Browse All : Tropical Cyclone and Tropical Rainfall Measuring Mission (TRMM) of Australia

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Tropical Cyclone Daryl
Title Tropical Cyclone Daryl
Description This pair of images shows the birth of Cyclone Daryl off the northwest coast of Western Australia on January 19, 2006. In the fifteen hours that elapsed between the time the Tropical Rainfall Measuring Mission (TRMM [ http://trmm.gsfc.nasa.gov/ ]) satellite captured the top image at 10:08 a.m. Australian Western Standard Time and when it captured the bottom image at 1:00 a.m., Daryl went from a weak, newly named storm to a mature storm roughly equivalent to a Category 1 hurricane on the Saffir-Simpson scale. The storm's center remained just offshore as it moved southwest along the coast, sparing coastal communities a direct hit. Both images show rain rates in the storm. In the top image, TRMM reveals that despite having a sizeable band of intense rain (dark red segment) centered in a broad area of light (blue areas) to occasionally moderate (green areas) rain, Daryl showed very little evidence of circulation. This lack of circulation indicated that Daryl was in the early stages of development. At the time of this image, Daryl was rated as a Category 1 cyclone by the Australian Bureau of Meteorology's Tropical Cyclone Warning Center, indicating peak wind gusts of less than 125 kilometers per hour (78 miles per hour)—equivalent to a tropical storm. The lower image was taken just 15 hours later at 17:00 UTC (1:00 a.m. Australian WST on January 20) and shows a very different-looking storm. Although Daryl did not have a well-defined closed eye, the heavy rain had separated into arcing bands (green and darker red arcs), indicating that Daryl had a more mature circulation than it did earlier. Daryl became a Category 3 cyclone the following day. Catching Tropical Cyclone Daryl in the act of building may provide new and critical data for understanding the complexities of storm intensification. Becuase storms tend to form and intensify well away from land, scientists are still trying to understand how cyclones intensify. Armed with both passive and active sensors, including the first and only precipitation radar in space, TRMM has proven itself to be a valuable tool for examining tropical cyclones. These images show rain rates as measured by a number of different sensors on the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar, while rain rates in the outer swath are from the TRMM Microwave Imager. The rain rates are overlaid on infrared data from the TRMM Visible Infrared Scanner. Launched in November 1997 to measure rainfall over the global tropics, TRMM is a joint mission between NASA and the Japanese space agency, JAXA. Images produced by Hal Pierce (SSAI, NASA/GSFC) and captioned by Steve Lang (SSAI, NASA/GSFC).
Tropical Cyclone Daryl
Title Tropical Cyclone Daryl
Description This pair of images shows the birth of Cyclone Daryl off the northwest coast of Western Australia on January 19, 2006. In the fifteen hours that elapsed between the time the Tropical Rainfall Measuring Mission (TRMM [ http://trmm.gsfc.nasa.gov/ ]) satellite captured the top image at 10:08 a.m. Australian Western Standard Time and when it captured the bottom image at 1:00 a.m., Daryl went from a weak, newly named storm to a mature storm roughly equivalent to a Category 1 hurricane on the Saffir-Simpson scale. The storm's center remained just offshore as it moved southwest along the coast, sparing coastal communities a direct hit. Both images show rain rates in the storm. In the top image, TRMM reveals that despite having a sizeable band of intense rain (dark red segment) centered in a broad area of light (blue areas) to occasionally moderate (green areas) rain, Daryl showed very little evidence of circulation. This lack of circulation indicated that Daryl was in the early stages of development. At the time of this image, Daryl was rated as a Category 1 cyclone by the Australian Bureau of Meteorology's Tropical Cyclone Warning Center, indicating peak wind gusts of less than 125 kilometers per hour (78 miles per hour)—equivalent to a tropical storm. The lower image was taken just 15 hours later at 17:00 UTC (1:00 a.m. Australian WST on January 20) and shows a very different-looking storm. Although Daryl did not have a well-defined closed eye, the heavy rain had separated into arcing bands (green and darker red arcs), indicating that Daryl had a more mature circulation than it did earlier. Daryl became a Category 3 cyclone the following day. Catching Tropical Cyclone Daryl in the act of building may provide new and critical data for understanding the complexities of storm intensification. Becuase storms tend to form and intensify well away from land, scientists are still trying to understand how cyclones intensify. Armed with both passive and active sensors, including the first and only precipitation radar in space, TRMM has proven itself to be a valuable tool for examining tropical cyclones. These images show rain rates as measured by a number of different sensors on the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar, while rain rates in the outer swath are from the TRMM Microwave Imager. The rain rates are overlaid on infrared data from the TRMM Visible Infrared Scanner. Launched in November 1997 to measure rainfall over the global tropics, TRMM is a joint mission between NASA and the Japanese space agency, JAXA. Images produced by Hal Pierce (SSAI, NASA/GSFC) and captioned by Steve Lang (SSAI, NASA/GSFC).
