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Recent Articles
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Female Afghan police make their markWritten by U.S. Army Sgt. 1st Class John D. Brown
Forward Operating Base Fenty, Afghanistan – Members of the Bastogne Female Engagement Team, 1st Brigade Combat Team, 101st Airborne Division, sat down with female members of the Afghan Uniformed Police (AUP) and Afghan Border Police (ABP) to develop a greater understanding of the roles women play within the AUP and ABP in Nangarhar Province January 19th at the ABP Zone 1 compound in Jalalabad, Afghanistan. ![]() 1st Brigade Combat Team, 101st Airborne Division Female Engagement Team members Spc. Samantha Banda, from La Feria, Texas, Spc. Bianca Roig from Eagle Pass, Texas, and Sgt. Stacey Coffield from Orange County, Calif. discuss a variety of issues with female members of the Afghan Uniformed Police and Afghan Border Patrol at the ABP compound in Jalalabad, Afghanistan, Jan. 18th, 2013. (U.S. Army photo by Sgt. 1st Class John D. Brown, TF 1-101 Public Affairs) «Read the rest of this article» Sections: News | 0 comments
Suzanne Simpson: One Woman’s Heart
«Read the rest of this article» Sections: News | 0 comments
LBL Hosting 3rd Annual Sustainable Tourism Business Seminar
Early registration is $10.00 per person through February 15th and includes lunch. Registration after the 15th is $15.00. «Read the rest of this article» Sections: Events | 0 comments
IRS says check your Eligibility for the Earned Income Tax Credit
Yet the IRS estimates that one out of five eligible taxpayers fails to claim their EITC each year. The IRS wants everyone who is eligible for the credit to get the credit that they’ve earned.
Sections: News | 0 comments
NASA’s Solar Dynamics Observatory gives insight into how Coronal Mass Ejections formWritten by Karen C. Fox
Something interesting did happen, however. Magnetic field lines in this area of the sun’s atmosphere, the corona, began to twist and kink, generating the hottest solar material – a charged gas called plasma – to trace out the newly-formed slinky shape. ![]() On July 19th, 2012, SDO captured images of a solar flare in numerous wavelengths. The 131 Angstrom wavelength, shown here in the middle and colorized in teal, portrays particularly hot material on the sun, at 10 million Kelvin, which is why the incredibly hot flare shows up best in that wavelength. The 131 wavelength was also able to show kinked magnetic fields known as a flux rope that lay at the heart of a coronal mass ejection (CME), which also erupted at the same time as the flare. (Credit: NASA/Goddard Space Flight Center) «Read the rest of this article» Sections: Technology | 0 comments
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