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BBAS3 21.30 ▼ 0.23% B3SA3 15.62 ▼ 0.70% WEGE3 47.96 ▲ 1.61% PRIO3 58.95 ▼ 3.12% SUZB3 43.18 ▼ 0.32% RENT3 37.86 ▲ 0.66% AZZA3 15.98 ▼ 2.68% CSAN3 4.07 — 0.00% RAIZ4 0.26 — 0.00% PCAR3 2.69 ▲ 3.86% GMAT3 3.99 ▼ 0.99% PSSA3 54.62 ▼ 0.15% CVCB3 1.36 ▲ 3.82% POSI3 3.54 ▼ 0.28% SLCE3 13.29 ▼ 0.67% NATU3 8.42 ▲ 0.48% BRKM5 5.83 ▼ 2.35% RANI3 8.22 ▲ 1.36% CSNA3 4.47 ▼ 7.64% CMIN3 5.67 ▼ 0.70% USIM5 7.41 ▲ 0.68% GGBR4 24.96 ▼ 0.08% ENEV3 26.59 ▲ 1.06% CPFE3 45.84 ▼ 0.65% CMIG4 11.23 ▼ 0.97% EQTL3 38.65 ▼ 0.03% LREN3 13.88 ▲ 2.06% VIVT3 32.59 ▼ 0.12% RAIL3 14.14 ▼ 2.08% KLABIN 18.24 ▼ 0.05% RAIA DROGASIL 18.66 ▲ 0.97% RDOR3 34.53 ▼ 0.32% HAPV3 11.55 ▲ 2.39% FLRY3 17.20 ▲ 0.35% SMTO3 14.47 ▼ 0.34% UGPA3 32.88 ▼ 0.51% VBBR3 36.04 ▼ 0.03% BBSE3 41.40 ▲ 0.34% BPAC11 57.04 ▲ 0.42% CURY3 31.23 ▲ 3.79% AERI3 2.17 ▲ 0.93% VIVARA 22.20 ▲ 0.09% COMPASS 24.70 ▼ 0.56% VAMOS 3.29 ▼ 1.50% SANB11 28.70 ▲ 0.28% ASAI3 8.47 ▼ 0.35% SBSP3 27.44 ▼ 0.94% WALMEX 50.10 ▼ 0.30% GMEXICO 209.15 ▲ 0.69% FEMSA 218.18 ▼ 1.48% CEMEX 20.79 ▲ 1.37% GFNORTE 199.60 ▼ 0.49% BIMBO 61.87 ▼ 0.15% TELEVISA 9.67 ▼ 1.43% AMX 21.89 ▼ 0.82% GAP 374.09 ▼ 0.65% ASUR 277.32 ▲ 0.62% OMA 230.43 ▼ 0.39% KOF 187.67 ▲ 0.22% GRUMA 259.90 ▲ 0.65% KIMBER 40.22 ▲ 0.05% SQM-B 62,001 ▼ 1.11% COPEC 6,350 — 0.00% BSANTANDER 80.19 ▼ 0.99% FALABELLA 6,230 ▲ 0.23% ENELAM 87.95 ▼ 0.05% CENCOSUD 1,955 — 0.00% CMPC 1,059 ▲ 0.41% BANCO CHILE 192.44 ▼ 0.66% LATAM AIR 25.28 ▲ 2.18% YPF 8,255 ▼ 0.42% GGAL 7,925 ▲ 0.55% PAMPA 5,480 ▼ 1.35% TXAR 655.00 ▼ 0.68% ALUAR 967.00 ▼ 1.07% TGS 9,905 ▼ 1.44% CEPU 2,383 ▼ 0.54% MIRGOR 16,450 ▲ 0.61% COME 43.54 ▼ 1.11% LOMA NEGRA 3,595 ▼ 0.69% BYMA 292.50 ▼ 1.02% TELECOM ARG 4,438 ▲ 0.68% ECOPETROL 16.52 ▼ 1.49% BANCOLOMBIA 91.35 ▼ 1.26% GRUPO AVAL 5.24 ▼ 0.76% CREDICORP 399.63 ▼ 0.24% SOUTHERN COPPER 183.51 ▲ 0.44% BUENAVENTURA 30.44 ▲ 0.53% MERCADOLIBRE 1,884 ▲ 0.32% NUBANK 14.34 ▲ 0.03% XP 17.01 ▼ 0.29% PAGSEGURO 9.60 ▼ 0.47% STONE 11.28 ▼ 0.88% GLOBANT 37.20 ▲ 1.63% TECNOGLASS 45.36 ▲ 4.41% GAP 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0.32% HAPV3 11.55 ▲ 2.39% FLRY3 17.20 ▲ 0.35% SMTO3 14.47 ▼ 0.34% UGPA3 32.88 ▼ 0.51% VBBR3 36.04 ▼ 0.03% BBSE3 41.40 ▲ 0.34% BPAC11 57.04 ▲ 0.42% CURY3 31.23 ▲ 3.79% AERI3 2.17 ▲ 0.93% VIVARA 22.20 ▲ 0.09% COMPASS 24.70 ▼ 0.56% VAMOS 3.29 ▼ 1.50% SANB11 28.70 ▲ 0.28% ASAI3 8.47 ▼ 0.35% SBSP3 27.44 ▼ 0.94% WALMEX 50.10 ▼ 0.30% GMEXICO 209.15 ▲ 0.69% FEMSA 218.18 ▼ 1.48% CEMEX 20.79 ▲ 1.37% GFNORTE 199.60 ▼ 0.49% BIMBO 61.87 ▼ 0.15% TELEVISA 9.67 ▼ 1.43% AMX 21.89 ▼ 0.82% GAP 374.09 ▼ 0.65% ASUR 277.32 ▲ 0.62% OMA 230.43 ▼ 0.39% KOF 187.67 ▲ 0.22% GRUMA 259.90 ▲ 0.65% KIMBER 40.22 ▲ 0.05% SQM-B 62,001 ▼ 1.11% COPEC 6,350 — 0.00% BSANTANDER 80.19 ▼ 0.99% FALABELLA 6,230 ▲ 0.23% ENELAM 87.95 ▼ 0.05% CENCOSUD 1,955 — 0.00% CMPC 1,059 ▲ 0.41% BANCO CHILE 192.44 ▼ 0.66% LATAM AIR 25.28 ▲ 2.18% YPF 8,255 ▼ 0.42% GGAL 7,925 ▲ 0.55% PAMPA 5,480 ▼ 1.35% TXAR 655.00 ▼ 0.68% ALUAR 967.00 ▼ 1.07% TGS 9,905 ▼ 1.44% CEPU 2,383 ▼ 0.54% MIRGOR 16,450 ▲ 0.61% COME 43.54 ▼ 1.11% LOMA NEGRA 3,595 ▼ 0.69% 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Ozone Hole Over Antarctica Peaks at 24 Million Square Kms, Greatest in Last Decade

