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The Era of Multi-Messenge
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eBay item number:386921116866
Item specifics
- Condition
- ISBN-13
- 9781009352888
- Type
- NA
- Publication Name
- NA
- ISBN
- 9781009352888
- Book Title
- Era of Multi-Messenger Solar Physics (Iau S372)
- Book Series
- Proceedings of the International Astronomical Union Symposia and Colloquia Ser.
- Publisher
- Cambridge University Press
- Item Length
- 10 in
- Publication Year
- 2023
- Format
- Hardcover
- Language
- English
- Illustrator
- Yes
- Item Height
- 0.5 in
- Genre
- Science
- Topic
- Physics / Astrophysics, Astronomy
- Item Width
- 7 in
- Number of Pages
- 200 Pages
About this product
Product Information
Multi-messenger science has a long history in solar astronomy, as direct measures of "in-situ" particles emanating from the Sun, like the solar wind, have long been used alongside remote observations to shape our understanding of the heliosphere. Still, the recent advent of several major observational facilities, such as Parker Solar Probe, Solar Orbiter, and the Inouye Solar Telescope, among many others, is now heralding an exciting new era of scientific opportunities within multi-messenger solar physics. This volume collects the proceedings of IAU Symposium 372 held during the XXXIst IAU General Assembly in Busan, Republic of Korea. Its main goal is to highlight how these facilities can address many of the pressing questions facing contemporary solar physics, with a special emphasis on their coordinated operation and the resulting synergies. Graduate students and researchers in solar physics will benefit from the many new results presented within.
Product Identifiers
Publisher
Cambridge University Press
ISBN-10
1009352881
ISBN-13
9781009352888
eBay Product ID (ePID)
25061933603
Product Key Features
Book Title
Era of Multi-Messenger Solar Physics (Iau S372)
Number of Pages
200 Pages
Language
English
Publication Year
2023
Topic
Physics / Astrophysics, Astronomy
Illustrator
Yes
Genre
Science
Book Series
Proceedings of the International Astronomical Union Symposia and Colloquia Ser.
Format
Hardcover
Dimensions
Item Height
0.5 in
Item Length
10 in
Item Width
7 in
Additional Product Features
Dewey Edition
23
Dewey Decimal
523.7
Lc Classification Number
Qb521.6
Table of Content
Part I. New Solar Facilities and Multi-Mission Science; Solar Physics in the 2020s: DKIST, Parker Solar Probe and Solar Orbiter as a multi-messenger constellation V. Martinez Pillet et al; The Aditya-L1 mission of ISRO Durgesh Tripathi et al; Solar observations with ALMA: A new frontier T. S. Bastian; Modeling efforts for multi-mission science C. Sasso and A. P. Rouillard; Part II. Magnetic Fields - Generation, Activity, and Instabilities: Solar flare-CME association Ting Li; Origin of extreme solar eruptive activity from the active region NOAA 12673 and the largest flare of solar cycle 24 Bhuwan Joshi and Prabir K. Mitra; Solar cycles reconstructed over the last millennium: Do Waldmeier and Gnevysev-Ohl rules work? Markus Similä and Ilya Usoskin; Study of ionospheric behaviour during the intense geomagnetic storms in 24th solar cycle over different latitudes and longitudes Bhupendra Malvi, Sharad C. Tripathi and P. K. Purohit; Power spectra of the Sun's large-scale magnetic field during solar cycles 23 and 24 Yukun Luo, Jie Jiang and Ruihui Wang; Long-term evolution of magnetic field proxies as deduced from archival data Dipankar Banerjee et al; Observational signature of tilt quenching of bipolar magnetic regions in the Sun Bibhuti Kumar Jha, Bidya Binay Karak and Dipankar Banerjee; Photospheric magnetic field variation during solar flares and their implication for the generation of sunquakes S. Vargas Domínguez, W. Caicedo Tez and J. C. Buitrago Casas; A new mechanism for the butterfly diagram of the solar cycle Zebin Zhang, Jie Jiang and Haowei Zhang; Automatic detection of solar active regions from SOHO/MDI and SDO/HMI synoptic magnetograms Ruihui Wang, Jie Jiang and Yukun Luo; Automatic algorithm for tracking bipolar magnetic regions Anu B. Sreedevi and Bibhuti Kuma Jha; Part III. Solar Atmosphere and Solar Wind: How has the solar wind evolved to become what it is today? A. A. Vidotto; Spectroscopic Detection of Alfvénic MHD waves in the sunspot chromosphere Jongchul Chae; Self-consistent nanoflare heating in model active regions: MHD avalanches in curved coronal arcades J. Reid, J. Threlfall and A. W. Hood; Study of the impact of coronal rain on kink oscillations of coronal loops Arpit Kumar Shrivastav and Vaibhav Pant; Understanding Weak Impulsive Narrowband Quiet Sun Emissions (WINQSEs) Divya Oberoi et al; Spatio-temporal characterization of hot chromospheric fibrils Parker Lamb, Gianna Cauzzi and Kevin Reardon; Part IV: Machine Learning in Solar Physics: Application of deep learning to solar and space weather data Yong-Jae Moon et al.
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