Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-23T11:25:03.708Z Has data issue: false hasContentIssue false

Ice Budgets for Antarctica and Changes in Sea-Level

Published online by Cambridge University Press:  30 January 2017

H. Wexler*
Affiliation:
U.S. Weather Bureau, Washington, D.C.
Rights & Permissions [Opens in a new window]

Abstract

Eight different ice budgets for the Antarctic Ice Sheet are examined. Five of these budgets call for rates of increase of the ice which are in surprisingly good agreement considering the wide dispersion of individual components of the budgets. The observed rise in sea-level of the world’s oceans would appear to contradict the removal of water required to nourish the Antarctic Ice Sheet at the claimed rates. The thermal expansion of oceanic columns, caused by “climatic” warming of the oceans, has been invoked to resolve this contradiction but it appears that this is not large enough judging from the 30 yr. difference in water temperatures measured by the Meteor and the Crawford in two profiles across the tropical Atlantic Ocean.

Résumé

Résumé

Huit bilans de masse de l’Indlandsis Antarctique proposés par différents auteurs sont confrontés dans le présent article. Cinq de ces bilans de masse indiquent des valeurs d’accroissement de la glace qui sont en accord d’une façon assez surprenante si l’on considère la grande disparité des composantes individuelles des bilans de masse. L’élévation obtenue du niveau moyen des mers du globe semble être en contradiction avec le transfert d’eau nécessaire à l’alimentation de l’Indlandsis Antarctique dans les proportions indiquées. L’expansion thermique de masses océaniques, causée par le réchauffement climatique des océans a été invoquée pour expliquer cette contradiction; mais il semble que cette cause soit insuffisante, à en juger par les différences de température des eaux marines mesurées à 30 ans d’intervalle par le “Meteor” et le “Crawford” le long de deux profils à travers la zone tropicale de l’Océan Atlantique.

Zusammenfassung

Zusammenfassung

Es werden 8 verschiedene Haushaltsberechnungen des antarktischen Inlandeises überprüft. 5 davon führen zu einer Zunahme des Eises, deren Zahlenwerte erstaunlich gut übereinstimmen, wenn man sich die grosse Streuung der Einzelkomponenten der Haushaltsberechnungen vor Augen hält. Die beobachtete Hebung des Wasserspiegels der Weltmeere scheint einer Entnahme von Wasser zur Ernährung des antarktischen Inlandeises in dem geforderten Mass zu widersprechen. Zur Erklärung dieses Widerspruchs wurde die Wärmeausdehnung ozeanischer Wassersäulen herangezogen, die durch eine „klimatische“ Erwärmung der Ozeane verursacht wird. Doch scheint diese nicht gross genug, wenn man von den Änderungen der Wassertemperatur in 30 Jahren ausgeht, wie sie von den Forschungsschiffen Meteor und Crawford in zwei Profilen über den tropischen Atlantik gemessen wurden.

Type
Research Article
Copyright
Copyright © International Glaciological Society 1961

The intensive investigation of Antarctica carried on during the International Geophysical Year of 1957–58, particularly in meteorology and glaciology, has had as one of its major goals the determination of the mass of ice and whether it is increasing or decreasing.

Based on earlier estimates by Sharp Reference Sharp and Crary 1 and Gould Reference Gould 2 plus a few scattered observations of ice thickness made before the I.G.Y., an average thickness of 2,000 m. was assumed over the 13.5 × 106 km.2 area, which for an average density of 0.9 g. cm.−3 amounted to 2.43 × 1022 g. 3 Later estimates by Crary Reference Crary 4 (1,950 m.) and Bauer Reference Crary 4 (2,130 m.) based on I.G.Y. data agreed fairly well with the earlier estimate; but there is not nearly so close agreement in the several ice budgets proposed by various investigators, or as to whether or not the ice is growing.

Eight different ice budgets are presented in Table I. The first budget shown, I, is that proposed by Kosack in 1956;Reference Kosack 5 it is based on an average liquid precipitation of 20.1 cm. yr.−1 or 2.85 × 1018g. yr.−1 over all of Antarctica. Losses are incurred by blowing snow (1.20 × 1018 g. yr.−1), by calving of icebergs (0.55 × 1018 g. yr.−1), and by ablation (surface melting, run-off and evaporation, 2.05 × 1018 g. yr.−1). No significant contribution is attributed to melting of ice shelves from below. These figures yield a net loss of 0.95 × 1018 g. yr.−1, which, if released to the ocean with no other compensatory changes, would increase world sea-level by 2.6 mm. yr.−1 since the area of all oceans including marginal seas is 360.8 × 106 km.2.