By · October 14, 2020 · 3 min read

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RIO DE JANEIRO, BRAZIL – The annually occurring ozone hole over the Antarctic is one of the largest and deepest in recent years. Analyses show that the hole has reached its maximum size. The 2020 ozone hole grew rapidly from mid-August and peaked at around 24 million square kilometers in early October. It now covers 23 million km2, above average for the last decade, and spreading over most of the Antarctic continent.

The annually occurring ozone hole over the Antarctic is one of the largest and deepest in recent years. Analyses show that the hole has reached its maximum size. The 2020 ozone hole grew rapidly from mid-August and peaked at around 24 million square kilometers in early October.
The annually occurring ozone hole over the Antarctic is one of the largest and deepest in recent years. (Photo internet reproduction)
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WMO’s Global Atmosphere Watch program works closely with Copernicus Atmospheric Monitoring Service, NASA, Environment and Climate Change Canada and other partners to monitor the Earth’s ozone layer, which protects us from the harmful ultraviolet rays of the sun.

NASA’s Ozone Watch reports a lowest value of 95 Dobson Units recorded on October 1. Scientists are seeing signs that the 2020 ozone hole now seems to have reached its maximum extent.

“There is much variability in how far ozone hole events develop each year. The 2020 ozone hole resembles the one from 2018, which also was a quite large hole, and is definitely in the upper part of the pack of the last fifteen years or so”, Vincent-Henri Peuch, Director of Copernicus Atmosphere Monitoring Service at ECMWF, said in a news release.

“With the sunlight returning to the South Pole in the last weeks, we saw continued ozone depletion over the area. After the unusually small and short/lived ozone hole in 2019, which was driven by special meteorological conditions, we are registering a rather large one again this year, which confirms that we need to continue enforcing the Montreal Protocol banning emissions of ozone depleting chemicals.”

Since the ban on halocarbons, the ozone layer has slowly been recovering; the data clearly show a trend in decreasing area of the ozone hole.

The latest WMO/UN Environment Program Scientific Assessment of Ozone Depletion, issued in 2018, concluded that the ozone layer was on the path of recovery and potential return of the ozone values over Antarctica to pre-1980 levels by 2060.

The large ozone hole in 2020 has been driven by a strong, stable and cold polar vortex, which kept the temperature of the ozone layer over Antarctica consistently cold.

Ozone depletion is directly related to the temperature in the stratosphere, which is the layer of the atmosphere between 10 km 50 km altitude. This is because polar stratospheric clouds, which have an important role in the chemical destruction of ozone, only form at temperatures below -78°C.

These polar stratospheric clouds contain ice crystals that can turn non-reactive compounds into reactive ones, which can then rapidly destroy ozone as soon as light from the sun becomes available to start the chemical reactions. This dependency on polar stratospheric clouds and solar radiation is the main reason the ozone hole is only seen in late winter/early spring.

Stratospheric ozone concentrations have been observed to have reduced to near-zero values over Antarctica around 20 to 25 km of altitude (50-100hPa), with the ozone layer depth coming just below 100 Dobson Units, about a third of its typical value outside of ozone hole events.

During the Southern Hemisphere spring season (August – October) the ozone hole over the Antarctic increases in size, reaching a maximum between mid-September and mid-October. When temperatures high up in the atmosphere (stratosphere) start to rise in late Southern Hemisphere spring, ozone depletion slows, the polar vortex weakens and finally breaks down, and by the end of December ozone levels have returned to normal.

This article was drafted with automated assistance and reviewed before publication. How we use AI · Report an error

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