Tropical Cyclone Daryl
Title Tropical Cyclone Daryl
Description This pair of images shows the birth of Cyclone Daryl off the northwest coast of Western Australia on January 19, 2006. In the fifteen hours that elapsed between the time the Tropical Rainfall Measuring Mission (TRMM [ http://trmm.gsfc.nasa.gov/ ]) satellite captured the top image at 10:08 a.m. Australian Western Standard Time and when it captured the bottom image at 1:00 a.m., Daryl went from a weak, newly named storm to a mature storm roughly equivalent to a Category 1 hurricane on the Saffir-Simpson scale. The storm's center remained just offshore as it moved southwest along the coast, sparing coastal communities a direct hit. Both images show rain rates in the storm. In the top image, TRMM reveals that despite having a sizeable band of intense rain (dark red segment) centered in a broad area of light (blue areas) to occasionally moderate (green areas) rain, Daryl showed very little evidence of circulation. This lack of circulation indicated that Daryl was in the early stages of development. At the time of this image, Daryl was rated as a Category 1 cyclone by the Australian Bureau of Meteorology's Tropical Cyclone Warning Center, indicating peak wind gusts of less than 125 kilometers per hour (78 miles per hour)—equivalent to a tropical storm. The lower image was taken just 15 hours later at 17:00 UTC (1:00 a.m. Australian WST on January 20) and shows a very different-looking storm. Although Daryl did not have a well-defined closed eye, the heavy rain had separated into arcing bands (green and darker red arcs), indicating that Daryl had a more mature circulation than it did earlier. Daryl became a Category 3 cyclone the following day. Catching Tropical Cyclone Daryl in the act of building may provide new and critical data for understanding the complexities of storm intensification. Becuase storms tend to form and intensify well away from land, scientists are still trying to understand how cyclones intensify. Armed with both passive and active sensors, including the first and only precipitation radar in space, TRMM has proven itself to be a valuable tool for examining tropical cyclones. These images show rain rates as measured by a number of different sensors on the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar, while rain rates in the outer swath are from the TRMM Microwave Imager. The rain rates are overlaid on infrared data from the TRMM Visible Infrared Scanner. Launched in November 1997 to measure rainfall over the global tropics, TRMM is a joint mission between NASA and the Japanese space agency, JAXA. Images produced by Hal Pierce (SSAI, NASA/GSFC) and captioned by Steve Lang (SSAI, NASA/GSFC).
Tropical Cyclone Fay
Title Tropical Cyclone Fay
Description Tropical Cyclone Fay first developed into a tropical depression on the 16th of March 2004 in the Timor Sea west of Bathurst Island off the northern coast of Australia. Just twelve hours after becoming a depression, Fay became a named tropical storm with winds estimated at 35 knots (40 mph). From there, the system took a general west southwestward track parallel to the northwestern coastline of Australia. On the 18th of March, Fay was upgraded to a Category 1 cyclone with maximum sustained winds estimated at 65 knots (75 mph). Fay then continued to steadily gain in strength becoming a Category 2 cyclone on the 19th, a Category 3 cyclone on the 20th, and a powerful Category 4 cyclone on the 21st with maximum sustained winds reaching an estimated 120 knots (138 mph). Fay is expected now to take a more southerly track ahead of an advancing trough and threaten the coast of Western Australia. The Tropical Rainfall Measuring Mission (TRMM) satellite has monitored the development of Fay capturing several unique images of the storm as it grew into a major cyclone. The first image (top left) was taken at 21:11 UTC on 17 March 2004 (5:11 am Australian WST 18 March). It shows the horizontal distribution of rain rates as seen from above by the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar (PR), the first and only precipitation radar in space, while rain rates in the outer swath are from the TRMM Microwave Imager (TMI). These rain rates are overlaid on infrared (IR) data from the TRMM Visible Infrared Scanner (VIRS). At the time of this first image, Fay was still a tropical storm with winds estimated at 45 knots (52 mph). TRMM reveals that the storm is still organizing with no evidence of an eye. However, a sizeable area of intense 2-inch-per-hour rain rates (darker red area) exists near the center of circulation, and the heating generated from this rainfall can help to drive the storm's circulation and make it stronger. The next image taken over a day later at 06:05 UTC on the 19th (top right) shows that Fay had become much better organized. The banding evident in the moderate intensity rain field (green arcs) is more pronounced, and an eye has started to form in the southeast portion of the main rain area. An area of intense rain rates (darker reds) is embedded in the northwest quadrant of the eyewall. Fay was at the time a Category 1 cyclone with sustained winds of 75 knots (86 mph). The last two images were taken at 20:00 UTC on March 20. Fay was now a Category 3 cyclone with sustained winds of 100 knots (115 mph). The eye of the storm is now readily apparent with moderate (green) to heavy (red) rain rates in the northern, western and southern portions of the eyewall. The final image (bottom right) shows a vertical slice through the center of Fay. It shows the heavy rain (red area) in the western eyewall as well as intense rain (dark reds) associated with deep convection (vertical blue/green tower) in an outer, rainband well west of the center. TRMM is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
