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Page Title: SATELLITE IMAGERY
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Rules for Forecasting the Intensity of Highs
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Aerographers Mate 1 & C
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SATELLITE IMAGERY PRINCIPLES

other. An estimate of the effects of each must be made before a decision is reached. · When surface pressure falls occur near the center and in the forward quadrants of the high, the high will weaken. · When  a  cold  high  that  is  moving  southward  is being  heated  from  below,  it  will  weaken,  unless  the heating  is  compensated  by  intensification  of  the  ridge aloft. The amount of intensification can be determined by correlating the contributions of height change at the 500-hPa level as progged and the change in thickness as advected. SATELLITE IMAGERY The  AG2  TRAMAN,  volume  1,  provides  a  detailed discussion  of  satellite   imagery   analysis.   It   may   be beneficial   to   review   Unit   10   before   you   read   this chapter. Satellite  imagery  provides  the  forecaster  with  an aid   in   forecasting   the   deepening   of   surface   low- pressure     systems.     In     the     following     series     of illustrations, both visual and infrared imagery depicts the  cloud  features  over  a  60-hour  period  during  the deepening  of  a  low-pressure  system.  See  figures  3-10 through 3-15. In  figure  3-10,  the  visual  pass  at  noon  local  time shows  a  large  cloud  mass  with  a  low  level  vortex centered  near  A.  A  frontal  band,  B,  extends  to  the southwest from the large cloud mass. The beginning of a dry tongue is evident. An interesting cloud band, C, which appears just north of the cloud mass, is of about the same brightness as the major cloud mass. The  infrared  scan  for  midnight,  figure  3-11,  shows the further development of the vortex with penetration of  the  dry  tongue.  Low-level  circulation  is  not  visible, but  the  brightness  (temperature)  distribution  differs from  the  visual  picture.  The  detail  within  the  frontal band is apparent, with a bright cold line, DE, along the upstream  edge  of  the  band.  In  all  probability,  this  is the cirrus generated  by  the  convection  near  the  polar jetstream.   The   cloud   band,   C,   from   the   previous (daylight) picture is seen in the IR, and is composed of lower clouds than would be anticipated from the video. By the second noon (fig. 3-12), the vortex is clearly defined, but again the spiral arm of the frontal band is nearly saturated, with a few shadows to provide detail on cloud layering. The National Meteorological Center (NMC) operational surface analysis during this period shows that the cyclone has deepened. Figure 3-11.-Infrared, local midnight, first night. In  figure  3-13,  the  pass  for  the  second  midnight shows the coldest temperatures form a hooked-shaped pattern  with  the  highest  cloudiness  still  equatorward of  the  vortex  center  at  F.  The  granular  gray-to-light- gray   temperature   within   the   dry   tongue   area,   G, suggests  cells  that  consist  of  cumulus  formed  from stratocumulus,    and    small    white    blobs    indicating cumulus congestus. The visual pass for the third noon (fig. 3-14) shows the  vortex  to  be  tightly  spiraled,  indicating  a  mature system.  The  frontal  band  is  narrower  than  it  was  24 hours earlier, with some cloud shadows present to aid in  determining  the  cloud  structure.  Surface  analysis indicates   that   the   lowest   central   pressure   of   the cyclone  was  reached  approximately  6  hours  prior  to this picture. The  final  pass  in  this  series  (fig.  3-15)  shows  the coldest  temperatures  completely  surround  the  vortex. The  frontal  band  also  shows  the  segmented  nature  of the  active  weather  areas  within  the  band.  A  typical vorticity 3-15

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