SOLAR DYNAMICS OBSERVATORY: THE MOVIE

FROM: NASA

Three Years of SDO Data--Narrated

This version of Three Years of SDO Data is extended, and narrated by NASA's Goddard Space Flight Center heliophysicist Alex Young. He highlights many interesting aspects of the video and points out several of the single-frame events that appear in it. In the three years since it first provided images of the sun in the spring of 2010, NASA’s Solar Dynamics Observatory (SDO) has had virtually unbroken coverage of the sun's rise toward solar maximum, the peak of solar activity in its regular 11-year cycle. This video shows those three years of the sun at a pace of two images per day. Credit: NASA's Goddard Space Flight Center

GLOBAL WARMING AND RAINFALL

 

Model simulations spanning 140 years show that warming from carbon dioxide will change the frequency that regions around the planet receive no rain (brown), moderate rain (tan), and very heavy rain (blue). The occurrence of no rain and heavy rain will increase, while moderate rainfall will decrease. Credit: NASA's Goddard Space Flight Center Scientific Visualization Studio

FROM: NASA

NASA Study Projects Warming-Driven Changes in Global Rainfall

WASHINGTON -- A NASA-led modeling study provides new evidence that global warming may increase the risk for extreme rainfall and drought.

The study shows for the first time how rising carbon dioxide concentrations could affect the entire range of rainfall types on Earth.

Analysis of computer simulations from 14 climate models indicates wet regions of the world, such as the equatorial Pacific Ocean and Asian monsoon regions, will see increases in heavy precipitation because of warming resulting from projected increases in carbon dioxide levels. Arid land areas outside the tropics and many regions with moderate rainfall could become drier.

The analysis provides a new assessment of global warming's impacts on precipitation patterns around the world. The study was accepted for publication in the American Geophysical Union journal Geophysical Research Letters.

"In response to carbon dioxide-induced warming, the global water cycle undergoes a gigantic competition for moisture resulting in a global pattern of increased heavy rain, decreased moderate rain, and prolonged droughts in certain regions," said William Lau of NASA's Goddard Space Flight Center in Greenbelt, Md., and lead author of the study.

The models project for every 1 degree Fahrenheit of carbon dioxide-induced warming, heavy rainfall will increase globally by 3.9 percent and light rain will increase globally by 1 percent. However, total global rainfall is not projected to change much because moderate rainfall will decrease globally by 1.4 percent.

Heavy rainfall is defined as months that receive an average of more than about 0.35 of an inch per day. Light rain is defined as months that receive an average of less than 0.01 of an inch per day. Moderate rainfall is defined as months that receive an average of between about 0.04 to 0.09 of an inch per day.

Areas projected to see the most significant increase in heavy rainfall are in the tropical zones around the equator, particularly in the Pacific Ocean and Asian monsoon regions.

Some regions outside the tropics may have no rainfall at all. The models also projected for every degree Fahrenheit of warming, the length of periods with no rain will increase globally by 2.6 percent. In the Northern Hemisphere, areas most likely to be affected include the deserts and arid regions of the southwest United States, Mexico, North Africa, the Middle East, Pakistan, and northwestern China. In the Southern Hemisphere, drought becomes more likely in South Africa, northwestern Australia, coastal Central America and northeastern Brazil.

"Large changes in moderate rainfall, as well as prolonged no-rain events, can have the most impact on society because they occur in regions where most people live," Lau said. "Ironically, the regions of heavier rainfall, except for the Asian monsoon, may have the smallest societal impact because they usually occur over the ocean."

Lau and colleagues based their analysis on the outputs of 14 climate models in simulations of 140-year periods. The simulations began with carbon dioxide concentrations at about 280 parts per million -- similar to pre-industrial levels and well below the current level of almost 400 parts per million -- and then increased by 1 percent per year. The rate of increase is consistent with a "business as usual" trajectory of the greenhouse gas as described by the United Nations' Intergovernmental Panel on Climate Change.

Analyzing the model results, Lau and his co-authors calculated statistics on the rainfall responses for a 27-year control period at the beginning of the simulation, and also for 27-year periods around the time of doubling and tripling of carbon dioxide concentrations.
They conclude the model predictions of how much rain will fall at any one location as the climate warms are not very reliable.

