Transcript

IZVESTIYA, ATMOSPHERIC AND OCEANIC PHYSICS Vol. 48 No. 9 2012

CARBON MONOXIDE EMISSIONS IN SUMMER 2010 IN THE CENTRAL PART OF THE RUSSIAN PLAIN AND ESTIMATION OF THEIR UNCERTAINTIES

WITH THE USE OF DIFFERENT LAND�COVER MAPS

A. N. SAFRONOV, E. V. FOKEEVA, V. S. RAKITIN, L. N. YURGANOV, AND E. I. GRECHKO

s5

s6

s4

s1

s2

s3

1:25000000 Terra 07.08.2010

Moscow

0 1:3000000250 500 1000 1500 2000km 0 37.5 75 150 225 300

km

peat

GLC�2000

12345678910111213141516171819202122

Moscow

Fig. 1. The land cover map GLC�2000 (SPOT�4/VGN) Global v1.1 and peatland nearby megacity Moscow. The s1–s6 symbolsmark the major underground peat fires. The big rivers and reservoirs are shown in Fig. 1 additionally. The hotspots at August 7,2010, obtained by MODIS/Terra, are presented on the tab.

MCD14ML Terra01.08−09.08 2010FRP, MW

0−5051−100101−150151−200201−250251−500501−10001001−3000

s1

Envisat MERIS�210, lakes and rivers (2009). 1:3000000 2 4 8 12 16

km

1:3000000 2 4 8 12 16

kmEnvisat MERIS�210, lakes and rivers (2009).

s1

MCD4501.08−09.08 2010

fire

Fig. 4. The details of peatland located nearby s1 model source are illustrated on GoogleEarth satellite photos. The dark squares indi�cate the peat mining. The drainage system is look like blue color lines between the dark squares. The water surface as map layer wasadded according to Envisat/MERIS�210 satellite data as of 2009 year status. The hotspot locations, which obtained during temporalperiod from August 1 to August 9, 2010, by MODIS/Terra satellite data (MCD14ML, method AF), are displayed on Fig. 4a as pointswith different colors, graduated by FRP values. The burned area locations, obtained by MODIS/Terra (MCD45, method BA) withthe same temporal period, were shown on Fig. 4b as red squares.

IZVESTIYA, ATMOSPHERIC AND OCEANIC PHYSICS Vol. 48 No. 9 2012

CARBON MONOXIDE EMISSIONS IN SUMMER 2010 IN THE CENTRAL PART OF THE RUSSIAN PLAIN AND ESTIMATION OF THEIR UNCERTAINTIES

WITH THE USE OF DIFFERENT LAND�COVER MAPS

A. N. SAFRONOV, E. V. FOKEEVA, V. S. RAKITIN, L. N. YURGANOV, AND E. I. GRECHKO


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