The imaging magnetograph experiment for the SUNRISE balloon Antarctica project

被引：25

作者：

Pillet, VM ^{[1
]}

Bonet, JA ^{[1
]}

Collados, M ^{[1
]}

Jochum, L ^{[1
]}

Mathew, S ^{[1
]}

Trujillo, JLM ^{[1
]}

Cobo, BR ^{[1
]}

Iniesta, JCD ^{[1
]}

Jiménez, ACL ^{[1
]}

Lorenzo, J ^{[1
]}

Herranz, M ^{[1
]}

Jerónimo, JM ^{[1
]}

Mellado, P ^{[1
]}

Morales, R ^{[1
]}

Rodríguez, J ^{[1
]}

Alvarez-Herrero, A ^{[1
]}

Belenguer, T ^{[1
]}

Heredero, RL ^{[1
]}

Menéndez, M ^{[1
]}

Ramos, G ^{[1
]}

Reina, M ^{[1
]}

Pastor, C ^{[1
]}

Sánchez, A ^{[1
]}

Villanueva, J ^{[1
]}

Domingo, V ^{[1
]}

Gasent, JL ^{[1
]}

Rodríguez, P ^{[1
]}

机构：

[1] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain

来源：

OPTICAL, INFRARED, AND MILLIMETER SPACE TELESCOPES, PTS 1-3 | 2004年 / 5487卷

关键词：

polarimetry; Fabry-Perot etalons; magnetographs; balloon home telescopes; sun;

D O I：

10.1117/12.549020

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The SUNRISE balloon project is a high-resolution mission to study solar magnetic fields able to resolve the critical scale of 100 kin in the solar photosphere, or about one photon mean free path. The Imaging Magnetograph eXperiment (IMaX) is one of the three instruments that will fly in the balloon and will receive light from the 1m aperture telescope of the mission. IMaX should take advantage of the 15 days of uninterrupted solar observations and the exceptional resolution to help clarifying our understanding of the small-scale magnetic concentrations that pervade the solar surface. For this, IMaX should act as a diffraction limited imager able to carry out spectroscopic analysis with resolutions in the 50.000-100.000 range and capable to perform polarization measurements. The solutions adopted by the project to achieve all these three demanding goals are explained in this article. They include the use of Liquid Crystal Variable Retarders for the polarization modulation, one LiNbO3 etalon in double pass and two modem CCD detectors that allow for the application of phase diversity techniques by slightly changing the focus of one of the CCDs.

引用

页码：1152 / 1164

页数：13

共 50 条

[11] Sunrise imaging
Imaging Magazine, 1994, 3 (12):
[12] A BALLOON MEASUREMENT OF OZONE NEAR SUNRISE
RANDHAWA, JS
BULLETIN OF THE AMERICAN METEOROLOGICAL SOCIETY, 1970, 51 (04) : 382 - &
[13] Unemployment and Addiction: The SUNRISE Project
Scherbaum, N.
Specka, M.
Kaspar, C.
Mikoteit, T.
Lieb, B.
GESUNDHEITSWESEN, 2018, 80 (01) : 73 - 78
[14] Stokes profile reconstruction with the imaging vector magnetograph
Leka, KD
Mickey, DL
Labonte, BJ
SOLAR POLARIZATION, 1999, 243 : 305 - 312
[15] GRAINE project and first results on 2018 balloon-borne experiment
Takahashi, Satoru
36TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2019, 2021,
[16] SUNRISE Project: Porto University Testbed
Martins, Ricardo
de Sousa, Joao Borges
Caldas, Renato
Petrioli, Chiara
Potter, John
2014 UNDERWATER COMMUNICATIONS AND NETWORKING (UCOMMS), 2014,
[17] Preflight calibration of the Imaging Magnetograph eXperiment polarization modulation package based on liquid-crystal variable retarders
Uribe-Patarroyo, Nestor
Alvarez-Herrero, Alberto
Martinez Pillet, Valentin
APPLIED OPTICS, 2012, 51 (21) : 4954 - 4970
[18] The protoMIRAX hard X-ray imaging balloon experiment
Braga, Joao
D'Amico, Flavio
Avila, Manuel A. C.
Penacchioni, Ana V.
Rodrigo Sacahui, J.
de Santiago, Valdivino A., Jr.
Mattiello-Francisco, Fatima
Strauss, Cesar
Fialho, Marcio A. A.
ASTRONOMY & ASTROPHYSICS, 2015, 580
[19] Retrieval of solar magnetic fields from high-spatial resolution filtergraph data: the Imaging Magnetograph eXperiment (IMaX)
Orozco Suarez, D.
Bellot Rubio, L. R.
Martinez Pillet, V.
Bonet, J. A.
Dominguez, S. Vargas
del Toro Iniesta, J. C.
ASTRONOMY & ASTROPHYSICS, 2010, 522
[20] A MOF-based full vector imaging magnetograph
Cacciani, A
Comari, M
Furlani, S
Hanslmeier, A
Messerotti, M
Moretti, PF
Pettauer, T
Veronig, A
SECOND ADVANCES IN SOLAR PHYSICS EUROCONFERENCE: THREE-DIMENSIONAL STRUCTURE OF SOLAR ACTIVE REGIONS, 1998, 155 : 265 - 269

← 1 2 3 4 5 →