"But if we look at the entire spectrum of rainfall types we see all the models agree in a very fundamental way -- projecting more heavy rain, less moderate rain events, and prolonged droughts," Lau said.

IRIS TO HELP SCIENTISTS UNDERSTAND SUN'S PHYSICAL PROCESSES



Workers unload NASA's IRIS spacecraft from a truck at the processing facility at Vandenberg where the spacecraft will be readied for launch aboard an Orbital Sciences Pegasus XL rocket. Photo credit: VAFB/Randy Beaudoin

FROM: NASA

NASA’s Interface Region Imaging Spectrograph (IRIS) satellite arrived at Vandenberg Air Force Base in California on Tuesday, April 16, to begin its final preparations for launch currently scheduled no earlier than May 28. IRIS will improve our understanding of how heat and energy move through the deepest levels of the sun’s atmosphere, thereby increasing our ability to forecast space weather. Following final checkouts, the IRIS spacecraft will be placed inside an Orbital Sciences Pegasus rocket. Deployment of the Pegasus from the L-1011 carrier aircraft is targeted for 7:27 p.m. PDT at an altitude of 39,000 feet at a location over the Pacific Ocean about 100 miles northwest of Vandenberg AFB off the central coast of California south of Big Sur.

"IRIS will contribute significantly to our understanding of the interface region between the sun's photosphere and corona," said Joe Davila, IRIS mission scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "This region is crucial for understanding how the corona gets so hot."

IRIS carries a single instrument, a multi-channel imaging spectrograph with an ultraviolet (UV) telescope that will help scientists better understand the physical processes in the sun’s interface region.

"With the high-resolution images from IRIS, scientists will be able to use advanced computer models to unravel how matter, light, and energy move from the sun’s 6,000 Kelvin surface to its million Kelvin corona," said Eric Ianson, IRIS mission manager at NASA Goddard. "Scientists will be able to combine data from NASA’s IRIS and Solar Dynamics Observatory and the NASA/JAXA Hinode missions to obtain a more comprehensive understanding of the sun’s atmosphere."

IRIS is a NASA Small Explorer mission. The program provides frequent flight opportunities for world-class scientific investigations from space using innovative, streamlined and efficient management approaches within the heliophysics and astrophysics areas.

NASA's Launch Services Program at Kennedy Space Center, Fla., is responsible for launch management. Lockheed Martin’s Advanced Technology Center Solar and Astrophysics Laboratory in Palo Alto, Calif., designed and built the IRIS spacecraft and instrument. NASA’s Ames Research Center in Moffett Field, Calif., is responsible for mission operations and ground data systems.

A STUDY OF ASTEROID 1999 RQ36

FROM: NASA
OSIRIS-REx Targets Near-Earth Asteroid
NASA is sending the OSIRIS-REx spacecraft to asteroid 1999 RQ36 to better understand the evolution of its orbit and to retrieve a pristine sample for study on Earth. Credit-NASA's Goddard Space Flight Center

CRATER SCIENCE

FROM: NASA
Planetary CSI: Crater Science Investigations
If you want to learn more about the history of Earth and other rocky planets in the solar system, craters are a great place to look. Now, thanks to LRO's LROC instrument, we can take a much closer look at Linné Crater on the moon--a pristine crater that's great to use to compare with other craters!

Credit-NASA's Goddard Space Flight Center

HIGH-RESOLUTION GLOBAL ATMOSPHERIC MODELING GIVES LOOK AT GLOBAL AERSOLS

FROM: NASA
Portrait of Global Aerosols
High-resolution global atmospheric modeling run on the Discover supercomputer at the NASA Center for Climate Simulation at Goddard Space Flight Center, Greenbelt, Md., provides a unique tool to study the role of weather in Earth's climate system. The Goddard Earth Observing System Model, Version 5 (GEOS-5) is capable of simulating worldwide weather at resolutions of 10 to 3.5 kilometers (km).

This portrait of global aerosols was produced by a GEOS-5 simulation at a 10-kilometer resolution. Dust (red) is lifted from the surface, sea salt (blue) swirls inside cyclones, smoke (green) rises from fires, and sulfate particles (white) stream from volcanoes and fossil fuel emissions.