Table I. Various Ice Budgets for Antarctica* (Unit 1018 g. yr.−1)

The second budget, II (Table I), is based on an assumption of steady-state equilibrium, where the average liquid precipitation over Antarctica was taken as 12.0 cm. yr−1, Reference Wexler 3 the larger of Loewe’s two values.Reference Loewe 6 The net water vapor transport southward across lat. 70° S., 1.62 × 1018 g. yr.−1, fell as snow and was taken equal to the northern transport of snow and ice across lat. 70° S. by blowing snow, calving of icebergs and melting at the bottom of the large ice shelves characteristic of Antarctica.

In the third budget, III, the water vapor transport is decreased to agree with a lower estimate of 7.0 cm. yr.−1 of average liquid precipitation over Antarctica made by Rubin,Reference Rubin 7 which agrees with an earlier estimate of Meinardus.Reference Meinardus, Köppen and Geiger 8 The transport of water vapor southward across lat. 70° S. is thus decreased to 0.945 × 1018 g. yr.−1. The northward transport figures are also adjusted: the blowing snow transport figure, admittedly too large in budget II, is decreased to one-fourth of its value, following Vickers.Reference Vickers 9 The calving rate, also admittedly too low in budget II, is increased by applying an average northward motion of 300 m. yr.−1 of a 200 m. average thick ice shelf, values slightly less than those observed at Little America V.Reference Wexler 10 To achieve mass balance only 17 per cent of Sverdrup’s ocean energy transport into the Maudheim Is-ShelfReference Sverdrup 11 is found necessary, instead of the 100 per cent needed in budget II.

Another ice budget proposed by Lister Reference Lister 12 is presented in Column IV. The average liquid precipitation of 14.2 cm. yr.−1 was computed by the present writer from Lister’s average annual accumulation of 13.1 g. cm.−2 plus his estimated evaporation and run-off values of 1.0 and 0.1 g. cm.−2, respectively. The sizeable loss attributed to net evaporation has been questioned.Reference Wexler 13, Reference Loewe 14 Lister’s budget indicates a net transport of 0.83 × 1018 g. yr.−1 into Antarctica, or an increase of 0.341 per cent of the present ice mass each century. This increase, if maintained, would double the present ice mass in 29,300 yr. and would cause a lowering of the world sea-level by 2.3 mm. yr.−1.

In Column V (Table I) is shown an ice budget proposed by Mellor.Reference Mellor 15 The average precipitation and evaporation figures are nearly the same as Lister’s but the blowing snow value is much larger and the melting rate much smaller. The net inward transport is larger, 1.05 × 1018 g. yr.−1, and would lower sea-level by 2.9 mm. yr.−1.

Two ice budgets based on minimum and maximum values, proposed by Loewe,Reference Loewe 6 are shown in Column VI. Loewe took average liquid accumulations of 10.0 and 12.0 cm. yr.−1, which, when added to minimum and maximum blowing snow values, gave average liquid precipitation values of 10.2 and 16.0 cm. yr.−1, respectively. Melting from the surface or from the bottoms of ice shelves contributed very little, if at all, to the loss of ice while net evaporation was considered to be zero. The net inflows of 1.11 × 1018 and 1.20 × 1018 g. yr.−1, respectively, would lower sea-level by 3.1 and 3.3 mm. yr.−1, respectively.

Finally, in Column VII there is shown a budget proposed by Kotliakov,Reference Kotliakov 17 based on an average liquid precipitation of 19 cm. yr.−1. A loss of 1.21×1018 g. yr.−1 by calving is the largest of all estimates shown in Table I. No shelf melting figure is included. The net gain of 1.33×1018 g. yr.−1 would result in a lowering of sea-level by 3.7 mm. yr.−1.

Thus it is seen from Table I, that budgets IV to VII (Lister, Mellor, Loewe, and Kotliakov) all agree that the Antarctic Ice Sheet is growing at rates which are in remarkably close agreement, considering the wide divergence of the figures from which they were derived. The average increase is 1.10 × 1018 g. yr.−1.

The first budget indicates a loss of Antarctic ice. The next two budgets, II and III, are based on approximate mass balance for which Robin Reference Robin 18 gives the following supporting arguments:

  • i. Domed shapes of the ice sheet.

  • ii. Scarcity of freshly exposed rock surfaces (which would be evidence against recent, i.e. within past few centuries, lowering of the ice).

  • iii. Small values of world-wide changes in mean sea-level.

