Announcement – Call for Papers: Global Human Health
By Maeve Hickok, posted on April 26th, 2010 in Announcements, Articles, Earth Observation, Health
www.Earthzine.org is soliciting articles worldwide for its theme issue on observing and monitoring Global Human Health, including contributions addressing current issues, techniques and applications of remote sensing, GIS, and geovisualization. We seek articles that document the use of Earth information and observing technologies that benefit human health, medical communities, governmental and NGO policy planners, and disaster response teams. The theme issue is scheduled for the third quarter of 2010, June 21 – September 21. Global Human Health Guest Editor is Assaf Anyamba, PhD. For more detail on the types of articles that are of interest and the formats for submission, please consult the Call for Papers. You can also help Earthzine reach potential contributors and readers by downloading the CfP, and forwarding or posting it within your network.
The photo to the right depicts two Anopheles gambiae mosquitoes as the female at the top of the image, was in the process of egg-laying atop a sheet of egg paper. The male is at the bottom of the image. A. gambiae is the principal vector of malaria in Africa.
Malaria is a serious and sometimes fatal disease caused by a parasite that commonly infects a certain type of mosquito which feeds on humans. People who get malaria are typically very sick with high fevers, shaking chills, and flu-like illness. Although malaria can be a deadly disease, illness and death from malaria can usually be prevented.
About 1,500 cases of malaria are diagnosed in the United States each year. The vast majority of cases in the United States are in travelers and immigrants returning from countries where malaria transmission occurs, many from sub-Saharan Africa and South Asia. Photo: US Centers for Disease Control
NASA Daily Image
Remnant of a Supernova
Vital clues about the devastating ends to the lives of massive stars can be found by studying the aftermath of their explosions. In its more than twelve years of science operations, NASA's Chandra X-ray Observatory has studied many of these supernova remnants sprinkled across the galaxy. The latest example of this important investigation is Chandra's new image of the supernova remnant known as G350.1-0.3. This stellar debris field is located some 14,700 light years from the Earth toward the center of the Milky Way. Evidence from Chandra and from ESA's XMM-Newton telescope suggest that a compact object within G350.1+0.3 may be the dense core of the star that exploded. The position of this likely neutron star, seen by the arrow pointing to "neutron star" in the inset image, is well away from the center of the X-ray emission. If the supernova explosion occurred near the center of the X-ray emission then the neutron star must have received a powerful kick in the supernova explosion. Data suggest this supernova remnant, as it appears in the image, is 600 and 1,200 years old. If the estimated location of the explosion is correct, this means the neutron star has been moving at a speed of at least 3 million miles per hour since the explosion. Another intriguing aspect of G350.1-0.3 is its unusual shape. Many supernova remnants are nearly circular, but G350.1-0.3 is strikingly asymmetrical as seen in the Chandra data in this image (gold). Infrared data from NASA's Spitzer Space Telescope (light blue) also trace the morphology found by Chandra. Astronomers think that this bizarre shape is due to stellar debris field expanding into a nearby cloud of cold molecular gas. The age of 600-1,200 years puts the explosion that created G350.1-0.3 in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because of the obscuring gas and dust that lies along our line of sight to the remnant. These results appeared in the April 10, 2011 issue of The Astrophysical Journal. Image Credits: X-ray: NASA/CXC/SAO/I. Lovchinsky et al; IR: NASA/JPL-Caltech