Tropical Cyclone Fay
Title Tropical Cyclone Fay
Description Tropical Cyclone Fay first developed into a tropical depression on the 16th of March 2004 in the Timor Sea west of Bathurst Island off the northern coast of Australia. Just twelve hours after becoming a depression, Fay became a named tropical storm with winds estimated at 35 knots (40 mph). From there, the system took a general west southwestward track parallel to the northwestern coastline of Australia. On the 18th of March, Fay was upgraded to a Category 1 cyclone with maximum sustained winds estimated at 65 knots (75 mph). Fay then continued to steadily gain in strength becoming a Category 2 cyclone on the 19th, a Category 3 cyclone on the 20th, and a powerful Category 4 cyclone on the 21st with maximum sustained winds reaching an estimated 120 knots (138 mph). Fay is expected now to take a more southerly track ahead of an advancing trough and threaten the coast of Western Australia. The Tropical Rainfall Measuring Mission (TRMM) satellite has monitored the development of Fay capturing several unique images of the storm as it grew into a major cyclone. The first image (top left) was taken at 21:11 UTC on 17 March 2004 (5:11 am Australian WST 18 March). It shows the horizontal distribution of rain rates as seen from above by the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar (PR), the first and only precipitation radar in space, while rain rates in the outer swath are from the TRMM Microwave Imager (TMI). These rain rates are overlaid on infrared (IR) data from the TRMM Visible Infrared Scanner (VIRS). At the time of this first image, Fay was still a tropical storm with winds estimated at 45 knots (52 mph). TRMM reveals that the storm is still organizing with no evidence of an eye. However, a sizeable area of intense 2-inch-per-hour rain rates (darker red area) exists near the center of circulation, and the heating generated from this rainfall can help to drive the storm's circulation and make it stronger. The next image taken over a day later at 06:05 UTC on the 19th (top right) shows that Fay had become much better organized. The banding evident in the moderate intensity rain field (green arcs) is more pronounced, and an eye has started to form in the southeast portion of the main rain area. An area of intense rain rates (darker reds) is embedded in the northwest quadrant of the eyewall. Fay was at the time a Category 1 cyclone with sustained winds of 75 knots (86 mph). The last two images were taken at 20:00 UTC on March 20. Fay was now a Category 3 cyclone with sustained winds of 100 knots (115 mph). The eye of the storm is now readily apparent with moderate (green) to heavy (red) rain rates in the northern, western and southern portions of the eyewall. The final image (bottom right) shows a vertical slice through the center of Fay. It shows the heavy rain (red area) in the western eyewall as well as intense rain (dark reds) associated with deep convection (vertical blue/green tower) in an outer, rainband well west of the center. TRMM is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
Tropical Cyclone Fay
Title Tropical Cyclone Fay
Description After meandering off the coast of western Australia, Cyclone Fay finally came ashore back on the 27th of March 2004 as a powerful Category 4 cyclone with maximum sustained winds estimated at 115 knots (132 mph). The cyclone quickly weakened over land. The Tropical Rainfall Measuring Mission (TRMM) satellite captured several unique images of Fay along its path (please, see the previous TRMM story on Cyclone Fay). The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center monitors rainfall over the global tropics. MPA rainfall totals are shown for western Australia and the eastern Indian Ocean in association with the passage of Fay for the period 20 to 27 March 2004. The heaviest rainfall totals are by far and away located over the eastern Indian Ocean. The darker red areas show rainfall totals due to Fay on the order of 12 inches in this region. The heaviest totals appear to the right of the storm track (shown by the white storm symbols plotted every 06Z). These heavy amounts are the product of an intense rain band located well to the north west of the center that was observed by TRMM starting back on the 19th of March. The highest totals over land appear right along the coast and are on the order of 3 to 5 inches (green areas). A swath of 1 to 2 inch amounts (blue areas) extends inland over Western Australia. TRMM is a joint mission between NASA and the Japanese space agency JAXA. Image produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