With respect to Robin’s third point, the net accretions to the Antarctic Ice Sheet shown in budgets IV–VII would call for reduction of the mass of the oceans such that sea-level would lower by 2.3 to 3.7 mm. yr.−1, if the following conditions were fulfilled:

  • i. No isostatic upward movements of the coasts.

  • ii. No tectonically caused upward movements of coasts.

  • iii. No compensatory warming and expansion of the world’s oceans.

Both isostatic and tectonic movements are known on several coasts and attempts have been made to eliminate these effects from long-term measurements of sea-level to obtain the eustatic changes of sea-level, that is, variations in sea-level caused by changes in the water cycle between ocean and land, assuming that the total mass of water substance in the oceanatmosphere–surface land layer remains constant.

Hela Reference Hela 19 has summarized eustatic sea-level changes determined by various investigators and the results are shown in Table II.

Table II. Eustatic Rises of Sea-Level (First Five Values from Hela;Reference Hela 19 Dates Added by Present Writer)

Apart from Thorarinsson’s value and Kuenen’s first value there is surprisingly good agreement among the other four investigators of an eustatic rise of sea-level of about 1.18 mm. yr.−1. Thorarinsson’s value of 0.5 mm. yr.−1 was computed by applying estimates of average losses of some five glaciers studied in Iceland, Spitsbergen, Sweden, and Switzerland to all other glaciers of the world with the exception of the whole of Antarctica and the accumulation area of the Greenland Ice Sheet. In the following discussion we shall disregard the possible effect of changes in the Greenland accumulation area so that we can apply Thorarinsson’s results directly to the problem of changes in the Antarctic Ice Sheet.

Despite this good agreement Hela states “… the present rate of eustatic rise of sea-level remains uncertain”. As an alternative to an increase of mass of ocean water and a resulting rise of sea-level caused by melting of glaciers, he cites the possibility of an increase of volume (with mass constant) because of heating and thermal expansion of the oceans. According to Munk and Revelle Reference Munk and Revelle 25 a heating by 1° C. of the entire ocean would raise the surface by 600 mm. Thus, the observed rise of 1.18 mm. yr.−1 might be explained by a warming of the total ocean by 0.002° C. yr.−1.

In absence of oceanic heating, if the Antarctic Ice Sheet is growing at a rate which removes water from the oceans so that sea-level would drop at the rate of 3.06 mm. yr.−1 (the average of the values given in Columns IV–VII in Table I), then the compensatory melting of ice elsewhere in the world must amount to an increase of sea-level by 4.24 mm. yr.−1 to give the observed eustatic sea-level rise of 1.18 mm. yr.−1. If the 4.24 mm. yr.−1 rise in sea-level is not eustatically caused but is of thermal origin, this would mean a warming of the entire ocean by 0.007° C. yr.−1.

It is difficult to prove whether an oceanic warming of this rate has occurred. It is equivalent to the added absorption by the oceans of 1 per cent of the total earth’s receipt of solar radiation.Reference Wexler 26 Hoinkes Reference Hoinkes 27 cites the warming of surface water in the North Atlantic, summarized by Bjerknes,Reference Bjerknes 28 of 0.3° C. in the 36 yr. from 1890–97 to 1926–33, or 0.008° C. yr.−1, as supporting evidence for the thermal explanation of the rise of sea-level. Thus Hoinkes concludes, as do Loewe and Mellor, that the growth of the Antarctic Ice Sheet does not necessarily contradict the observed rise in sea-level.

However, a word of caution is necessary; Bjerknes’s warming figure cited above is only for surface waters of the North Atlantic. What about the deep waters? Data on long-term climatic changes of deep ocean temperatures are scarce but Fuglister,Reference Fuglister 29 in comparing temperatures in the Meteor profiles VI (lat. 16° S.) and VIII (lat. 8° S.) with observations taken 30 yr. later by the Crawford, concludes “… the deep water is a little cooler, perhaps a little more saline and has lost some oxygen. The bottom Antarctic water is warmer and more saline.” Scaling off from Fuglister’s profiles the average temperature differences over the 5,000 m. deep ocean gives the results in Table III. These values are probably too large since they include relatively large seasonal effects in the top few hundred meters. The average annual temperature increase of 0.0009° C. from Table III, if representative of all oceans, is too small by a factor of 7 to account for the thermal vertical expansion of the oceans by 4.24 mm. yr.−1 needed to agree with the observed rise of 1.18 mm. yr.−1 and the estimated depletion of the world’s oceans by 3.06 mm. yr.−1 to support the estimated growth of the Antarctic Ice Sheet.

