mercredi 19 août 2015

Japanese HTV-5 Cargo Mission Launches and Reaches Orbit












JAXA - H-II Transfer Vehicle HTV-5 Mission logo.

August 19, 2015


Image above: The Japan Aerospace Exploration Agency (JAXA)’s H-IIB rocket launched at 7:50 a.m. EDT on Wednesday, Aug. 19, 2015. Image Credit: JAXA.

Right on schedule, the Japan Aerospace Exploration Agency (JAXA)’s H-IIB rocket launched at 7:50 a.m. EDT on Wednesday, Aug. 19 from the Tanegashima Space Center in southern Japan. At the time of launch, the space station was flying 250 miles above the Atlantic Ocean east of Brazil.

Approximately 15 minutes after launch, the HTV-5 cargo spacecraft successfully separated from the rocket and began its five-day rendezvous with the International Space Station. The spacecraft is carrying more than 9,500 pounds of research and supplies for the six-person station crew, including the CALorimetric Electron Telescope (CALET) investigation, an astrophysics mission that will search for signatures of dark matter and provide the highest energy direct measurements of the cosmic ray electron spectrum.

Japanese Cargo Ship Sets Sail for the Space Station

JAXA and NASA teams adjusted the cargo manifest to deliver additional food supplies and critical components lost in the failure of the seventh SpaceX commercial resupply services mission. The delivery will ensure the crew has plenty of food through the end of 2015. HTV-5 is delivering two multifiltration beds that filter contaminants from the station’s water supply, a Fluids Control and Pump Assembly used for urine processing to support water recycling, a Wring Collector used in conjunction with the on-orbit toilet, a Respiratory Support Pack used in space to provide breathing assistance to an astronaut in the event lung function were impaired and space suit support equipment used during spacewalks.

On Monday, Aug. 24, JAXA Flight Engineer Kimiya Yui will use the Canadarm2 robotic arm to capture the unpiloted HTV spacecraft at approximately 6:55 a.m. NASA TV coverage Friday will begin at 5:15 a.m. NASA Flight Engineer Kjell Lindgren will provide assistance as necessary. The HTV will spend five weeks attached to the Earth-facing port of the Harmony module on the international outpost.

Follow the conversation on Twitter via @Space_Station and the hashtag #HTV5. To learn more about all the ways to connect and collaborate with NASA, visit: http://www.nasa.gov/connect

For more information on the International Space Station and its crews, visit: http://www.nasa.gov/station

Japan Aerospace Exploration Agency (JAXA): http://global.jaxa.jp/

KOUNOTORI 5 (HTV-5): http://global.jaxa.jp/projects/rockets/htv/

Image (mentioned), Video, Text, Credits: NASA/JAXA.

Best regards, Orbiter.ch

mardi 18 août 2015

Suomi NPP Satellite Sees Typhoon Goni's Strongest Sides













NASA / NOAA - Suomi-NPP Mission logo.

Aug. 18, 2015

Goni (was 16W - Northwest Pacific Ocean)


Image above: NASA-NOAA's Suomi satellite captured an infrared image of Goni on August 18 at 12:18 a.m. EDT that showed the strongest thunderstorms (red) with the coldest cloud top temperatures were in the eastern and southern quadrants. Image Credits: NRL/NASA/NOAA.

NASA-NOAA's Suomi NPP satellite passed over Typhoon Goni and gathered infrared data that helped identify the strongest part of the storm as the south and eastern quadrants.

The Visible Infrared Imaging Radiometer Suite (VIIRS) instrument aboard NASA-NOAA's Suomi satellite captured an infrared image of Goni on August 18 at 4:18 UTC (12:18 a.m. EDT) that showed the strongest thunderstorms with the coldest cloud top temperatures (near -63F/-53C) were in the eastern and southern quadrants.

The Joint Typhoon Warning Center noted that animated enhanced infrared satellite imagery showed a slight warming of convective tops, which means that they weren't reaching as high into the troposphere as a result of weakening uplift or push in the atmosphere. Otherwise, the system has maintained overall convective signature with tightly-curved banding wrapping into a 15-nautical mile diameter eye.

