PPT-Coronal Seismology Based on EUV Waves

P F Chen China Moreton wave P F Chen ISSIBeijing Moreton et al 1961 Moreton waves are associated with big flares Propagation velocity 1 000 kms Propagation distance . Nuclear-Test-Ban Treaty Monitoring . Steven J. Gibbons. Workshop on Arrays in Global Seismology,. Raleigh, North Carolina, May 15-16 2013. .. Rethinking Array Seismology in Nuclear-Test-Ban Treaty Monitoring . Claire Cramer. IACHEC Meeting. 25 March, 2013. Who am I and why am I here?. Outline . Introduction/Background Material. Flux/Detector Response . Calibrations. Spectroscopy and Detector Development. What is NIST?. in Solar Disk Images . (and how to compare to models). Working Group Report. Nick Arge. .  . Rachel Hock. .  . Carl Henney. Definitions . (from our invited speakers). Coronal holes. : observable used as. ● What is Seismology?. ● What are Seismic Waves?: Types of Seismic waves. ● Where do Earthquakes Happen?. ● Why do Earthquakes Happen?. ● How is the Epicenter of an Earthquake Located?. ● How are Earthquakes Magnitude Measured?. Abstract. We observed a filament eruption, whose shape is like a dandelion, associated with the solar flare that occurred on 2011 February 16 at the active region NOAA 11158. The H. a. . full disk images of the flare were taken by FMT. . By: Valentina, Laurel, Miriam, Crystal, Isaiah, Adam, Landon, and Emma.. What Does a Seismologist . S. tudy?. A seismologist studies earthquakes, faults, and seismology. Seismologist also use a Richter Scale to measure earthquakes. . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. team meeting: . january. 2010. T. b. LIMB MODEL, RECENT LAB ANALYSIS & UVIS OBSERVATIONS . SUBMITTED FUV LIMB PAPER (T. Dayglow. , Nightglow & Eclipse . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. team meeting: . January 2011. Titan . dayglow. . Motivation. . The Corona is a Magnetically Dominated System. Coronal Magnetism is the Source of Space Weather. Coronal Mass Ejections. Energetic Particle Acceleration . Coronal Heating. Solar Wind Acceleration. outline. Lithography. Introduction to EUVL. Basic concepts. Why do we need EUVL?. EUVL Process. Basic technology for EUV. EUV masks. All Reflective Optics. Advantages. Disadvantages. Conclusion. WHAT IS LITHOGRAPHY . JOSEPH AJELLO. JPL. MICHAEL STEVENS. NRL. ROBERT WEST. JPL. JACQUES GUSTIN. LPAP. GREG HOLSCLAW. CU. TODD BRADLEY. UCF. Team meeting: Jan20112. TITAN PROTON PLASMA (0.1 keV-4 . MeV. ) & SOLAR XUV GENERATES . DR. AKANKSHA SINGH. SECTIONS OF THE BRAIN. TRANSVERSE SECTION. SAGGITAL SECTION . CORONAL SECTION. THESE SECTIONS ARE VERY IMP FOR VIVA POINT OF VIEW…….. IDENTIFY INTERNAL CAPSULE. VENTRICLES. CORPUS STRIATUM. UV . Hanle. Effect . Coronal Magnetic Field & Plasma Dynamics . N.-E. . R. aouafi . Coronal Zeeman effect. Limitations. . Few . applications because of the weakness. of . the coronal magnetic field and of coronal signal. Energy is moving, not water. orbital motion. energy is transferred via circular motions. water (and gull) return to original position. the wave form moves forward. Motion decreases with depth. At. a depth of ½ of the wavelength, the motion is not significant..