Table III. Average Temperature Rises (°C.) Between Meteor and Crawford Stations (1927–1957)

If we accept an average warming of the oceans by 0.001° C. yr.−1 and a release of water from melting glaciers outside of Antarctica amounting to a sea-level rise of 0.5 mm. yr.−1 (Thorarinsson’s minimum value), then we can compute the change of sea-level caused by changes in the Antarctic Ice Sheet as shown in Table IV.

Table IV. Eustatic and Thermal Changes of Sea-Level

Expressed in terms of the mass of ice removed from Antarctica each year, this eustatic increase of sea-level by 0.08 mm. yr.−1 amounts to an ice loss of 0.029 × 1018 g. yr.−1. If a value of 12 mm. yr.−1, or more than twice Thorarinsson’s minimum value for water released by non-Antarctic glaciers is used, then the rate of growth of the Antarctic Ice Sheet is equivalent to −0.62 mm. yr.−1 change in sea-level or an increase of ice by 0.224 × 1018 g. yr.−1, about one-fifth of the average of the net transport values shown in Columns IV–VII of Table I. A decrease of about 10 per cent in the estimated average precipitation values in these columns would wipe out this increase.

If there were no oceanic warming, then from Table IV the change in the Antarctic Ice Sheet would be between −0.246 × 1018 and +0.007 × 1018 g. yr.−1 depending on whether Thorarinsson’s minimum value or 2.4 times that value were used.

Another possibility to be considered in studying changes in sea-level is that the storage of water vapor in the atmosphere may change. On the average there are about 30 mm. of precipitable water vapor in an atmospheric column of 1 cm.2 cross-section area. Because of climatic warming the atmospheric capacity for water vapor may increase. Willett Reference Willett 30 estimates that the average world temperature from 1850 to 1940 has increased by 0.8° C. If this temperature increase is translated into saturation vapor pressure increase, maintaining the same value of average relative humidity, then the resulting increase in precipitable water vapor would be 1.6 mm. in 90 yr. or 0.0018 mm. yr.−1, much too small compared with the other terms listed in Table IV.

Kuenen Reference Kuenen 22 has examined the possibility of the surface water supply being increased by juvenile water from the earth’s interior but concludes it is less than 0.0002 × 1018 g. yr.−1.

In view of the uncertainties of the various components of water exchange between ocean, atmosphere and land, and the lack of adequate data on long-period thermal changes at all depths of the world’s oceans, it seems risky at this time to state that the Antarctic Ice Sheet is either increasing or decreasing.

Acknowledgement

It is a pleasure to acknowledge the assistance and critical review provided by my colleagues, M. Rubin and F. Ostapoff.