Image credit-William Putman, NASA-Goddard

NASA VIDEO: EXPLORATION OF THE EARLY UNIVERSE

NASA's Fermi Explores the Early Universe

This animation tracks several gamma rays through space and time, from their emission in the jet of a distant blazar to their arrival in Fermi's Large Area Telescope (LAT). During their journey, the number of randomly moving ultraviolet and optical photons (blue) increases as more and more stars are born in the universe. Eventually, one of the gamma rays encounters a photon of starlight and the gamma ray transforms into an electron and a positron. The remaining gamma-ray photons arrive at Fermi, interact with tungsten plates in the LAT, and produce the electrons and positrons whose paths through the detector allows astronomers to backtrack the gamma rays to their source.

Credit: NASA's Goddard Space Flight Center/Cruz ...

NASA TESTS NEW SPACE TELESCOPE

FROM:  NASA
Several critical items related to NASA's next-generation James Webb Space Telescope currently are being tested in the thermal vacuum test chamber at NASA's Goddard Space Flight Center, Greenbelt, Md. This image shows the Optical Telescope Element Simulator, or OSIM, wrapped in a silver blanket on a platform, being lowered into the Space Environment Simulator vacuum chamber via crane to be tested to withstand the cold temperatures of space. Image Credit: NASA/Chris Gunn

NASA RECRUITS AMATEUR ASTRONOMERS TO TARGET ASTEROIDS

WASHINGTON -- A new NASA outreach project will enlist the help of
amateur astronomers to discover near-Earth objects (NEOs) and study
their characteristics. NEOs are asteroids with orbits that
occasionally bring them close to the Earth.

Starting today, a new citizen science project called "Target
Asteroids!" will support NASA's Origins Spectral Interpretation
Resource Identification Security - Regolith Explorer (OSIRIS-REx)
mission objectives to improve basic scientific understanding of NEOs.
OSIRIS-REx is scheduled for launch in 2016 and will study material
from an asteroid.

Amateur astronomers will help better characterize the population of
NEOs, including their position, motion, rotation and changes in the
intensity of light they emit. Professional astronomers will use this
information to refine theoretical models of asteroids, improving
their understanding about asteroids similar to the one OSIRIS-Rex
will encounter in 2019, designated 1999 RQ36.

OSIRIS-REx will map the asteroid's global properties, measure
non-gravitational forces and provide observations that can be
compared with data obtained by telescope observations from Earth. In
2023, OSIRIS-REx will return back to Earth at least 2.11 ounces (60
grams) of surface material from the asteroid.

Target Asteroids! data will be useful for comparisons with actual
mission data. The project team plans to expand participants in 2014
to students and teachers.

"Although few amateur astronomers have the capability to observe 1999
RQ36 itself, they do have the capability to observe other targets,"
said Jason Dworkin, OSIRIS-REx project scientist at NASA's Goddard
Space Flight Center in Greenbelt, Md.
Previous observations indicate 1999 RQ36 is made of primitive
materials. OSIRIS-REx will supply a wealth of information about the
asteroid's composition and structure. Data also will provide new
insights into the nature of the early solar system and its evolution,
orbits of NEOs and their impact risks, and the building blocks that
led to life on Earth.

Amateur astronomers long have provided NEO tracking observations in
support of NASA's NEO Observation Program. A better understanding of
NEOs is a critically important precursor in the selection and
targeting of future asteroid missions.

"For well over 10 years, amateurs have been important contributors in
the refinement of orbits for newly discovered near-Earth objects,"
said Edward Beshore, deputy principal investigator for the OSIRIS-REx
mission at the University of Arizona in Tucson.

NASA's Goddard Space Flight Center in Greenbelt, Md., will provide
overall mission management, systems engineering and safety and
mission assurance for OSIRIS-REx. Dante Lauretta is the mission's
principal investigator at the University of Arizona. Lockheed Martin
Space Systems in Denver will build the spacecraft. OSIRIS-REx is the
third mission in NASA's New Frontiers Program. NASA's Marshall Space
Flight Center in Huntsville, Ala., manages New Frontiers for the
agency's Science Mission Directorate in Washington.