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Department of Medicine, University of California San Diego, La Jolla, California 92093-0623
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ABSTRACT |
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Barometric
pressures (PB) near the summit
of Mt. Everest (altitude 8,848 m) are of great physiological interest
because the partial pressure of oxygen is very near the limit for human
survival. Until recently, the only direct measurement on
the summit was 253 Torr, which was obtained in October 1981, but,
despite being only one data point, this value has been used by several
investigators. Recently, two new studies were carried out. In May 1997, another direct measurement on the summit was within ~1 Torr of 253 Torr, and meteorologic data recorded at the same time from weather
balloons also agreed closely. In the summer of 1998, over 2,000 measurements were transmitted from a barometer placed on the South Col
(altitude 7,986 m). The mean PB
values during May, June, July, and August were 284, 285, 286, and 287 Torr, respectively, and there was close agreement with the
PB-altitude (h) relationship
determined from the 1981 data. The
PB values are well predicted
from the equation PB = exp
(6.63268
0.1112 h
0.00149 h2), where h is in kilometers.
The conclusion is that on days when the mountain is usually climbed,
during May and October, the summit pressure is 251-253 Torr.
extreme altitude; maximal oxygen uptake; acclimatization; work capacity; extreme hypoxia
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INTRODUCTION |
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BAROMETRIC PRESSURES near the summit of Mt. Everest (altitude 8,848 m) are of great interest to high-altitude physiologists because the pressure is so low that the PO2 is very near the limit for human survival. Until recently, only one direct measurement of barometric pressure had been made on the Everest summit. This was done by Dr. Christopher Pizzo on October 24, 1981 during the American Medical Research Expedition to Everest (AMREE), and the value he obtained was 253 Torr (8). The measurement was made with a crystal sensor that was calibrated in the field against a mercury barometer.
Despite being only one data point, the value of 253 Torr has been extensively used in high-altitude physiology. For example, it was the pressure selected for the "summit" in the long-term low-pressure chamber study Operation Everest II (1). In addition, the summit measurement and additional measurements just above the South Col at an altitude of 8,050 m were used to define the relationship between barometric pressure and altitude on high mountains at latitudes near the equator with good predictive power (5). Mt. Everest is especially suitable for determining the pressure-altitude relationship because not only is its summit at 8,848 m the highest point on Earth but also the South Col (altitude 7,986 m) is a well-defined saddle, and therefore its altitude has been accurately determined.
Clearly, it would be desirable to have additional data on barometric pressures at extreme altitudes on Mt. Everest, and in the last 3 yr two new studies have been carried out. The present paper describes the results, compares the new information with that already available, and discusses the physiological implications.
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1997 NOVA EVEREST EXPEDITION |
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In the spring of 1997, the television science program NOVA organized an expedition to Mt. Everest, and five people reached the summit. The scientific program included measurements of neuropsychological function at extreme altitude, and these were compared with the results from brain imaging before and after the expedition. Cardiopulmonary studies were also made.
We were not aware of the expedition until the last minute but were able to send a handheld barometer in the hope that it would be possible to obtain a measurement on the summit. The instrument was a Pretel Alti Plus K2 barometer (Groupe Pretel, Claix, France). Although we had used the barometer extensively at altitudes up to ~5,000 m at normal ambient temperatures, there was not time before the expedition to calibrate it for the very low pressure expected on the summit and for the very low temperature.
A single measurement was made by David Breashears at 7:00 AM
Nepalese time on May 23, 1997. The value was 346 mbar, which corresponds to 259.5 Torr. The barometer was carried in his backpack and so was exposed to the ambient temperature. This was not measured directly, but according to weather balloon soundings made at the same
time (see WEATHER BALLOON SOUNDINGS)
the temperature was approximately
22°C.
When the barometer was returned to University of California San Diego,
it was directly calibrated against a mercury column at barometer
temperatures of 21,
6, and
20°C. The graph of
barometer reading against mercury height showed excellent linearity.
