Meteorology: Difference between revisions

Content deleted Content added
No edit summary
Line 20: Line 20:


=== Discovery of Stratosphere ===
=== Discovery of Stratosphere ===
Teisserenc de Bort designed and built meterological recording instruments and sent them aloft on balloons and kites of his own design and modification.
Teisserenc de Bort designed and built meteorological recording instruments and sent them aloft on balloons and kites of his own design and modification.


On 9 September 1899, he had come briefly into the public eye when one of his kite flights -- a large kite carrying a meteorograph and ten other "helping-kites" supporting the tethering cable --- broke free and, traling 7 kilometers of cable, cut a narrow but astonishing swath through PAris, where it stopped traffic, disabled a train, and cut off all telegraphic communication with Rennes on the day when all France and most of the rest of the world were anxiously awaiting the result of the famous Dreyfus court-martial at that city.
On 9 September 1899, he had come briefly into the public eye when one of his kite flights -- a large kite carrying a meteorograph and ten other "helping-kites" supporting the tethering cable --- broke free and, trailing 7 kilometers of cable, cut a narrow but astonishing swath through Paris, where it stopped traffic, disabled a train, and cut off all telegraphic communication with Rennes on the day when all France and most of the rest of the world were anxiously awaiting the result of the famous Dreyfus court-martial at that city.


Under the circumstances, de Bort suspended kite flying for a while and return to a series of upper-air experiments with free balloons. He preferred working with those made of kerosened paper. These were filled with hydrogen and trailed a very short cable holding the meteorograph and a bag of sand ballast, which dribbled out at a steady rate to control the balloon's rate of ascent. de Bort's aim was to get these all up as high as possible, often over 11 kilometers and occassionally as high as 14 kilometers. When the balloon reached its maximum altitude, the instrument pack was parachuted back to earth.
Under the circumstances, de Bort suspended kite flying for a while and return to a series of upper-air experiments with free balloons. He preferred working with those made of kerosened paper. These were filled with hydrogen and trailed a very short cable holding the meteorograph and a bag of sand ballast, which dribbled out at a steady rate to control the balloon's rate of ascent. de Bort's aim was to get these all up as high as possible, often over 11 kilometers and occasionally as high as 14 kilometers. When the balloon reached its maximum altitude, the instrument pack was parachuted back to earth.


When de Bort looked at the temperature records on flights that reached altitudes of 10 kilometers or greater, he noted that the recorded air temperatures failed to decrease with altitude, though theory predicted that they should. The measurement performed by James Glaisher in the 1860s and corrected by Aßmann some years later showed that the temperature should decrease by about 6 C with each kilometer of ascent. In de Bort's records, however, the temperature showed no such decrease between 10 and 14 kilometers.
When de Bort looked at the temperature records on flights that reached altitudes of 10 kilometers or greater, he noted that the recorded air temperatures failed to decrease with altitude, though theory predicted that they should. The measurement performed by James Glaisher in the 1860s and corrected by Aßmann some years later showed that the temperature should decrease by about 6 C with each kilometer of ascent. In de Bort's records, however, the temperature showed no such decrease between 10 and 14 kilometers.


Aßmann had measured this effect several times between 1894 and 1897 in manned balloon ascents, but he was reasonably sure that it was due to the warming of instrument packet by solar radiaton. He was delighted to treat the phenomenon as another problem in instrument design. Hergesell agreed that the phenomenon was probably due to instrument warming, and so did de Bort. All of them tried various ways to shield their thermometers from reflecting or absorbing surfaces on the instrument packets that contained them, in order to keep the thermometers from false readings.
Aßmann had measured this effect several times between 1894 and 1897 in manned balloon ascents, but he was reasonably sure that it was due to the warming of instrument packet by solar radiation. He was delighted to treat the phenomenon as another problem in instrument design. Hergesell agreed that the phenomenon was probably due to instrument warming, and so did de Bort. All of them tried various ways to shield their thermometers from reflecting or absorbing surfaces on the instrument packets that contained them, in order to keep the thermometers from false readings.


De Bort took the investigation further. He solved all the instrumental problems he could think of. Aware of the possibility of a radiation effect,he began to fly balloons at night. When these night flight also showed a steady temperature around 11 kilometers, he began a systematic program to see whether there was a seasonal variation. The radiation effect should be smaller in the winter than the summer.
De Bort took the investigation further. He solved all the instrumental problems he could think of. Aware of the possibility of a radiation effect, he began to fly balloons at night. When these night flight also showed a steady temperature around 11 kilometers, he began a systematic program to see whether there was a seasonal variation. The radiation effect should be smaller in the winter than the summer.


