Observation & Instrumental seminar
Purpose
To learn current instrumentation in solar observation, their aims,
and method of data analysis, and to think future directions of
solar observations and his/her own research from a long_term point of view.
これまでの観測装置やその目的、解析手法を知ることにより、
現在どのような観測がされているのか、また今後どのような観測が必要となるのか、
長期的な目で見たときの太陽観測の方向性を考えると同時に、
自分の研究内容の理解をふかめよう、という趣旨のゼミです。
In 2017FY, we will mainly practice
・ MULTI (non LTE radiative transfer) to interpret observation data
・ ZEMAX to design optics
Next seminar
＊ Nobember 28th, 2017 15:00-17:00
_ Presentations in TENMON GAKKAI
_ Optics (Denis & Anan)
＊
Guidelines
|
Course Year |
|
|
Term |
A year |
|
Day |
Irregular |
|
Location |
Hida
observatory & #4 Build. Of faculty of Science, Kyoto University |
|
Credits |
0 |
|
Restriction |
No |
|
Lecture Forms |
Seminar |
|
Language |
English |
|
Instructor |
K. Ichimoto,
A. Asai, S. Ueno, S. Nagata |
Textbook
FY
2017: “Radiative transfer in stellar atospheres”
R.J, Rutten
Carlsson
1986, UppOR, 33, C in multi.zip
“Stellat atmospheres” Mihalas 1978
“Radiative
processes in Astorphysics” Rybicki, & Lightman 1979
FY
2016: “Solar Prominences”2015,
Springer, Vial, Jean-Claude, Engvold, Oddbjorn (Eds.)
＊
Previous presentations
|
Date |
Title |
Presenter |
File |
|
2017/11/28 |
The ASJ 2018 spring meeting FMT |
Denis |
|
|
2017/10/27 |
Aberrations Telescopes |
Anan Denis |
|
|
2017/10/12 |
Basic of optics Telescopes |
Anan Denis |
|
|
2017/10/06 |
Basics of optics |
Anan |
|
|
2017/08/25 |
PROM7 |
Okada |
|
|
2017/07/28 |
Non LTE radiative transfer and codes |
Kou Anan |
|
|
2017/07/07 |
Discussion of objectives in
this seminar |
|
|
|
2017/06/19 |
Introduction of ZEMAX |
Nagata |
|
|
|
How to use Zemax from outside of key server’s
network |
|
|
|
2017/06/07 |
Discussion of presentation in ASJ meeting |
|
|
|
2017/05/26 |
Introduction of this seminar
& MULTI |
Anan |
|
|
2017/03/06 |
12. MHD equilibrium and triggers for prominence
eruption |
Hirose |
|
|
2017/02/02 |
Practice for presentation of
Master thesis |
Kou |
|
|
2017/01/20 |
12. MHD equilibrium and triggers for prominence
eruption |
Hirose |
|
|
2016/11/15 |
|
Nagata |
|
|
2016/11/01 |
5. Radiative Transfer in Solar Prominences |
Kou Hubeny & Mihalas (2014), Griem
(1997) Rutten Griem, 1997 |
|
|
2016/07/20 |
Discussion on event list Plasma structure and dynamics |
Sakaue |
|
|
2016/07/13 |
TF40 of SMART/SDDI |
Otsuji |
|
|
2016/07/06 |
2. Description and Classification of Prominences Discussion of science objectives using data obtained by
SMART/SDDI |
Ninomiya Asai, Ishii |
|
|
2016/06/21 |
Description
and Classification of Prominences |
Ninoyama |
|
|
2016/6/15 |
Calibration data for
SMART/SDDI |
Denis |
|
|
2016/5/11 |
Introduction & discussion about this seminar |
|
|
|
2016/1/25 |
ALMA seminar |
Shimojo |
|
|
2016/1/19 |
For ALMA seminar |
Asai, Anan |
|
|
2016/1/5 |
Observations of the Sun at millimeter and submilimeter wavelengths (Wedemeyer
et al. SSRv) DST spectro-polarimeter |
Sakaue Anan |