Tropical Cyclone Fay
Title Tropical Cyclone Fay
Description After meandering off the coast of western Australia, Cyclone Fay finally came ashore back on the 27th of March 2004 as a powerful Category 4 cyclone with maximum sustained winds estimated at 115 knots (132 mph). The cyclone quickly weakened over land. The Tropical Rainfall Measuring Mission (TRMM) satellite captured several unique images of Fay along its path (please, see the previous TRMM story on Cyclone Fay). The TRMM-based, near-real time Multi-satellite Precipitation Analysis (MPA) at the NASA Goddard Space Flight Center monitors rainfall over the global tropics. MPA rainfall totals are shown for western Australia and the eastern Indian Ocean in association with the passage of Fay for the period 20 to 27 March 2004. The heaviest rainfall totals are by far and away located over the eastern Indian Ocean. The darker red areas show rainfall totals due to Fay on the order of 12 inches in this region. The heaviest totals appear to the right of the storm track (shown by the white storm symbols plotted every 06Z). These heavy amounts are the product of an intense rain band located well to the north west of the center that was observed by TRMM starting back on the 19th of March. The highest totals over land appear right along the coast and are on the order of 3 to 5 inches (green areas). A swath of 1 to 2 inch amounts (blue areas) extends inland over Western Australia. TRMM is a joint mission between NASA and the Japanese space agency JAXA. Image produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
Tropical Cyclone Fritz
Title Tropical Cyclone Fritz
Description Tropical Cyclone Fritz first formed into a tropical cyclone on 10 February 2004 in the Coral Sea east of Queensland, Australia. The storm then came ashore on the morning of the 11th (LST) as a minimal cyclone along the northeast coastline of Queensland just north of Cape Melville. Most of the rainfall with Fritz was away from the center near Weipa to the north and Cairns to the south. The system weakened into a tropical depression over land and continued moving westward cutting across the Cape York Peninsula before re-emerging over the waters of the Gulf of Carpentaria. It then re-intensified back into a Category 1 cyclone on the 12th. Fritz's circulation, however, was too disrupted over land to have time to get too well organized and thus allow for significant strengthening. However, it did manage to reach Category 2 status with peak wind gusts exceeding 125 kph (75 mph) before crossing Mornington Island in the southern Gulf of Carpentaria. Fritz then made landfall again on the far northwest coast of Queensland. The Tropical Rainfall Measuring Mission (TRMM) satellite captured these unique images of Cyclone Fritz while it was in the southern Gulf of Carpentaria. The images were taken at 14:18 UTC on 11 February 2004 (12:18 am Australian EST 12 February 2004). At the time, Fritz was categorized as a Category 1 cyclone by the Brisbane Tropical Cyclone Warning Centre with peak wind gusts of less then 125 kph (75 mph). The first image shows the horizontal distribution of rain rates as seen by the TRMM satellite. Rain rates in the center swath are from the TRMM Precipitation Radar (PR), the first precipitation radar in space, while rain rates in the outer swath are from the TRMM Microwave Imager (TMI). The rain rates are overlaid on infrared (IR) data from the TRMM Visible Infrared Scanner (VIRS). Fritz is shown to have a poorly organized circulation with no discernable eyewall. At this time only small, isolated areas of heavy rainfall are present (dark red spots). Tropical cyclones need the heat that is released when water vapor condenses into the cloud droplets that form the precipitation to drive the storm. This process is most efficient when the storm is well-organized and the heating takes place near the center. The second image shows a vertical cross section looking towards the west through the northern part of storm from the TRMM PR. It shows areas of heavy rainfall (darker reds) associated with rainbands away from the center of circulation. TRMM is a joint mission between NASA and the Japanese space agency JAXA. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
Tropical Cyclone Hubert
Title Tropical Cyclone Hubert
