Showing posts with label STP. Show all posts
Showing posts with label STP. Show all posts

Thursday, March 6, 2014

JAXA Hinode SOT Solar Image: Sunspot Activity - Active Region 11967

Active Region 11967 consisted of a major sunspot that released numerous solar flares in early 2014. 

Above is an image taken by the Solar Optical Telescope (SOT) aboard Hinode in the Calcium II H line on Feb. 7, 2014 at 16:09 UT. 

Below is a wider view of Active Region 11967 as seen by SDO on Feb.12, 2014, at 01:35 UT. 

By studying the sun's magnetic field, scientists hope to shed new light on explosive solar activity that can interfere with satellite communications and electric power transmission grids on Earth and threaten astronauts on the way to or working on the surface of the moon. 

Solar Optical Telescope (SOT)
In particular they want to learn if they can identify the magnetic field configurations that lead to these explosive energy releases and use this information to predict when these events may occur. 

The Honide mission is led by the Japan Aerospace Exploration Agency (JAXA), and is a collaboration between the space agencies of Japan, the United States, the United Kingdom and Europe. 

NASA helped in the development, funding and assembly of the spacecraft's three science instruments. 

Hinode is part of the Solar Terrestrial Probes (STP) Program within the Heliophysics Division of NASA's Science Mission Directorate in Washington, which are also responsible for the Solar Dynamcis Observatory (SDO). 

Image credit: NASA/JAXA/Lockheed Martin

Wednesday, March 5, 2014

NASA Lightning Imaging Sensor (LIS) to Capture 'Striking' Lightning Data

Flight hardware backups allow NASA to seamlessly continue work in the unlikely event something goes down for a repair.

When projects end, these handy spares can sometimes find second lives in new areas for use.

Researchers at NASA’s Marshall Space Flight Center in Huntsville, Ala., developed a sophisticated piece of flight hardware called a Lightning Imaging Sensor (LIS) to detect and locate lightning over the tropical region of the globe.

Launched into space in 1997 as part of NASA’s Tropical Rainfall Measuring Mission (TRMM), the sensor undertook a three-year baseline mission, delivering data used to improve weather forecasts.

It continues to operate successfully aboard the TRMM satellite today.

The team that created this hardware in the mid-1990s built a spare -- and now that second unit is stepping up to contribute, as well.

The sensor is scheduled to launch on a Space Exploration Technologies (SpaceX) Falcon 9 rocket to the International Space Station in February 2016.

Once mounted to the station, it will serve a two-year baseline mission as part of a U.S. Department of Defense (DoD) Space Test Program (STP)-H5 science and technology development payload.

STP-H5 is integrated and flown under the management and direction of the DoD's STP.

NASA selected the LIS spare hardware to fly to the space station in order to take advantage of the orbiting laboratory’s high inclination.

This vantage point gives the sensor the ability to "look" farther towards Earth's poles than the original LIS can aboard the TRMM satellite.

Once installed, the sensor will monitor global lightning for Earth science studies, provide cross-sensor calibration and validation with other space-borne instruments, and ground-based lightning networks.

LIS will also supply real-time lightning data over data-sparse regions, such as oceans, to support operational weather forecasting and warning.

"Only LIS globally detects all in-cloud and cloud-to-ground lightning -- what we call total lightning -- during both day and night," said Richard Blakeslee, LIS project scientist at Marshall.

"As previously demonstrated by the TRMM mission, better understanding lightning and its connections to weather and related phenomena can provide unique and affordable gap-filling information to a variety of science disciplines including weather, climate, atmospheric chemistry and lightning physics.”

LIS measures the amount, rate and radiant energy of global lightning, providing storm-scale resolution, millisecond timing, and high, uniform-detection efficiency -- and it does this without land-ocean bias.