Roles of Ground-based Solar Observations of Hida Observatory toward the Solar-C Era

被引：0

作者：

Ueno, S. ^{[1
]}

Shibata, K. ^{[1
]}

Ichimoto, K. ^{[1
]}

Nagata, S. ^{[1
]}

Dorotovic, I. ^{[2
]}

Shahamatnia, E. ^{[2
]}

Ribeiro, R. A. ^{[2
]}

Fonseca, J. M. ^{[2
]}

机构：

[1] Kyoto Univ, Kwasan & Hida Observ, Kyoto 6068501, Japan

[2] UNINOVA CTS, Computat Intelligence Res Grp CA3, Campus FCT UNL Quinta Torre, P-2829516 Monte De Caparica, Caparica, Portugal

来源：

GROUND-BASED SOLAR OBSERVATIONS IN THE SPACE INSTRUMENTATION ERA | 2016年 / 504卷

关键词：

JETS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

For the realization of the Solar-C satellite, discussions about scientific themes and preliminary observations are internationally carried out now. At Hida Observatory of Kyoto University, we will play the following roles toward the Solar-C era by utilizing the Domeless Solar Telescope (DST) and the international solar chromospherirc full-disk observation network (CHAIN project) that includes the Solar Magnetic Activity Research Telescope (SMART) with international collaborations, for example, such as the development of image-analysis software by UNINOVA (Portugal) and so on.

引用

页码：309 / 312

页数：4

共 50 条

[21] Mass determination of small solar system bodies with ground-based observations
Aslan, Z.
Gumerov, R.
Hudkova, L.
Ivantsov, A.
Khamitov, I.
Pinigin, G.
SOLAR AND STELLAR PHYSICS THROUGH ECLIPSES, 2007, 370 : 52 - +
[22] GROUND-BASED NEAR-INFRARED OBSERVATIONS OF GLOBAL SOLAR OSCILLATIONS
DIDKOVSKY, LV
KOTOV, VA
INFRARED SOLAR PHYSICS, 1994, (154): : 277 - 282
[23] New ground-based solar instrumentation
Mein, P
SOLAR AND HELIOSPHERIC PLASMA PHYSICS, 1997, 489 : 241 - 260
[24] Sky Brightness Evaluation at Concordia Station, Dome C, Antarctica, for Ground-Based Observations of the Solar Corona
Liberatore, Alessandro
Capobianco, Gerardo
Fineschi, Silvano
Massone, Giuseppe
Zangrilli, Luca
Susino, Roberto
Nicolini, Gianalfredo
SOLAR PHYSICS, 2022, 297 (03)
[25] Sky Brightness Evaluation at Concordia Station, Dome C, Antarctica, for Ground-Based Observations of the Solar Corona
Alessandro Liberatore
Gerardo Capobianco
Silvano Fineschi
Giuseppe Massone
Luca Zangrilli
Roberto Susino
Gianalfredo Nicolini
Solar Physics, 2022, 297
[26] Estimation of the Solar Energy Potential in Greece Using Satellite and Ground-Based Observations
Kosmopoulos, P. G.
Kazadzis, S.
Taylor, M.
Bais, Alkiviadis F.
Lagouvardos, K.
Kotroni, V.
Keramitsoglou, I.
Kiranoudis, C.
PERSPECTIVES ON ATMOSPHERIC SCIENCES, 2017, : 1149 - 1156
[27] Recent observations of the solar corona with a new ground-based coronagraph in Argentina (MICA)
Stenborg, G
Schwenn, R
Srivastava, N
Inhester, B
Podlipnik, B
Rovira, M
Francile, C
SOLAR WIND NINE, 1999, 471 : 561 - 564
[28] New observational facts about solar flares from ground-based observations
Sakurai, T.
Hiei, E.
Advances in Space Research, 17 (4-5):
[29] The atmospheric conditions of Maidanak observatory in Uzbekistan for the ground-based observations
Ilyasov, Sabit
Tillayev, Yusufjon
INTERNATIONAL CONFERENCE ON SPACE INFORMATION TECHNOLOGY 2009, 2010, 7651
[30] Ground-based observations of ozone at Athens, Greece during the solar eclipse of 1999
Tzanis, C
INTERNATIONAL JOURNAL OF REMOTE SENSING, 2005, 26 (16) : 3585 - 3596

← 1 2 3 4 5 →