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METEOROLOGI
METEOROLOGIPelatihan OSK SMAN 2 TangerangTangerang, 14-15 Desember 2013Oleh : M. Reza Ardian TOIKI 2011
Disadur dari berbagai sumberKomposisi Atmosfer Dekat Permukaan Bumi
Permanen kadar tetapVariabel kadar berbeda-beda tergantung tempatUap AirGas variabel paling pentingMengontrol sebagian besar gejala-gejala cuacaKadar bisa hingga 4% di tempat yang benar-benar lembabTermasuk GRK
Transformasi Fasa Air
CO2
Sejarah Terbentuknya AtmosferKetika baru terbentuk, atmosfer bumi terdiri dari H2, He, serta senyawa ber-HGas lain? dari outgassing
N2 dan O2 dari mana?
Lapisan Atmosfer
TermosferMesosferStratosferTroposfer
Berdasarkan strukturtemperatur
TroposferRata-rata susut suhu sekitar 6,5C/kmKira-kira 80% total massa atmosferMengandung seluruh uap air dan aerosolKetinggian berbeda-beda (8-16 km) rt2 11 kmWell-stirred by convective air currentBoundary layerStratosfer
Lapisan inversi, shg not well-stirred & isotermalKarena??Lapisan O3serap UVTropopause s/d~50 km
MesosferMakin tinggi makin dingin50-80 kmSuhu terendah di atmosfer (-90C) pada mesopauseKebanyakan meteor yang sampai ke bumi biasanya terbakar di lapisan ini.99,9% massa atmosfer dibawah lapisan ini, shg sangat tipis
Termosfer80-500 kmKomposisi heterogenInversi akibat penyerapan radiasi oleh atom OTemperatur juga dipengruhi aktivitas matahari
EksosferMolekul ringan H2 bisa melepaskan diriO2, H2, He
Berdasarkan Komposisi
HomosphereNitrogen and oxygen are wellmixed (~78% and ~21%)
HeterosphereAtom berat diatas, atom ringan di bawahIonosferAtom-atom terionisasiXray, UV
Ionosfer dan Komunikasi
Unsur CuacaSuhuTekananKelembabanAwanPresipitasiVisibilitasAngin
TEMPERATURTemperatur
Kalor Spesifik
Kalor Laten
Transfer KalorKonduksiKonveksiRadiasi
Parsel udara naik ekspansi, mendinginParsel udara turun kompresi, memanas
Radiasi EM
Hukum Wien
max = 2897 m K / T(K)Albedo
Mengapa makin atas makin dingin?
GRKwater vapor, carbon dioxide, methane, nitrous oxide, and ozone.
Neraca Energi
Aurora
Insolation (Incoming Solar Radiation)
Lama Siang dan Malam
Empat Musim
Gerak Semu Matahari Berdasarkan Lintang
Net Radiation
HarianTahunanTEKANANTekanan
Profil Tekanan
Gaya Gradien Tekanan
Gaya Coriolis
Angin Geostrofik
Angin Gradien
Isobar
KelembapanUdara lembap = udara kering + uap air
Ukuran KelembapanKelembapan mutlak (g H2O / m3 udara lembap)Kelembapan spesifik (g H2O / kg udara lembap)Kelembapan relatif (RH)Mixing ratio (g H2O / kg udara kering)Tekanan uap & tekanan uap jenuhTitik Embun (Suhu dimana RH = 100%)Temperatur bola basahTemperatur bola keringTekanan Uap
RH
Titik EmbunDepresi titik embun = selisih T dengan TdT > TdDepresi titik embun berbanding terbalik dengan kelembapan
ContohSuatu parsel udara bersuhu 27C memiliki titik embun 21C. Berapa kelembaban relatifnya?Suatu parsel udara bersuhu 21C memiliki kelembaban relatif 84%. Berapa titik embunnya?