At 1500 UTC (11 a.m. EDT), on August 18, Typhoon Goni had maximum sustained winds near 100 knots (115.1 mph/185.2 kph).That makes Goni a Category Three typhoon on the Saffir-Simpson Scale. Goni is not expected to strengthen further.

Suomi satellite. Image Credit: NASA

It was centered near 18.8 North latitude and 132.1 East longitude, about 546 nautical miles (628 miles/ 1,011 km) east-southeast of Kadena Air Base, Okinawa, Japan. Goni was moving to the west at 16 knots (18.4 mph/29.6 kph).

The Joint Typhoon Warning Center expects Goni to approach and pass north of Luzon, Philippines by August 20 and 21 before approaching Taiwan from the southeast.

For more information about Suomi-NPP satellite mission, visit: http://npp.gsfc.nasa.gov/

Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Rob Gutro.

Greetings, Orbiter.ch

Expedition 44 Crew Readies for Arrival of Fifth Resupply Mission










ISS - Expedition 44 Mission patch.

August 18, 2015

The six-member Expedition 44 crew participated in a wide array of science today as Japan counts down to Wednesday morning’s launch of its fifth resupply mission. Meanwhile, three new Soyuz taxi crew members flew to the launch site at the Baikonur Cosmodrome to finalize their mission preparations.

The majority of the station crew members had their blood pressure and vision checked today for the long-running Ocular Health study. Japanese astronaut Kimiya Yui had his legs scanned with an ultrasound for the SPRINT exercise study. NASA astronaut Kjell Lindgren explored fluid physics and surface tension for the Capillary Beverage experiment.


Image above: Japanese astronaut Kimiya Yui soars through the Destiny lab module. Image Credit: NASA.

Back on Earth, veteran station cosmonaut Sergei Volkov and first time Soyuz Flight Engineers Andreas Mogensen and Aidyn Aimbetov are getting ready for their 10-day mission to the International Space Station. The trio will launch Sept. 2 inside the Soyuz TMA-18M spacecraft from the Baikonur Cosmodrome in Kazakhstan. Volkov will stay in space until next year. Mogensen and Aimbetov will return Sept. 11 with Gennady Padalka who has been in space since March.

The Japan Aerospace Exploration Agency (JAXA) is getting ready to roll out its H-IIB rocket this afternoon at the Tanegashima Space Center. JAXA is scheduled to launch the “Kounotori” HTV-5 cargo craft at 7:50 a.m. EDT (11:50 a.m. UTC) Wednesday for a five day trip to the space station. The HTV-5 will deliver more than 4.5 tons of research and supplies, including water, spare parts and experiment hardware.

Aurora's Colorful Veil Over Earth

Image above: NASA astronaut Scott Kelly (@StationCDRKelly) shared this photograph on social media Twitter, taken from the International Space Station on August 15, 2015. Kelly wrote, "#Aurora trailing a colorful veil over Earth this morning. Good morning from @space_station! #YearInSpace". Image Credit: NASA.

The dancing lights of the aurora provide spectacular views, but also capture the imagination of scientists who study incoming energy and particles from the sun. Aurora are one effect of such energetic particles, which can speed out from the sun both in a steady stream called the solar wind and due to giant eruptions known as coronal mass ejections or CMEs. After a trip toward Earth that can last two to three days, the solar particles and magnetic fields cause the release of particles already trapped near Earth, which in turn trigger reactions in the upper atmosphere in which oxygen and nitrogen molecules release photons of light. The result: the Northern and Southern lights.

Related links:

Ocular Health study: http://www.nasa.gov/mission_pages/station/research/experiments/204.html

SPRINT exercise study: http://www.nasa.gov/mission_pages/station/research/experiments/972.html

Capillary Beverage experiment: http://www.nasa.gov/mission_pages/station/research/experiments/2029.html

NASA Resources on Aurorae: http://www.nasa.gov/mission_pages/sunearth/aurora-news-stories/index.html

For more information on the International Space Station and its crews, visit: http://www.nasa.gov/station

Images (mentioned), Text, Credits: NASA/Sarah Loff.

Best regards, Orbiter.ch

lundi 17 août 2015

NASA's LADEE Spacecraft Finds Neon in Lunar Atmosphere












NASA - LADEE Mission patch.