References

1. Sharp, R. P. Objectives of Antarctic glaciological research. (In Crary, A. P., and others, ed. Antarctica in the International Geophysical year. Washington, D.C., American Geophysical Union, 1956, p. 2735. (Geophysical Monograph, No. 1.))Google Scholar
2. Gould, L. M. Antarctic prospect. Geographical Review, Vol. 47, No. 1, 1957, p. 128.CrossRefGoogle Scholar
3. Wexler, H. Some aspects of Antarctic geophysics. Tellus, Vol. 10, No. 1, 1958, p. 7682.CrossRefGoogle Scholar
4. Crary, A. P. Private communication, November 1960.Google Scholar
5. Kosack, H.-P. Zur Frage des Wasserhaushalts in der Antarktis. Polarforschung, Bd. 3, 24 Jahrg., Ht. 1/2, 1954 [pub. 1956], p. 28694.Google Scholar
6. Loewe, F. Etudes de glaciologie en Terre Adélie, 1951–52. Paris, Hermann, 1956. (Expéditions Polaires Françaises. Résultats scientifiques, No. 9.)Google Scholar
7. Rubin, M. Private communication, November 1960.Google Scholar
8. Meinardus, W. Klimakunde der Antarktis. (In Köppen, W. Geiger, R., ed. Handbuch der Klimatologie. Bd. 4, Teil U. Berlin, Borntraeger, 1938.)Google Scholar
9. Vickers, W. W. Wind transport of Antarctic snow. Transactions. American Geophysical Union, Vol. 40, No. 2, 1959, p. 16267; I.G.ϒ. Bulletin (Washington, D.C.), No. 22, 1959, p. 4–9.Google Scholar
10. Wexler, H. Heating and melting of floating ice shelves. Journal of Glaciology, Vol. 3, No. 27, 1960, p. 62645.CrossRefGoogle Scholar
11. Sverdrup, H. U. The currents off the coast of Queen Maud Land. Norsk Geografisk Tidsskrift, Bd. 14, Nr. 1–4, 5953, p. 23949.CrossRefGoogle Scholar
12. Lister, H. Geophysical investigations of the Commonwealth Trans-Antarctic Expedition. Geographical Journal, Vol. 125, Pt. 3–4, 1959, p. 34351.CrossRefGoogle Scholar
13. Wexler, H. [Correspondence with M. Mellor on Antarctic geophysics.] Tellus, Vol. 10, No. 4, 1958, p. 49899.Google Scholar
14. Loewe, F. Notes concerning the mass budget of the Antarctic inland ice. (Summary.) Symposium on Antarctic meteorology. Melbourne, 1959.Google Scholar
15. Mellor, M. Mass balance studies in Antarctica. Journal of Glaciology, Vol. 3, No. 26, 1959, p. 52233.CrossRefGoogle Scholar
16. Loewe, F. Notes by M. Rubin of F. Loewe’s lecture cited above in ref. 14.Google Scholar
17. Kotliakov, V. M. The intensity of nourishment of the Antarctic ice sheet. [Paper presented at Symposium on Antarctica, twelfth General Assembly, International Union of Geodesy and Geophysics, Helsinki, July-August 1960 (table published in Hoinkes, H., Die Umschau, Bd. 60, Nr. 20, 1960, p. 62730).]Google Scholar
18. Robin, G. de Q. Geophysical studies in polar regions. The Antarctic ice sheet. Geophysical journal of the Royal Astronomical Society, Vol. 1, No. 3, 1958, p. 34751.CrossRefGoogle Scholar
19. Hela, I. Causes bringing about the difference between the geoid and the mean sea level surface. [Paper presented at twelfth General Assembly, I.U.G.G., Helsinki, July-August 1960.]Google Scholar
20. Gutenberg, B. Changes in sea level, postglacial uplift, and mobility of the earth’s interior. Bulletin of the Geological Society of America, Vol. 52, 1941, p. 72172.CrossRefGoogle Scholar
21. Thorarinsson, S. Present glacier shrinkage, and eustatic changes of sea-level. Geografiska Annaler, Arg. 22, Ht. 3–4, 1940, p. 13159.Google Scholar
22. Kuenen, Ph. H. Marine geology. New York, John Wiley and Sons, 1950.Google Scholar
23. Dietrich, G. Ozeanographisch-meteorologische Einflüsse auf Wasserstandsänderungen des Meeres am Beispiel der Pegelbeobachtungen von Esbjerg. Die Küste, Bd. 2, Ht. 2, 1954.Google Scholar
24. Hafemann, D. Anstieg des Meeresspiegels in geschichtlicher Zeit. Die Umschau, Bd. 60, Nr. 7, 1960, p. 19396.Google Scholar
25. Munk, W. Revelle, R. Sea level and the rotation of the earth. American journal of Science, Vol. 250, 1952, p. 82933.CrossRefGoogle Scholar
26. Wexler, H. Meteorology in the International Geophysical Year. Scientific Monthly, Vol. 84, No. 3, 1957, P. 14145. Google Scholar
27. Hoinkes, H. Neue Ergebnisse der glaziologischen Erforschung der Antarktis, III. Die Umschau, Bd. 60, Nr. 20, 1960, p. 62 730.Google Scholar
28. Bjerknes, J. The recent warming in the North Atlantic. (In Rossby memorial volume. The atmosphere and the sea in motion. New York, Rockefeller Institute Press, 1959, p. 65.)Google Scholar
29. Fuglister, F. C. Preliminary results of a re-survey of Meteor Profiles VI and VIII. [Paper presented at eleventh General Assembly, I.U.G.G., Toronto, 1957.]Google Scholar
30. Willett, H. C. Temperature trends of the past century. Centenary Proceedings of the Royal Meteorological Society, 1950, p. 195206.Google Scholar
31. Maksimov, I. V. Izmeneniye urovnya mirovogo okeana v svyazi s izmeneniyem moshchnosti materikovykh l’dov Antarktidy . Informatsionnyy Byulleten’ Sovetskoy Antarkticheskoy Ekspeditsii , No. 19, 1960, p. 57.Google Scholar
Figure 0

Table I. Various Ice Budgets for Antarctica*(Unit 1018 g. yr.−1)

Figure 1

Table II. Eustatic Rises of Sea-Level (First Five Values from Hela;19 Dates Added by Present Writer)

Figure 2

Table III. Average Temperature Rises (°C.) Between Meteor and Crawford Stations (1927–1957)

Figure 3

Table IV. Eustatic and Thermal Changes of Sea-Level