However, the barometer read 1-2 Torr low at 760 Torr and 5.3 Torr
high at barometric pressures between 232 and 283 Torr at a temperature of 21°C. When the measurements were made after the barometer had been left overnight in a
20°C cold room, the error increased to 7 Torr in the pressure range of 232-283 Torr. Therefore, the corrected pressure was 259.5 Torr minus 7 Torr, that is, 252.5 Torr.
This is in close agreement with the value of 253 Torr obtained by Pizzo
on October 24, 1981.
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WEATHER BALLOON SOUNDINGS |
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Additional information on barometric pressures at an altitude of 8,848 m in the vicinity of Mt. Everest at the time of the direct measurement was obtained from weather balloon soundings. These radiosondes are released from many locations all over the world at 0000 and 1200 UTC (Universal coordinated time) every day. We used data from radiosondes released from the 14 stations closest to Mt. Everest at 0000 UTC on May 23, 1997. This corresponds to 5:40 AM local time and so is close to the time when the direct measurement was made. The latitude and longitude of the Everest summit are 27°59'N and 86°56'E, and the weather stations were all between 22 and 38°N and between 74 and 95°E. The data for each radiosonde were retrieved by Laurence G. Riddle of the Scripps Institution of Oceanography, University of California San Diego.
Altitudes for barometric pressures of 150, 200, 250, 300, 400, 500, and
700 mbar were obtained for each radiosonde (from knowledge of its
ascent rate) and plotted as log barometric pressure vs. altitude.
Figure 1 shows an example for the station
at Gorakhpur, which is near Everest at 26.75°N, 83.37°E (Fig.
2). The data points lay almost
on a straight line but an even better fit was obtained by using a
parabola, and the pressure for altitude 8,848 m was then obtained by
interpolation. For Gorakhpur, this was 338.2 mbar. These pressures in
millibars were converted to Torr by multiplying by 0.7500, and the
results are shown in Fig. 2. Other data are also available from the
radiosondes, including temperature, humidity, wind direction, and wind
velocity. The temperature data showed that, at an altitude of 8,848 m,
the temperature was about
22°C, and therefore this was used
to calibrate the barometer as indicated under 1997
NOVA EVEREST EXPEDITION.
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Figure 2 shows that the barometric pressure at an altitude of 8,848 m above Gorakhpur just to the south and west of Everest was 254 Torr, whereas above Gauhati just to the south and east of Everest the pressure was 253 Torr. There is another close station at Patna at 25.60°N, 85.10°E, but unfortunately this radiosonde failed and no data were reported above 5,850 m. The agreement between the radiosonde pressures and the direct measurement is close.
An interesting feature of the radiosonde data is that a high-pressure
system was located near the summit of Mt. Everest at the time of the
direct measurement. This is apparent from Fig. 2 but is more easily
seen in plots of the altitude for a barometric pressure of 300 mbar
(225 Torr), which are available from the radiosonde data. Figure
3 shows that, at the coordinates of the Everest summit, the altitude of the 300-mbar pressure was 9,715 m,
which corresponds to almost the highest altitude on the chart.
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BAROMETRIC PRESSURES ON THE SOUTH COL OF EVEREST (ALTITUDE 7,986 M) OBTAINED IN THE SUMMER OF 1998 |
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An Everest study organized by the Media Laboratory of the Massachusetts
Institute of Technology placed a weather station on the South Col
(altitude 7,986 m) (3) in early May 1998. Barometric pressure was
measured with a Motorola sensor (MPX 5100AP, Motorola, Schaumburg, IL),
which has a pressure range of 0-760 Torr and can operate at
temperatures down to
40°C. The data were transmitted up to
one of three polar orbiting National Oceanic and Atmospheric Administration satellites and then to a ground station. These data were
posted on the Web site http://janson.media.mit.edu/weather/14836, and
up to 30 measurements of pressure and time of day were available every
day from May 4 to August 26. The probe also transmitted temperature,
wind speed, and degree of lightness or darkness.