Aug. 17, 2015

The moon's thin atmosphere contains neon, a gas commonly used in electric signs on Earth because of its intense glow. While scientists have speculated on the presence of neon in the lunar atmosphere for decades, NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft has confirmed its existence for the first time.


Image above: Artist’s concept of NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft in orbit above the moon. Image Credits: NASA Ames/Dana Berry.

"The presence of neon in the exosphere of the moon has been a subject of speculation since the Apollo missions, but no credible detections were made," said Mehdi Benna of NASA's Goddard Space Flight Center in Greenbelt, Maryland and the University of Maryland, Baltimore County. "We were very pleased to not only finally confirm its presence, but to show that it is relatively abundant." Benna is lead author of a paper describing observations from LADEE's Neutral Mass Spectrometer (NMS) instrument published May 28 in Geophysical Research Letters.

There's not enough neon to make the moon visibly glow because the moon's atmosphere is extremely tenuous, about 100 trillion times less dense than Earth's atmosphere at sea level. A dense atmosphere like Earth's is relatively rare in our solar system because an object has to be sufficiently massive to have enough gravity to hold onto it.

The behavior of a dense atmosphere is driven by collisions between its atoms and molecules. However, the moon's atmosphere is technically referred to as an exosphere because it’s so thin, its atoms rarely collide. Exospheres are the most common type of atmosphere in our solar system, so scientists are interested in learning more about them. "It's critical to learn about the lunar exosphere before sustained human exploration substantially alters it," Benna said. Since the moon's atmosphere is so thin, rocket exhaust and outgassing from spacecraft could easily change its composition.

Most of the moon's exosphere comes from the solar wind, a thin stream of electrically conducting gas blown from the surface of the sun into space at around a million miles per hour. Most of the solar wind is hydrogen and helium, but it contains many other elements in small amounts, including neon. All these elements impact the moon, but only helium, neon, and argon are volatile enough to be returned back to space. The rest of the elements will stick indefinitely to the moon’s surface.

The LADEE NMS instrument confirms that the moon’s exosphere is made up of mostly helium, argon, and neon. Their relative abundance is dependent on the time of day on the moon--argon peaks at sunrise, with neon at 4 a.m. and helium at 1 a.m. The instrument conducted systematic measurements of these gases for seven months, which allowed the team to understand how these gases are supplied to the exosphere, and how they are ultimately lost.

While most of the lunar exosphere comes from the solar wind, NMS showed that some gas comes from lunar rocks. Argon-40 results from the decay of naturally occurring radioactive potassium-40, found in the rocks of all the terrestrial planets as a leftover from their formation.

"We were also surprised to find that argon-40 creates a local bulge above an unusual part of the moon's surface, the region containing Mare Imbrium and Oceanus Procellarum," said Benna. Although the reason for this local enhancement is not yet understood, "One could not help to notice that this region happens to be the place where potassium-40 is most abundant on the surface. So there may be a connection between the atmospheric argon, the surface potassium and deep interior sources," said Benna.

A second surprising behavior of argon was that the overall amount in the lunar exosphere was not constant over time. Instead, it increased and then decreased by about 25 percent during the course of the LADEE mission. According to Benna, this transient source of argon may be the result of enhanced outgassing from the surface that is triggered by tidal stress on the moon.

NMS also revealed an unexpected source of some of the helium in the lunar exosphere. "About 20 percent of the helium is coming from the moon itself, most likely as the result from the decay of radioactive thorium and uranium, also found in lunar rocks," said Benna. This helium is being produced at a rate equivalent to about seven liters per second at standard atmospheric pressure.

"The data collected by the NMS addresses the long-standing questions related to the sources and sinks of exospheric helium and argon that have remained unanswered for four decades," said Benna. "These discoveries highlight the limitations of current exospheric models, and the need for more sophisticated ones in the future."

Launched in September 2013 from NASA's Wallops Flight Facility in Virginia, LADEE began orbiting the moon Oct. 6 and gathering science data Nov. 10. The spacecraft entered its science orbit around the moon's equator on Nov. 20, and in March 2014, LADEE extended its mission operations following a highly successful 100-day primary science phase. LADEE lacked fuel to maintain a long-term lunar orbit or continue science operations and was intentionally sent into the lunar surface, impacting the moon on April 17, 2014. The spacecraft's orbit naturally decayed following the mission's final low-altitude science phase.

