HR: 1340h
AN: SH53A-1050 [Abstracts]
TI: Cross calibration of soft X-ray telescopes between Hinode/XRT and GOES13/SXI
AU: * Narukage, N
EM: narukage@solar.isas.jaxa.jp
AF: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
(ISAS/JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
AU: Sakao, T
EM: Sakao.Taro@isas.jaxa.jp
AF: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
(ISAS/JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
AU: Kano, R
EM: ryouhei.kano@nao.ac.jp
AF: National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588,
Japan
AU: Shimojo, M
EM: shimojo@nro.nao.ac.jp
AF: National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588,
Japan
AU: Cirtain, J
EM: jcirtain@head.cfa.harvard.edu
AF: Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, United
States
AU: DeLuca, E
EM: edeluca@cfa.harvard.edu
AF: Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, United
States
AU: Nitta, N
EM: nitta@lmsal.com
AF: Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, CA
94304, United States
AU: Lemen, J
EM: lemen@lmsal.com
AF: Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, CA
94304, United States
AB:
The X-Ray Telescope (XRT) aboard Hinode satellite is a grazing incidence telescope to
observe all the coronal features with a wide temperature range from less than 1MK to
more than 10MK. And the XRT has 9 X-ray analysis filters which are optimized to
observed the almost whole coronal plasma and to derived the coronal temperature distribution.
Meanwhile, the GOES13 satellite carries a Solar X-ray Imager (SXI) to monitor the solar X-rays.
The SXI is also a grazing incidence telescope and has 7 X-ray filters.
The XRT and SXI are similar telescopes to observe the dynamic solar corona.
On 24 Nov 2006, the XRT and SXI-team performed the simultaneous observation
for the cross calibration between XRT and SXI. In this study, we analyzed this data set
and checked the actual characteristics of each X-ray analysis filter.
DE: 7509 Corona
DE: 7554 X-rays, gamma rays, and neutrinos
DE: 7594 Instruments and techniques
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Fall Meeting