NASA's TRMM satellite saw Tropical Storm Karina get a boost on August 22 in the form of some moderate rainfall and towering thunderstorms in the center of the storm.
The Tropical Rainfall Measuring Mission or TRMM satellite passed directly above the center of Tropical Storm Karina on August 22, 2014 at 0151 UTC (Aug. 21 at 9:51 p.m. EDT).
A rainfall analysis that used data from TRMM's Microwave Imager (TMI) showed that storms near Karina's center were dropping rain at a rate near 25 mm/1 inch per hour.
Where the heaviest rainfall was occurring, TRMM spotted a couple of towering thunderstorms as high as 15 km (~9 miles).
NOAA's GOES-West satellite captured Tropical Storm Karina, Tropical Storm Lowell and Tropical Storm Marie in an infrared image on Aug. 22 at 5 a.m. EDT.
Karina appeared to be in the lead of the triple tropical train of storms moving through the Eastern Pacific Ocean. The image showed how much smaller and compact Karina is in comparison to Tropical Storm Lowell.
At 11 a.m. EDT, Tropical Storm Karina's maximum sustained winds had increased to near 70 mph (110 kph), and the National Hurricane Center (NHC) noted that some fluctuations in intensity are possible before Karina begins to weaken on August 23.
The center of Tropical Storm Karina was located near latitude 15.0 north and longitude 135.6 west, about 1,325 miles (2,130 km) east of Hilo, Hawaii. Karina is moving to the northeast near 3 mph (6 kph) and is expected to turn to the east-northeast as it continues being affected by nearby Tropical Storm Lowell.
Forecaster Roberts at NHC noted that in two days Karina should be on a weakening trend because the storm will be moving into cooler waters and it will run into stable, dry air.
Text credit: Rob Gutro
NASA's Goddard Space Flight Center
Rob Gutro | Eurek Alert!
NASA finds newly formed tropical storm lan over open waters
17.10.2017 | NASA/Goddard Space Flight Center
The melting ice makes the sea around Greenland less saline
16.10.2017 | Aarhus University
University of Maryland researchers contribute to historic detection of gravitational waves and light created by event
On August 17, 2017, at 12:41:04 UTC, scientists made the first direct observation of a merger between two neutron stars--the dense, collapsed cores that remain...
Seven new papers describe the first-ever detection of light from a gravitational wave source. The event, caused by two neutron stars colliding and merging together, was dubbed GW170817 because it sent ripples through space-time that reached Earth on 2017 August 17. Around the world, hundreds of excited astronomers mobilized quickly and were able to observe the event using numerous telescopes, providing a wealth of new data.
Previous detections of gravitational waves have all involved the merger of two black holes, a feat that won the 2017 Nobel Prize in Physics earlier this month....
Material defects in end products can quickly result in failures in many areas of industry, and have a massive impact on the safe use of their products. This is why, in the field of quality assurance, intelligent, nondestructive sensor systems play a key role. They allow testing components and parts in a rapid and cost-efficient manner without destroying the actual product or changing its surface. Experts from the Fraunhofer IZFP in Saarbrücken will be presenting two exhibits at the Blechexpo in Stuttgart from 7–10 November 2017 that allow fast, reliable, and automated characterization of materials and detection of defects (Hall 5, Booth 5306).
When quality testing uses time-consuming destructive test methods, it can result in enormous costs due to damaging or destroying the products. And given that...
Using a new cooling technique MPQ scientists succeed at observing collisions in a dense beam of cold and slow dipolar molecules.
How do chemical reactions proceed at extremely low temperatures? The answer requires the investigation of molecular samples that are cold, dense, and slow at...
Scientists from the Max Planck Institute of Quantum Optics, using high precision laser spectroscopy of atomic hydrogen, confirm the surprisingly small value of the proton radius determined from muonic hydrogen.
It was one of the breakthroughs of the year 2010: Laser spectroscopy of muonic hydrogen resulted in a value for the proton charge radius that was significantly...
17.10.2017 | Event News
10.10.2017 | Event News
10.10.2017 | Event News
18.10.2017 | Health and Medicine
18.10.2017 | Life Sciences
17.10.2017 | Life Sciences