For more information about the LADEE mission, visit: http://www.nasa.gov/ladee

Image, Text, Credits: NASA Goddard Space Flight Center/William Steigerwald/Bill Steigerwald.

Greetings, Orbiter.ch

Chasms on Dione












NASA - Cassini Mission to Saturn patch.

Aug. 17, 2015


While not bursting with activity like its system satellite Enceladus, the surface of Dione is definitely not boring. Some parts of the surface are covered by linear features, called chasmata, which provide dramatic contrast to the round impact craters that typically cover moons.

The bright network of fractures on Dione (698 miles or 1123 kilometers across) was seen originally at poor resolution in Voyager images and was labeled as "wispy terrain." The nature of this terrain was unclear until Cassini showed that they weren't surface deposits of frost, as some had suspected, but rather a pattern of bright icy cliffs among myriad fractures. One possibility is that this stress pattern may be related to Dione's orbital evolution and the effect of tidal stresses over time.

This view looks toward the trailing hemisphere of Dione. North on Dione is up. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on April 11, 2015.

The view was acquired at a distance of approximately 68,000 miles (110,000 kilometers) from Dione. Image scale is 2,200 feet (660 meters) per pixel.

Artist's view of Cassini approaching Dione

The Cassini mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov or http://www.nasa.gov/cassini . The Cassini imaging team homepage is at http://ciclops.org and http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens

Images, Text, Credits: NASA/JPL-Caltech/Space Science Institute/Tony Greicius.

Greetings, Orbiter.ch

vendredi 14 août 2015

Progress M-26M has successfully undocked from the ISS











ROSCOSMOS - Russian Vehicles patch.

14/08/2015

Progress-M space cargo undocking ISS. Image Credit: NASA TV

In accordance with the flight of the International Space Station on August 14, 2015 in 13 hours 18 minutes Moscow time, the command was given to undock cargo spacecraft Progress M-26M from the service module of the Russian segment of the ISS (13:19 - undocking). After removal of the ship to a safe distance from the station, Mission Control Center specialists have started FSUE TsNIIMash controlled reduction of the spacecraft from orbit.

The Progress M-26M was docked on ISS on February 17, 2015. After completing the main task of delivering needed to maintain the functioning of the station life systems for the crew (new filters and parts, food, water), was used for 12 orbit correction at providing ballistic flight station.

Russian Space Station Supply Ship Departs ISS

Video Credit: NASA TV.

According to the calculations of experts providing ballistic flight service station, engine of cargo ship Progress M-26M to be deorbited today in 16 hours 28 minutes Moscow time and, having worked on the braking pulse position, the ship was oriented to the descent to Earth.

At 17 hours 17 minutes Moscow Time fireproof structural elements of the ship fall in the estimated area of ​​non-navigational area of ​​the Pacific Ocean.

In accordance with the schedule of flights to the International Space Station, is scheduled for August 17 launch of the Japanese cargo spacecraft HTV-5 after 4 days is expected to dock with the ISS. Progress M-29M is scheduled for October 1, 2015.

ROSCOSMOS Press Release: http://www.federalspace.ru/21639/ and http://www.federalspace.ru/21641/

Image (mentioned), Video (mentioned), Text, Credits: Press Service of the Russian Federal Space Agency (ROSCOSMOS)/Orbiter.ch Aerospace.

Greetings, Orbiter.ch

How Does NASA Study Hurricanes?












NASA patch.

Aug. 14, 2015

Hurricanes are the most powerful weather event on Earth. NASA’s expertise in space and scientific exploration contributes to essential services provided to the American people by other federal agencies, such as hurricane weather forecasting.

The National Oceanic and Atmospheric Administration and the National Hurricane Center (NHC) use a variety of tools to predict these storms’ paths. These scientists need a wealth of data to accurately forecast hurricanes. NASA satellites, computer modeling, instruments, aircraft and field missions contribute to this mix of information to give scientists a better understanding of these storms.


