ATTENTION: All class announcements, assignments, and handouts will be through Google Classroom.Please feel free to contact me at any time!I am here from 8:00-3:05 daily. If you need additional assistance with your school work, please contact me to schedule an appropriate time for us to work together.Email is the BEST WAY to reach me: email@example.comCLICK HERE FOR EARTHQUAKES THAT OCCUR IN REAL TIME! http://earthquaketrack.com/Name: Bamber-Wichtendahl, LisaPhone: (908) 852-8554 ext. 826
Where is the ISS? http://www.isstracker.comWatch views from the ISS 24/7 http://www.ustream.tv/channel/iss-hdev-payload
PICTURE OF THE DAY
Polar oppositesThis image reveals the magnetic field in the sun’s corona, derived from data provided through the National Solar Observatory’s Global Oscillation Network Group. Magnetic field lines that are closed on the sun are shown in blue, while those that are open are shown in red and green. The sun, like the Earth, has two poles, similar to a bar magnet. On the sun, magnetic fields wrap themselves up over approximately a five- to six-year period. They then spend the next five years winding down, relaxing and producing solar flares and coronal mass ejections to release excess energy.
Visit Website | Image credit: National Solar Observatory/Association of Universities for Research in Astronomy/NSF