The problem was difficult because the effect was elusive. The zone of steady temperature moved up and down between 8 - 12 kilometers, though it was most often at 11 kilometers. It was stronger and weaker over a range of many degrees. By 1900, he had the record of 146 ascents to report to the Academia des Sciences in Paris, but he still postponed conclusions concerning his measurements of temperatures at altitudes above 10 kilometers, unsure as to the character of what he was seeing.
The problem was difficult because the effect was elusive. The zone of steady temperature moved up and down between 8 - 12 kilometers, though it was most often at 11 kilometers. It was stronger and weaker over a range of many degrees. By 1900, he had the record of 146 ascents to report to the Academia des Sciences in Paris, but he still postponed conclusions concerning his measurements of temperatures at altitudes above 10 kilometers, unsure as to the character of what he was seeing.


He worked for two more years on the problem, and in 1902, with an accumulation of 236 ascents to support his argument, he made the plunge and publicly rejected the prevailing theory of temperature decrease with altitude. He asserted the existence of an isothermal zone with varying thickness, in which the adiabatic lapse rate (of temperature with altitude) diminished to zero, usually at an altitude of 11 kilometers after which the temperature would remain constant for several kilometers. The layer was higher over high-pressure centers (anticyclones) and lower over low-pressure centers (cyclones). He suggested the problem of the general circulation of the atmosphere would have to be reconsidered, sich such an isothermal layer meant the atmosphere as a whole was not in convective equilibrium, but only that part bounded above by this "isothermal zone".
He worked for two more years on the problem, and in 1902, with an accumulation of 236 ascents to support his argument, he made the plunge and publicly rejected the prevailing theory of temperature decrease with altitude. He asserted the existence of an isothermal zone with varying thickness, in which the adiabatic lapse rate (of temperature with altitude) diminished to zero, usually at an altitude of 11 kilometers after which the temperature would remain constant for several kilometers. The layer was higher over high-pressure centers (anticyclones) and lower over low-pressure centers (cyclones). He suggested the problem of the general circulation of the atmosphere would have to be reconsidered, such such an isothermal layer meant the atmosphere as a whole was not in convective equilibrium, but only that part bounded above by this "isothermal zone".



Aßmann realized immediately what he had missed and rushed to claim a share of it for himself, based on the analysis of six balloon ascents at Berlin in 1901. He endorsed de Bort's results, but modified them by asserting that his own superior rubber-balloon technology, with a controlled rate of ascent and more sensitive recorders could prove that this was not simply an isothermal zone, but a true "inversion zone". The temperature not only stopped decreasing in this region, but actually increased for several kilometers before decreasing again. Moreover, he thought he could detect an upper boundary to the region of temperature shift in a layer at about 15 kilometers, meaning that there was both a "lower inversion" and an "upper inversion".
Aßmann realized immediately what he had missed and rushed to claim a share of it for himself, based on the analysis of six balloon ascents at Berlin in 1901. He endorsed de Bort's results, but modified them by asserting that his own superior rubber-balloon technology, with a controlled rate of ascent and more sensitive recorders could prove that this was not simply an isothermal zone, but a true "inversion zone". The temperature not only stopped decreasing in this region, but actually increased for several kilometers before decreasing again. Moreover, he thought he could detect an upper boundary to the region of temperature shift in a layer at about 15 kilometers, meaning that there was both a "lower inversion" and an "upper inversion".
Line 43: Line 42:
The atmosphere's weather zone had thus a ceiling as well as floor. Storm systems might now be seen as coherent masses of air, trapped between the boundaries of Earth's surface below and the tropopause above.
The atmosphere's weather zone had thus a ceiling as well as floor. Storm systems might now be seen as coherent masses of air, trapped between the boundaries of Earth's surface below and the tropopause above.


It meant that the atmosphere had to be "remapped" from pole to equator and through its full vertical height. No one knew how the tropopause changed with latitude, or how it differed over land and over the oceans, or even why it was there. Was it a matter of temperature and pressure alone, or was it the result of a chemical differentiation of the atmospher with altitude?
It meant that the atmosphere had to be "remapped" from pole to equator and through its full vertical height. No one knew how the tropopause changed with latitude, or how it differed over land and over the oceans, or even why it was there. Was it a matter of temperature and pressure alone, or was it the result of a chemical differentiation of the atmosphere with altitude?