Image above: This visible image of Hurricane Katrina was taken on August 29 at 05:16 UTC (1:16 a.m. EDT) by the MODIS instrument that flies aboard NASA's Aqua satellite as it approached landfall in Louisiana. Image Credits: NASA Goddard MODIS Rapid Response Team.

NASA's Research Role

NASA’s role as a research agency is to bring new types of observational capabilities and analytical tools to learn about the fundamental processes that drive hurricanes and work to help incorporate that data into forecasts. NASA collaborates with its interagency partners so that the nation benefits from our respective capabilities.

“Before we had satellites and aircraft, hurricanes would destroy entire cities, like the Labor Day Hurricane in Key West back in 1935,” said Gail Skofronick-Jackson, the project scientist for NASA’s Global Precipitation Measurement mission at NASA's Goddard Space Flight Center in Greenbelt, Maryland. “You would have no idea if a hurricane was coming until it was too late.”

Hurricanes in the Atlantic Ocean can form when sub-Saharan thunderstorms travel westward with areas of lower pressure. These troughs are known as African Easterly Waves. Warm, moist air rises within the storm clouds, drawing air into the thunderstorms. Like an ice skater pulling in her arms to increase her spin, this inward moving air increases the rotation of the air within the storm cloud. Moving across the warm Atlantic, this cycle repeats on a daily basis, and, with a favorable environment, potentially accelerates to create a monstrous vortex powered by oceanic heat.


Image above: MTSTAT and CloudSat imagery of Typhoon Dolphin. Image Credits: Natalie D. Tourville/Colorado State University.

NASA uses an arsenal of instruments to learn more about how these storms progress as they form. These devices orbit Earth on a fleet of spacecraft, including Aqua, Terra, the Global Precipitation Measurement core observatory, NASA-NOAA's Suomi NPP satellite, Calipso, Jason-2 and CloudSat.

“There are typically multiple instruments on every spacecraft with various purposes that often complement each other,” said Eric Moyer, the Earth science operations manager at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We can see the progression of a storm from one day to the next using the Terra and Aqua satellites—a morning and afternoon view of every storm system, every day.”

What NASA Studies

These instruments analyze different aspects of these storms, such as rainfall rates, surface wind speed, cloud heights, ocean heat and environmental temperature and humidity. Observing these factors helps identify the potential for storm formation or intensification. Similarly, the data allows meteorologists to better predict where, when and how hard hurricanes will strike land.

NASA's RapidScat instrument that flies aboard the International Space Station measures surface winds over the ocean and is used to gather data on tropical cyclones. This can show where in a hurricane the strongest winds occur. RapidScat continues a long satellite record of these observations that began with NASA's QuikScat satellite.

Scientists must completely understand a hurricane to predict its trajectory and strength. This means meteorologists must peer inside the cloud itself.

“Looking at the cloud structure can help us understand the storm’s structure and location, which improves our forecasts,” said Michael Brennan, a senior hurricane specialist at the National Oceanic and Atmospheric Administration’s National Hurricane Center. “We heavily rely on the passive microwave imagers from satellites to see what is happening in the core of the storm.”


Image above: This 3-D view of the area northeast of Typhoon Dolphin's eye on May 16 created by data from NASA/JAXA's GPM core satellite shows heaviest rain over the open waters of the Pacific Ocean at a rate of over 65 mm (2.6 inches) per hour. Image Credits: NASA/SSAI/JAXA, Hal Pierce.

Passive microwave imagers aboard NASA’s Global Precipitation Measurement and NASA-NOAA's Suomi National Polar-orbiting Partnership missions can peer through cloud canopies, allowing scientists to observe where the water is churning in the clouds.

“Just like a doctor using x-rays to understand what’s happening in the human body, our radiometers can pierce the clouds and understand the cyclone’s structure,” Skofronick-Jackson said. “We learn about the amount of liquid water and falling snow in the cloud. Then we know how much water may fall out over land and cause floods.”

“Having satellites to watch the oceans is critical, and that will never change,” Skofronick-Jackson said. “Radars on Earth can only see a certain distance out in the ocean, so without spacecraft, you would need radars on every ship. With satellite data informing computer models, we can predict the storms’ paths, to the point where regions only need to evacuate half as much coastline as before. That’s important, because it costs a lot of money to pack up, move to a hotel and close down businesses.”