In general, the data were internally very consistent with small daily and monthly SDs. However, there were 23 rogue measurements that were clearly outliers. For example, on May 7 all but one of the measurements were between 10.7 and 11.27 in. Hg, whereas one at 0246 UTC was 3.11 in. Hg. Again on July 1, all the measurements were between 10.93 and 11.27 in. Hg except for one of 25.88 in. Hg, which was clearly an outlier. In addition, the measurements at the start of the data transmission on May 4 and early on May 5 were erroneously high because the barometer was still being carried up at this time. If these outliers are rejected, the total number of measurements between May 6 and August 26 was 2,572.
The mean and SD pressures for May, June, July, and August, respectively, were as follows: 11.17 ± 0.10, 11.24 ± 0.05, 11.27 ± 0.04, and 11.30 ± 0.03 in. Hg. Note that the monthly SDs were <0.5% of the means. When these these pressures were converted to Torr, the monthly means for May, June, July, and August were 283.7, 285.5, 286.3, and 286.9 Torr. The gradual increase in barometric pressure from May to July is to be expected because of the well-known seasonal variation (e.g., see Fig. 3 in Ref. 8).
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COMPARISON WITH PREVIOUS DATA AND PHYSIOLOGICAL SIGNIFICANCE |
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Direct measurement on the Everest summit by the 1997 NOVA Everest Expedition. The agreement within ~1 Torr of this measurement with that made by Pizzo in October 1981 is gratifying. There is a substantial seasonal variation in barometric pressure at an altitude of 8,848 m (as shown in Fig. 3 of Ref. 8). The highest pressures are seen in July and August and the lowest pressures in January. May and October are at approximately the same height on the descending limbs of the plot of pressure against month. Therefore, we can expect the pressures in these 2 mo to be similar.
The fact that the pressure was as high as 253 Torr does not mean that this is the mean pressure at the summit during May or October. Climbers tend to choose high pressure days for their summit bid, and, for example, October 24, 1981 was unusually warm with the temperature directly measured on the summit being
9°C (8). In the case
of Breashears' measurement on May 23, 1997, Fig. 3 shows that Everest
was near the center of a high-pressure system. Radiosonde measurements
made from New Delhi show that the mean monthly barometric pressure for
an altitude of 8,848 m at latitude 28°N is ~251 Torr for both May
and October (8). In July and August the mean monthly pressure is
between 254 and 255 Torr, whereas in January it falls to as low as 243 Torr.
Radiosonde measurements for 0000 UTC on May 23, 1997. Again, the agreement between the radiosonde data and the direct measurement is close. The isobars for the pressure of 300 mbar (Fig. 3) show that a high-pressure zone extended from the weather stations at Gorakhpur and Gauhati to include Everest. The same pattern is seen in the altitudes for the 500-mbar pressure, which is not reproduced here. Therefore, we can conclude that the radiosonde value at the Everest summit was close to 253 Torr.
Barometric pressures on the Everest South Col, May to August 1998. The South Col of Mt. Everest is ~860 m below the summit, and it might therefore be argued that barometric pressure data from that location are not valuable in determining the summit pressure. However, the altitude of the South Col is accurately known, and therefore the barometric pressure data can be used to locate the line relating pressure to altitude.
The weather probe measurements can be compared with those made at Camp 5 during the AMREE in 1981. The altitude of this camp was ~60 m above the South Col at 8,050 m, and six barometric pressure measurements were made between October 12 and October 25, the range of values being 281.5 to 285.1 Torr. The mean and SD was 283.6 ± 1.5 Torr (8). The mean pressure recorded from the Massachusetts Institute of Technology (MIT) weather probe for May 1998 (when the seasonal variation is comparable with October) was 283.7 Torr so agreement between the two studies was close. At this altitude, an increase in altitude of 60 m corresponds to a fall in pressure of ~2 Torr.Relationship between barometric pressure and altitude on Mt.
Everest.
