEp was at a normal level during the maintenance of secondary polycythemia from high-altitude exposure. On descent, with removal of altitude hypoxia, siEp decreased, but despite secondary polycythemia levels remained measurable and in the range found in subjects normally resident at sea level. On Mount Everest, siEp was significantly (P less than 0.01) elevated above preexpedition sea-level controls after 2–4 wk at or above 6,300 m. There was no correlation between estimates of siEp and plasma renin activity in samples collected before and during both expeditions.


1956 ◽  
Vol 9 (4) ◽  
pp. 505
Author(s):  
RM Jacklyn

The records from a vertical counter telescope measuring the hard component of cosmic radiation at sea-level have disclosed significant diurnal variations of the barometer coefficient at Hobart, Tas. The amplitude of the variation is about 5 per cent., and there are secular changes of the same order during the mean day.


1975 ◽  
Vol 26 ◽  
pp. 395-407
Author(s):  
S. Henriksen

The first question to be answered, in seeking coordinate systems for geodynamics, is: what is geodynamics? The answer is, of course, that geodynamics is that part of geophysics which is concerned with movements of the Earth, as opposed to geostatics which is the physics of the stationary Earth. But as far as we know, there is no stationary Earth – epur sic monere. So geodynamics is actually coextensive with geophysics, and coordinate systems suitable for the one should be suitable for the other. At the present time, there are not many coordinate systems, if any, that can be identified with a static Earth. Certainly the only coordinate of aeronomic (atmospheric) interest is the height, and this is usually either as geodynamic height or as pressure. In oceanology, the most important coordinate is depth, and this, like heights in the atmosphere, is expressed as metric depth from mean sea level, as geodynamic depth, or as pressure. Only for the earth do we find “static” systems in use, ana even here there is real question as to whether the systems are dynamic or static. So it would seem that our answer to the question, of what kind, of coordinate systems are we seeking, must be that we are looking for the same systems as are used in geophysics, and these systems are dynamic in nature already – that is, their definition involvestime.


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