Computer Modeling

Computer modeling is another powerful NASA research tool.

NASA's Global Modeling and Assimilation Office, or GMAO works to improve the understanding of hurricanes and assess models and procedures for quality. GMAO helps to identify information that was missing and determines what services could be added to help future investigation and prediction of hurricane systems.


Image above: On July 14, RapidScat saw the sustained winds surrounding Claudette's center of circulation were no stronger than 21 meters per second with the exception of stronger winds in the southwestern quadrant. Image Credits: NASA JPL/Doug Tyler.

As NASA launches more sophisticated Earth-observing instruments, teams produce models with higher and higher resolutions, the ability to ingest such data, or the data assimilation procedure, increases. Each new instrument provides scientists and modelers a closer and more varied look at tropical cyclones. The higher the resolution of models and the capability of data assimilation systems, the easier it is to exploit data from satellite-borne instruments and to determine a hurricane’s intensity and size in terms of things such as the wind field and cloud extent.

Airborne Missions

NASA also conducts field missions to study hurricanes. With an arsenal of instruments, ranging from radiometers that read moisture levels; lidars that measure aerosols, moisture, and winds; dropsonde systems to measure high-resolution profiles of temperature, pressure, moisture, and winds; to Doppler radar systems to map the 3-D precipitation and winds within storms. These instruments monitor the structure and environment of hurricanes and tropical storms as they evolve.



Image above: NASA's Hurricane and Severe Storm Sentinel (HS3) ran its field campaign phase during the summers of 2012, 2013, and 2014 performed by Global Hawk well-suited for hurricane investigations. Image Credit: NASA.

The most recent NASA field mission to study hurricanes was the Hurricane and Severe Storm Sentinel or HS3. For three consecutive years, the HS3 mission investigated the processes that underlie hurricane formation and intensity change in the Atlantic Ocean basin. The mission used the Global Hawk, a high-altitude long-endurance aircraft capable of flights of 26 hours at altitudes above 55,000 ft. Flying from the Wallops Flight Facility in Virginia, the uninhabited Global Hawks could cover the entire Atlantic Ocean, enabling measurements of storms at early stages in the central or eastern Atlantic or spending 12-18 hours over storms in the western Atlantic.

A Future Mission

In 2016, NASA is launching the Cyclone Global Navigation Satellite System, a constellation of eight small satellites. CYGNSS will probe the inner core of hurricanes in such detail to better understand their rapid intensification. One advantage of CYGNSS is that it can get frequent measurements within storms.  This allows CYGNSS to make accurate measurements of ocean surface winds both in and near the eye of the storm throughout the lifecycle of tropical cyclones. The goal is to improve hurricane intensity forecasts.

NASA data and research allows scientists to observe the fundamental processes that drive hurricanes. Meteorologists incorporate this satellite, aircraft and computer modeling data into forecasts in the United States and around the world.

For more on NASA’s hurricane observations and research, visit: http://www.nasa.gov/hurricane

Related links:

NASA’s Global Precipitation Measurement mission: http://www.nasa.gov/mission_pages/GPM/main/

NASA-NOAA's Suomi NPP satellite: http://npp.gsfc.nasa.gov/

NASA-NOAA's Calipso satellite: http://www.nasa.gov/mission_pages/calipso/main/

NASA-NOAA's Jason-2 satellite: http://www.nasa.gov/mission_pages/ostm/main/

NASA-NOAA's CloudSat satellite: http://www.nasa.gov/mission_pages/cloudsat/main/

Terra and Aqua satellites: http://modis.gsfc.nasa.gov/about/

NASA's QuikScat satellite: https://winds.jpl.nasa.gov/missions/quikscat/

Hurricane and Severe Storm Sentinel or HS3: http://www.nasa.gov/mission_pages/hurricanes/missions/hs3/index.html#.VcJzJYtjpMa

Cyclone Global Navigation Satellite System (CYGNSS): http://www.nasa.gov/cygnss/

Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Max Gleber/Karl Hille.

Best regards, Orbiter.ch