|
|
2015/12/28 |
DST
Spectro-polarimeter |
Anan |
|
|
2015/12/21 |
The formation of millimeter radiation in the Sun |
Asai |
|
|
2015/12/11 |
DST
spectro-polarimeter Solar
Prominences |
Anan |
|
|
2015/11/30 |
DST spectro-polarimeter |
Anan |
|
|
2015/11/17 |
For
submission of ALMA proposal DST
spectro-polarimeter |
Anan |
|
|
2015/10/30 |
For submission of ALMA proposal |
Anan |
|
|
2015/10/19 |
IRIS
paper (Mg II k&h line formation) |
Tei |
|
|
2015/9/28 |
IRIS paper (Mg II k&h
line formation) |
Tei |
|
|
2015/9/28 |
IRIS
paper (Mg II k&h line formation) |
Tei |
|
|
2015/8/26 |
IRIS paper (Mg II k&h
line formation) |
Tei |
|
|
2015/8/10 |
Review of spicule observation |
Anan |
|
|
2015/7/6 |
シリーズ現代の天文学 光赤外 Sec.3 Optics |
Hirose |
|
|
2014/10/24 |
シリーズ現代の天文学 光赤外Sec.3 Optics |
Hirose |
|
|
2014/10/24 |
シリーズ現代の天文学 光赤外Sec.3 Optics |
Hirose |
|
|
2014/10/16 |
シリーズ現代の天文学 光赤外Sec.3 Optics |
Hirose |
|
|
2014/09/03 |
研究紹介及び学会で発表する内容の紹介 |
|
|
|
2014/08/04 |
Introduction of the seminar |
|
|
|
2014/07/16 |
“High-speed
imaging” |
Ichimoto |
|
|
“High-speed imaging” High-speed cameras |
Anan |
||
|
2014/07/08 |
“High-speed
imaging” Change of
brightness due to seeing |
Kawate |
|
|
“High-speed
imaging” |
Ichimoto |
|
|
|
2014/07/03 |
“High-speed
imaging” Physics of short brightness variation |
Isobe |
|
|
2014/05/15 |
Analysis |
|
|
|
2013/12/10 2013/11/26 |
Hinode SOT |
Ichimoto |
|
|
※SOT polarimetric calibration |
Ichimoto |
||
|
※SOT SP sp_prep |
Ichimoto |
||
|
※Optical performance of SOT (Suematsu-san)
|
Ichimoto |
||
|
2013/10/29 |
Observation in visible and near infrared |
Oi |
|
|
※The farthest astronomical object |
Asai |
||
|
2013/10/15 2013/10/07 |
Ground-based telescope in the world and DST |
Ueno |
|
|
※Observation at Mt. Wilson |
Watanabe |
||
|
※Optical ray-path of SacPeak
DST |
Oi |
||
|
2013/09/26 |
Weak
field approximation |
Watanabe |
|
|
2013/09/06 |
Overview of the adaptive optics |
Yamaguchi |
|
|
2013/08/21 |
UV
spectroscopy |
Kawate |
|
|
※SDO/EVE |
Asai |
||
|
2013/08/01 |
Basics
of optics |
Sano |
|
|
※Aberration |
Watanabe |
||
|
2013/07/26 |
Basics
of optics |
Sano |
|
|
※Gaussian
optics |
Kitai |
||
|
2013/07/19 |
Fabry-Perot filter in the world |
Nagata |
Upcoming
[nonLTE]
・
Dependence of transition rates on physical quantities or
spectral lines
・ Exercise using statistical equilibrium with Kou, IAS,
MULTI, & RH (will be proposed by Kou)
・ Calculation of fine structure of neutral hydrogen in
MULTI (Anan)
・
[Optics]
1.
Design of DST (Anan)
Why we choose Newton-Gregorian telescope as DST?
Check the scale in paraxial approximation
How is aberrations
Performance (Diffraction limit, size of image, brightness
of image, F number, PSF, MTF, and so on)
2.
Design of FMT (Denis)
3.
All functions of Zemax (Denis & Anan)
4.
Optical performance of SMART/T2 in 10830_, design
corrector to improve the performance
[Prominences]
・MHD equilibrium and triggers for prominence eruption
(Hirose-san)
継続課題
Event
list of observation at Hida