Pregled bibliografske jedinice broj: 640843
Satellite-based overshooting tops detection methods: comparison and validation
Satellite-based overshooting tops detection methods: comparison and validation // Croatian-USA Workshop on Mesometeorology
Zagreb, Hrvatska, 2012. (predavanje, nije recenziran, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 640843 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Satellite-based overshooting tops detection methods: comparison and validation
Autori
Mikuš, Petra ; Strelec Mahović, Nataša
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Skup
Croatian-USA Workshop on Mesometeorology
Mjesto i datum
Zagreb, Hrvatska, 18.06.2012. - 20.06.2012
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Nije recenziran
Ključne riječi
overshooting tops; satellite data; brightness temperature differences
Sažetak
Overshooting convective cloud top (OT) is a dome-like protrusion above a cumulonimbus anvil, often penetrating into the lower stratosphere. It represents a very strong updraft. A single OT exists for less than 30 minutes and has a maximum diametar of ~15 km. According to investigations, storms with OTs often produce hazardous weather conditions such as heavy rainfall, damaging winds, large hail, cloud-to-ground lightning and tornadoes. The OTs also generate gravity waves which can produce significant turbulence. These events represent a considerable hazard to property and human lives, but also to the air traffic. OTs are most easily identified in the high-resolution visible (HRV) channel imagery as the lumpy textured (cauliflower-like) appearance, however only during day-time. Consequently, the techniques which use combinations with solar satellite channels perform well only during the day time. Therefore satellite based methods for the detection of convective clouds and the heights of their tops are usually based on the infra-red window (IRW) measurements, available during both day and night. In the infrared 10.8 μm satellite imagery, a small group of very cold pixels can indicate the appearance of the OT. Due to the restriction of using visible images only during daytime, four detection methods based on the IR window channel 10.8 µm and the absorption channels of water vapor (6.2 µm), ozone (9.7 µm) and carbon dioxide (13.4 µm) in form of brightness temperature differences were used. The theoretical background of all four methods is explained and the results of detection are compared with the High Resolution Visible (HRV) satellite images during day-time, in order to validate each method. Out of four tested methods best performance is found for the combination of brightness temperature differences 6.2-10.8 and 9.7-10.8 µm, which are connected to the overshootings in HRV images in 80% of the cases.
Izvorni jezik
Engleski
Znanstvena područja
Geologija
POVEZANOST RADA
Projekti:
004-1193086-3036 - Oluje i prirodne katastrofe u Hrvatskoj (Ivančan-Picek, Branka, MZOS ) ( CroRIS)
Ustanove:
Državni hidrometeorološki zavod