東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Hard x-ray imaging of solar flares

Piana, Michele.

Linked to FindBook

Google Book

Amazon

博客來

Hard x-ray imaging of solar flares

Record Type:	Electronic resources : Monograph/item
Title/Author:	Hard x-ray imaging of solar flares/ by Michele Piana ... [et al.].
other author:	Piana, Michele.
Published:	Cham :Springer International Publishing : : 2022.,
Description:	xviii, 164 p. :ill., digital ;24 cm.
[NT 15003449]:	1. Hard X-ray Emission in Solar Flares -- 2. X-Ray Imaging Methods -- 3. RHESSI and STIX -- 4. Image Reconstruction Methods -- 5. Count-based Imaging Methods -- 6. Visibility-based Imaging Methods -- 7. Application to Solar Flares -- 8. Future Possibilities.
Contained By:	Springer Nature eBook
Subject:	Solar flares. -
Online resource:	https://doi.org/10.1007/978-3-030-87277-9
ISBN:	9783030872779

Hard x-ray imaging of solar flares
Hard x-ray imaging of solar flares[electronic resource] /by Michele Piana ... [et al.]. - Cham :Springer International Publishing :2022. - xviii, 164 p. :ill., digital ;24 cm.

1. Hard X-ray Emission in Solar Flares -- 2. X-Ray Imaging Methods -- 3. RHESSI and STIX -- 4. Image Reconstruction Methods -- 5. Count-based Imaging Methods -- 6. Visibility-based Imaging Methods -- 7. Application to Solar Flares -- 8. Future Possibilities.

The idea for this text emerged over several years as the authors participated in research projects related to analysis of data from NASA's RHESSI Small Explorer mission. The data produced over the operational lifetime of this mission inspired many investigations related to a specific science question: the when, where, and how of electron acceleration during solar flares in the stressed magnetic environment of the active Sun. A vital key to unlocking this science problem is the ability to produce high-quality images of hard X-rays produced by bremsstrahlung radiation from electrons accelerated during a solar flare. The only practical way to do this within the technological and budgetary limitations of the RHESSI era was to opt for indirect modalities in which imaging information is encoded as a set of two-dimensional spatial Fourier components. Radio astronomers had employed Fourier imaging for many years. However, differently than for radio astronomy, X-ray images produced by RHESSI had to be constructed from a very limited number of sparsely distributed and very noisy Fourier components. Further, Fourier imaging is hardly intuitive, and extensive validation of the methods was necessary to ensure that they produced images with sufficient accuracy and fidelity for scientific applications. This book summarizes the results of this development of imaging techniques specifically designed for this form of data. It covers a set of published works that span over two decades, during which various imaging methods were introduced, validated, and applied to observations. Also considering that a new Fourier-based telescope, STIX, is now entering its nominal phase on-board the ESA Solar Orbiter, it became more and more apparent to the authors that it would be a good idea to put together a compendium of these imaging methods and their applications. Hence the book you are now reading.

ISBN: 9783030872779

Standard No.: 10.1007/978-3-030-87277-9doiSubjects--Topical Terms:

2149191
Solar flares.

LC Class. No.: QB526.F6

Dewey Class. No.: 523.75

Hard x-ray imaging of solar flares
LDR:03144nmm a2200337 a 4500 001 2296917
003 DE-He213
005 20211221111819.0
006 m d
007 cr nn 008maaau
008 230324s2022 sz s 0 eng d
020 $a 9783030872779 $q (electronic bk.)
020 $a 9783030872762 $q (paper)
024 7 $a 10.1007/978-3-030-87277-9 $2 doi
035 $a 978-3-030-87277-9
040 $a GP $c GP
041 0 $a eng
050 4 $a QB526.F6
072 7 $a UYT $2 bicssc
072 7 $a COM012000 $2 bisacsh
072 7 $a UYT $2 thema
072 7 $a UYQV $2 thema
082 0 4 $a 523.75 $2 23
090 $a QB526.F6 $b H258 2022
245 0 0 $a Hard x-ray imaging of solar flares $h [electronic resource] / $c by Michele Piana ... [et al.].
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2022.
300 $a xviii, 164 p. : $b ill., digital ; $c 24 cm.
505 0 $a 1. Hard X-ray Emission in Solar Flares -- 2. X-Ray Imaging Methods -- 3. RHESSI and STIX -- 4. Image Reconstruction Methods -- 5. Count-based Imaging Methods -- 6. Visibility-based Imaging Methods -- 7. Application to Solar Flares -- 8. Future Possibilities.
520 $a The idea for this text emerged over several years as the authors participated in research projects related to analysis of data from NASA's RHESSI Small Explorer mission. The data produced over the operational lifetime of this mission inspired many investigations related to a specific science question: the when, where, and how of electron acceleration during solar flares in the stressed magnetic environment of the active Sun. A vital key to unlocking this science problem is the ability to produce high-quality images of hard X-rays produced by bremsstrahlung radiation from electrons accelerated during a solar flare. The only practical way to do this within the technological and budgetary limitations of the RHESSI era was to opt for indirect modalities in which imaging information is encoded as a set of two-dimensional spatial Fourier components. Radio astronomers had employed Fourier imaging for many years. However, differently than for radio astronomy, X-ray images produced by RHESSI had to be constructed from a very limited number of sparsely distributed and very noisy Fourier components. Further, Fourier imaging is hardly intuitive, and extensive validation of the methods was necessary to ensure that they produced images with sufficient accuracy and fidelity for scientific applications. This book summarizes the results of this development of imaging techniques specifically designed for this form of data. It covers a set of published works that span over two decades, during which various imaging methods were introduced, validated, and applied to observations. Also considering that a new Fourier-based telescope, STIX, is now entering its nominal phase on-board the ESA Solar Orbiter, it became more and more apparent to the authors that it would be a good idea to put together a compendium of these imaging methods and their applications. Hence the book you are now reading.
650 0 $a Solar flares. $3 2149191
650 0 $a X-ray astronomy. $3 539069
650 1 4 $a Image Processing and Computer Vision. $3 891070
650 2 4 $a Optics, Lasers, Photonics, Optical Devices. $3 2209850
650 2 4 $a Theoretical, Mathematical and Computational Physics. $3 1066859
700 1 $a Piana, Michele. $3 3591973
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer Nature eBook
856 4 0 $u https://doi.org/10.1007/978-3-030-87277-9
950 $a Computer Science (SpringerNature-11645)