The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1

Lauri Alha; Juhani Huovelin; Thomas Hackman; H Andersson; C. J Howe; Eero Esko; Mikko Väänänen

doi:10.1016/j.nima.2008.08.138

The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1

Lauri Alha, Juhani Huovelin, Thomas Hackman, H Andersson, C. J Howe, Eero Esko, Mikko Väänänen

Tutkimustuotos: Artikkelijulkaisu › Artikkeli › Tieteellinen › vertaisarvioitu

Abstrakti

The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESA's SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband solar flare spectra including highly ionized Fe-lines are also presented. (C) 2008 Elsevier B.V. All rights reserved.

Alkuperäiskieli	englanti
Lehti	Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment
Vuosikerta	596
Numero	3
Sivut	317-326
Sivumäärä	10
ISSN	0168-9002
DOI - pysyväislinkit	https://doi.org/10.1016/j.nima.2008.08.138
Tila	Julkaistu - 2008
OKM-julkaisutyyppi	A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä, vertaisarvioitu

Tieteenalat

115 Avaruustieteet ja tähtitiede

Pääsy asiakirjaan

10.1016/j.nima.2008.08.138

Siteeraa tätä

@article{4c524f6e3acf41bdbee1029ff34cee4e,

title = "The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1",

abstract = "The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESA's SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband solar flare spectra including highly ionized Fe-lines are also presented. (C) 2008 Elsevier B.V. All rights reserved.",

keywords = "115 Astronomy, Space science",

author = "Lauri Alha and Juhani Huovelin and Thomas Hackman and H Andersson and Howe, {C. J} and Eero Esko and Mikko V{\"a}{\"a}n{\"a}nen",

year = "2008",

doi = "10.1016/j.nima.2008.08.138",

language = "English",

volume = "596",

pages = "317--326",

journal = "Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier Scientific Publ. Co",

number = "3",

}

Alha, L, Huovelin, J , Hackman, T, Andersson, H, Howe, CJ, Esko, E & Väänänen, M 2008, 'The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1', Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment, Vuosikerta 596, Nro 3, Sivut 317-326. https://doi.org/10.1016/j.nima.2008.08.138

The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1. / Alha, Lauri; Huovelin, Juhani ; Hackman, Thomas et al.

julkaisussa: Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment, Vuosikerta 596, Nro 3, 2008, s. 317-326.

Tutkimustuotos: Artikkelijulkaisu › Artikkeli › Tieteellinen › vertaisarvioitu

TY - JOUR

T1 - The in-flight performance of the X-ray Solar Monitor (XS0M) on-board SMART-1

AU - Alha, Lauri

AU - Huovelin, Juhani

AU - Hackman, Thomas

AU - Andersson, H

AU - Howe, C. J

AU - Esko, Eero

AU - Väänänen, Mikko

PY - 2008

Y1 - 2008

N2 - The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESA's SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband solar flare spectra including highly ionized Fe-lines are also presented. (C) 2008 Elsevier B.V. All rights reserved.

AB - The operation, performance, and in-flight calibrations of the X-ray Solar Monitor (XSM) on-board ESA's SMART-1 mission to the Moon are presented. The basic method of deriving the response and effective area of the XSM is described. The evolution of the energy resolution as a function of time is studied, and sample data of high quality broadband solar flare spectra including highly ionized Fe-lines are also presented. (C) 2008 Elsevier B.V. All rights reserved.

KW - 115 Astronomy, Space science

U2 - 10.1016/j.nima.2008.08.138

DO - 10.1016/j.nima.2008.08.138

M3 - Article

VL - 596

SP - 317

EP - 326

JO - Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment

JF - Nuclear Instruments & Methods in Physics Research. Section A: Accelerators, Spectrometers, Detectors, and Associated Equipment

SN - 0168-9002

IS - 3

ER -