Pemanasan dan Pendinginan AdiabatikAdiabatik tidak ada kalor yang keluar masukKarena sifat udara yang menghantar kalor dengan burukAdiabatik Kering (10C/km)Adiabatik Jenuh (6,5C/km)Stabilitas AtmosferStabil dan Tidak Stabil
Pada UdaraStabil Jika diturunkan/ dinaikkan, kembali ke posisi semulaTidak stabil Jika diturunkan/ dinaikkan, jalan terus
Angin : Sirkulasi Global & LokalSkala Gerak Atmosfer
Sirkulasi 3 sel
-Hadley-Ferrel-KutubITCZ
Easterly windWesterly windAngin pasatDistribusi Presipitasi Berdasar Lintang
Turbulensi TermalParsel udara naik karena pemanasan permukaanBiasa terjadi tengah hari
Angin Fohn
Angin Fohn di berbagai daerahBahorok Dataran rendah Deli UtaraKumbang CirebonGending ProbolinggoGenggong PasuruanBrubu MakassarWambraw Biak
Gelombang Lee
Angin Darat Angin LautCp darat < Cp lautDarat lebih cepat menyerap & melepas kalorAkibatnya, pada siang hari daratan lebih cepat panasPada malam hari, daratan lebih cepat dingin
Angin Gunung Angin Lembah
KONDENSASI & AWANInti KondensasiDibutuhkan suatu partikel higroskopis untuk mengkondensasi uap airDebu, asap, SO2, garam, dsb0,001 mikron 10 mikron
KondensasiSebelum RH 100% jika ada inti kondensasiEfek larutan vs efek kelengkungan
Klasifikasi Awan
ENVI 1400 : Meteorology and Forecasting75High-Level CloudsCirrus (Ci): White, delicate, fibrous in appearance. Forms in patches or narrow bands. May for comma-shaped streaks or mares tails (cirrus uncinus)
Cirrus clouds are formed entirely of ice crystals. These grow and evaporate slowly, leading to soft edges to clouds.ENVI 1400 : Meteorology and Forecasting76
Cirrostratus (Cs): Thin, transparent sheet or veil; sun clearly visible & casting shadows at surface. A halo may be seen around the sun (or moon). Sheets of cirrostratus may cover entire sky, and be up to several 1000m deep.
ENVI 1400 : Meteorology and Forecasting77Cirrocumulus (Cc): Thin white patch or sheet of cloud; appears dappled or rippled. Dappling results from convective overturning within the cloud, ripples from gravity waves.
Aircraft contrails: condensation from aircraft exhaust. May dissipate quickly, or be very long-lived depending on conditions.ENVI 1400 : Meteorology and Forecasting78Medium-Level CloudsAltostratus (As): A greyish sheet of cloud, may be fibrous or uniform in appearance. Thin enough in parts to make out the sun, but no halo.
ENVI 1400 : Meteorology and Forecasting79Altocumulus (Ac): white or grey patches arranged in sheets. Shape and texture are variable.There are several distinct sub-classes of altocumulus
ENVI 1400 : Meteorology and Forecasting80Altocumulus lenticularis (Ac len): white or grey lenticular (lens shaped) clouds formed by the lifting of air over a topographic barrier.
ENVI 1400 : Meteorology and Forecasting81
Altocumulus castellanus (Ac cas): white or grey, broken cumulus-like clouds; upper part appearing castle-like. Sometimes arranged in lines.
ENVI 1400 : Meteorology and Forecasting82
Altocumulus undulatus (Ac und): white or grey patches or sheets of cloud with an undulating or rippled appearance.
ENVI 1400 : Meteorology and Forecasting83Low-Level Clouds
Cumulus (Cu): Brilliant white to grey, dense detached clouds. Forms clumped or heaped (cauliflower-like) shapes, usually with sharp outlines and flat base. Field of Cu often have bases all at same (lifting condensation) level.
ENVI 1400 : Meteorology and Forecasting84Cumulus humilis (Cu hum): small cumulus, of limited vertical extent, may have a flattened appearance. Also called fair-weather cumulus
ENVI 1400 : Meteorology and Forecasting85Cumulus mediocris : cumulus, of moderate vertical extent.
ENVI 1400 : Meteorology and Forecasting86
Cumulus congestus: crowded (congested) field of cumulus or greater vertical extent. May produce rain.ENVI 1400 : Meteorology and Forecasting87
Pileus : cap clouds that form above large cumulus as the upward motion of the convective cloud distorts the layer of air above (pileus is latin for skull-cap)ENVI 1400 : Meteorology and Forecasting88
ENVI 1400 : Meteorology and Forecasting89
Cumulonimbus (Cb) : huge towering cloud, dark base and white sides. Associated with heavy rain, thunderstorms, and hail. Frequently has an anvil shaped top.ENVI 1400 : Meteorology and Forecasting90
mammatus : smooth, rounded shapes sometimes formed on the underside of cumulonimbus; they result from downdrafts within the cloud.ENVI 1400 : Meteorology and Forecasting91Stratocumulus (Sc) : white or grey sheet of cloud, usually formed in mounds or rolls.
ENVI 1400 : Meteorology and Forecasting92
ENVI 1400 : Meteorology and Forecasting93
ENVI 1400 : Meteorology and Forecasting94
Stratocumulus with virga hair-like strands of falling rain, which evaporate below cloud before reaching the surface.ENVI 1400 : Meteorology and Forecasting95Stratus (St) : grey featureless layer of cloud with a uniform base. Often associated with drizzle or snow.
ENVI 1400 : Meteorology and Forecasting96Nimbostratus (Ns) : Dark grey, featureless, thick layer of cloud. Associated with prolonged precipitation. Commonly forms in frontal systems
Arcus
Fibratus
Inkus
LainnyaUndulatusFraktusFibratusKalvusKapilatusNebulosusTranslucidusUncinusdllSiklus Hidup Awan Kumulus
Presipitasi