'Ray flares' presentation slideshows

Part 2: Stars

Part 2: Stars. Monday, February 10 Reading: Chapter 6 [Ed. 9, 10, 11, 12] The nature of light: How we use spectra to measure the properties of stars Wednesday, February 12 Reading: Chapters 8, 9.1, 9.5 or Orion Nebula Stars: distance, luminosity, mass, composition. Star formation.

554 views • 41 slides

Joint BAT and XRT Data Analysis for Gamma-Ray Bursts

Joint BAT and XRT Data Analysis for Gamma-Ray Bursts. Enwei Liang Co-authors: Youdong Hu, Fangkun Peng, Bing Zhang, Xiang-Yu Wang, Xuefeng Wu GXU-NAOC Center for Astrophysics & Space Sciences IHEP, 2014- 03-22. Outlines.

449 views • 35 slides

Chandra Observations of Sgr A*

Chandra Observations of Sgr A*. Frederick Baganoff. Massachusetts Institute of Technology. Chandra Galactic Center Deep Field. 17 x 17 arcmin 40 x 40 pc 590 ks. Red 2-3.7 keV Green 3.7-4.5 keV Blue 4.5-8 keV. Chandra Galactic Center Deep Field. 8.4 x 8.4 arcminutes.

497 views • 29 slides

Blazars: VLBA and GLAST

Blazars: VLBA and GLAST. Glenn Piner Whittier College. Overview. Review of EGRET and current TeV observations. VLBA observations of EGRET and TeV blazars. Future ?-ray telescopes (AGILE, GLAST, VERITAS) and predictions of source detections. VLBA Observations of GLAST sources.

366 views • 25 slides

Long term X-ray and GeV flares in GRB light curves

303 views • 20 slides

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682. Space Sciences Directorate Monthly Report Monday, 25 March 2002. The Reuven Ramaty High Energy Solar Spectroscopic Image - RHESSI. Solar Flares.

312 views • 20 slides

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682

First RHESSI Results Brian R. Dennis RHESSI Mission Scientist Code 682. Space Sciences Directorate Monthly Report Monday, 25 March 2002. The Reuven Ramaty High Energy Solar Spectroscopic Image - RHESSI. Solar Flares.

211 views • 20 slides

The Milky Way II

289 views • 19 slides

DELAY TIMES BETWEEN GEOEFFECTIVE SOLAR DISTURBANCES AND GEOMAGNETIC INDICES

DELAY TIMES BETWEEN GEOEFFECTIVE SOLAR DISTURBANCES AND GEOMAGNETIC INDICES. Y. D. PARK 1 , Y. -J. MOON 1 , I. S. KIM 2 , H. S. YUN 3. 1.Korea Astronomy Observatory, Daejeon, KOREA 2. Sternberg State Astronomical Institute, Moscow Univ. RUSSIA 3. Seoul National Univ. Seoul, KOREA.

231 views • 14 slides

Alessandra Galli 1,2,3

137 views • 13 slides

GOES Space Weather Complement

GOES I-M SXI SEM EPS HEPAD XRS Magnetometers GOES N-O-P SXI SEM EPS Magnetometers XRS & EUVS. GOES R SIS SXI XRS EUVS SEISS MPS Low High SGPS EHIS Magnetometer SCOR (P3I). GOES Space Weather Complement. Solar Imaging Suite (SIS) - 1. Sun-staring instruments.

176 views • 6 slides

M Tavani et al. Nature 000 , 1-4 (2009) doi:10.1038/nature08578

Hard-X-ray flux from Cyg X-3 and ? -ray flares. M Tavani et al. Nature 000 , 1-4 (2009) doi:10.1038/nature08578.

117 views • 1 slides