Table 1 summarizes the barometric pressure
data available from the 1997 NOVA Everest Expedition, the 1998 Everest
study organized by MIT, and the 1981 AMREE. After the 1981 expedition,
a line relating barometric pressure to altitude was derived on the
basis of the measurements made at 8,848, 8,050, and 5,400 m as shown in
Table 1 (Fig. 2 of Ref. 8). The line used the logarithm of barometric
pressure because the data then almost fall on a straight line.
Subsequently, the Model Atmosphere equation was derived that fitted
these data together with barometric pressures measured at many
high-altitude stations, the altitudes of which are accurately known
(5). Many of these measurements were from locations within 30° of
the equator, and most were in the summer. These locations and time of
year were chosen because the barometric pressures are lower at higher
latitudes and in the winter months. The Model Atmosphere
equation is PB = exp (6.63268
0.1112 h
0.00149 h2) where
PB is barometric pressure in
Torr and h is altitude in kilometers. It was shown that
barometric pressures of most locations were predicted within 1%.
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Physiological significance of the new data.
The new data greatly increase our confidence in the barometric
pressure-altitude relationship at altitudes of 8,000 m and above on Mt.
Everest where there was previously so little data. The new measurements
confirm that the inspired PO2 is only
42-43 Torr on the summit and justify the use of this value in
determining the maximal oxygen consumption
(
O2 max) on the summit
(4, 7). The measurements further emphasize the extreme sensitivity of
O2 max to barometric
pressure at these great altitudes.
O2 max declined from
1,450 to 1,070 ml/min (see Table 6 in Ref. 7). This means that the
slope of the line relating
O2 max to inspired
PO2 was ~63
ml · min
1 · Torr
1.
A very similar result was found in Operation Everest II (4; see Fig.
11.17 in Ref. 6).
The extreme steepness of the line relating
O2 max to inspired
PO2 has some interesting
physiological implications. For example, if the barometric pressure on
the summit were 236 Torr, as predicted from the International Civil
Aviation Organization Standard Atmosphere (2), the inspired
PO2 on the summit would be only 39.5 Torr. Therefore, the reduction in inspired PO2 from the value of 43 Torr, which
would exist for a summit pressure of 253 Torr, would be 3.5 Torr. The
reduction of oxygen consumption would therefore be ~222 to a value of
~848 ml/min, or a reduction of ~21%. It seems very unlikely that
the mountain could be climbed under these conditions.
In fact, even the reduction of barometric pressure of only 10 Torr,
such as occurs between summer and winter on the Everest summit, is
predicted to reduce
O2 max by
~133 ml/min. In other words,
O2 max on the summit
would fall from 1,070 to ~940 ml/min, that is, by ~12%. This is
presumably one reason why the mountain has not yet been climbed in
midwinter without supplementary oxygen.
In summary, the new direct measurement of barometric pressure made in
May 1997 and the very extensive series of measurements of barometric
pressure on the South Col in 1998 greatly increase our confidence in
the barometric pressure-altitude relationship at altitudes of 8,000 m
and above on Mt. Everest. They provide additional evidence that humans
at these altitudes are very close to the limit of tolerance to hypoxia.
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ACKNOWLEDGEMENTS |
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I am indebted to Liesl Clark and David Breashears of the 1997 NOVA Everest expedition, Michael Hawley and others at the Massachusetts Institute of Technology for help with the data from the 1998 study, and Laurence G. Riddle of the Scripps Institution of Oceanography, University of California San Diego for help with the radiosonde data.
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FOOTNOTES |
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The costs of publication of this article were defrayed in part by the payment of page charges. The article must therefore be hereby marked "advertisement" in accordance with 18 U.S.C. §1734 solely to indicate this fact.
Address for reprint requests: J. B. West, UCSD Dept. of Medicine 0623A, 9500 Gilman Dr., La Jolla, CA 92093-0623 (E-mail: jwest{at}ucsd.edu).
Received 5 October 1998; accepted in final form 27 October 1998.
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