Description The Tropical Rainfall Measuring Mission (TRMM) flew directly over Tropical Cyclone Hubert as the storm was building off Australia's northwestern coast on April 6, 2006. Hubert is one of the seasonal storms that form between December and April in the region between Australia's northwestern coast and the western islands of the Indonesian chain. In a typical year, the cyclone season winds down in April when the Asian Monsoon developing in the north shifts storm formation away from the Australian coastline. The 2006 Australian cyclone season has seen just slightly more than the typical number of storms, including the unusually powerful Cyclone Glenda, which swept over northwestern Australia in late March. The TRMM satellite brought its full suite of instruments to bear on Tropical Cyclone Hubert. The outer regions of the storm were observed by the Visible and Infrared Scanner instrument, showing the extent and structure of clouds in the building storm. Superimposed on top of the clouds (wide outer swath) is the rain intensity, as detected by passive microwave energy using the TRMM Microwave Radiometer. The innermost swath shows the rain intensity as measured by the TRMM Precipitation Radar (PR). Reds indicated the heaviest rain regions, with the PR instrument able to peer into the clouds to discern the structure and intensity of the storm. The spiral structure of the rain bands, with the most intense rainfall in the storm center, is not at all obvious to other instruments, where the absence of a clear eye structure disguises the underlying storm form. TRMM's unique abilities provide insight into pressing questions in meteorological research, particularly in critical areas such as how storm systems form and intensify. TRMM observed Hubert at 10:47 a.m. local time (02:47 UTC) on April 6, 2006. At the time of this observation, Hubert was strong enough to be classified as a cyclone, but not particularly intense. Cyclone Hubert had a basic spiral form, but lacked the well-developed eye and tight-wound shape of a powerful storm. The PR observations show that the spiral structure and eye formation existed within the storm even though it was not evident in the cloud tops. Sustained, peak winds in the storm system were roughly 100 kilometers per hour (65 miles per hour) around the time the image was captured. The Tropical Rainfall Measurement Mission is shared between NASA and the Japanese space agency, JAXA. More detailed images of hurricane rain structure can be found on the TRMM website. [ http://trmm.gsfc.nasa.gov/ ] NASA image courtesy of Hal Pierce, SSAI/Goddard Space Flight Center
Tropical Cyclone Monica
Title Tropical Cyclone Monica
Description Cyclone Monica became the strongest storm of the 2006 Australian cyclone season with wind gusts reaching 350 kilometers per hour (215 miles per hour) as reported by the Australian Bureau of Meteorology's Cyclone Warning Centre. The Category 5 cyclone hit along the sparsely populated coastline of the Northern Territory, sparing the city of Darwin. Monica originated in the Coral Sea below the southeastern tip of Papua New Guinea, becoming a minimal tropical storm on April 17, 2006. The storm tracked due west towards the Cape York Peninsula in Queensland, where it came ashore just south of Lockart River on the afternoon of April 19 as a Category 3 cyclone. Monica weakened as it crossed the peninsula, but when it reached the warm waters of the Gulf of Carpentaria on the other side, it re-organized and re-intensified. The image above shows Cyclone Monica during this re-intensification. The visualization combines data from several different instruments from the Tropical Rainfall Measuring Mission (TRMM) satellite, which observed the storm at 16:08 UTC on April 22, 2006 (1:38 a.m., April 23, Australian CST). With an active radar and a passive microwave sensor, TRMM can peer into the core of these storms and relay important details on storm structure and location to forecasters. In this case, TRMM showed a pattern of very heavy rain (red) forming an intense symmetric eyewall around a small, complete eye with tightly curved rainbands spiraling into the center—the signature of a mature, intense tropical cyclone. Rain rates in the center swath are from the TRMM Precipitation Radar, and rain rates in the outer swath are from the TRMM Microwave Imager. The rain rates are overlaid on infrared data from the TRMM Visible Infrared Scanner. At the time of this TRMM overpass, Monica's sustained winds were estimated to be 230 kilometers/hour (144 mph) or equivalent to a Category 4 hurricane on the Saffir-Simpson scale. Soon after these images were taken, Monica reached Category 5 status with sustained winds estimated at 285 km/hr (178 mph). The cyclone tracked westward, skirting the northern coastline of Australia before coming ashore west of Maningrida in the Northern Territory just after 8 p.m. local time. The storm quickly lost strength as it moved inland and passed by the main population center of Darwin. TRMM is a joint mission between NASA and the Japanese space agency, JAXA. TRMM made several passes over Monica, during both the early and the mature stages of the storm. Since its launch in 1997, TRMM has provided valuable information on tropical storms. With an active radar and a passive microwave sensor, TRMM can peer into the core of these storms and relay details on storm structure and location to forecasters. Images produced by Hal Pierce (SSAI/NASA GSFC) and caption by Steve Lang (SSAI/NASA GSFC).
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