NDLI: Present and Future Observing Trends in Atmospheric Magnetoseismology

Content Provider	Springer Nature Link
Author	Banerjee, D. Erdélyi, R. Oliver, R. O’Shea, E.
Copyright Year	2007
Abstract	With modern imaging and spectral instruments observing in the visible, EUV, X-ray, and radio wavelengths, the detection of oscillations in the solar outer atmosphere has become a routine event. These oscillations are considered to be the signatures of a wave phenomenon and are generally interpreted in terms of magnetohydrodynamic (MHD) waves. With multiwavelength observations from ground- and space-based instruments, it has been possible to detect waves in a number of different wavelengths simultaneously and, consequently, to study their propagation properties. Observed MHD waves propagating from the lower solar atmosphere into the higher regions of the magnetized corona have the potential to provide excellent insight into the physical processes at work at the coupling point between these different regions of the Sun. High-resolution wave observations combined with forward MHD modeling can give an unprecedented insight into the connectivity of the magnetized solar atmosphere, which further provides us with a realistic chance to reconstruct the structure of the magnetic field in the solar atmosphere. This type of solar exploration has been termed atmospheric magnetoseismology. In this review we will summarize some new trends in the observational study of waves and oscillations, discussing their origin and their propagation through the atmosphere. In particular, we will focus on waves and oscillations in open magnetic structures (e.g., solar plumes) and closed magnetic structures (e.g., loops and prominences), where there have been a number of observational highlights in the past few years. Furthermore, we will address observations of waves in filament fibrils allied with a better characterization of their propagating and damping properties, the detection of prominence oscillations in UV lines, and the renewed interest in large-amplitude, quickly attenuated, prominence oscillations, caused by flare or explosive phenomena.
Starting Page	3
Ending Page	29
Page Count	27
File Format	PDF
ISSN	00380938
Journal	Solar Physics
Volume Number	246
Issue Number	1
e-ISSN	1573093X
Language	English
Publisher	Springer Netherlands
Publisher Date	2007-10-16
Publisher Place	Dordrecht
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Coronal loops MHD waves MHD oscillations Astrophysics Extraterrestrial Physics, Space Sciences Astronomy
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

Sl.	Authority	Responsibilities	Communication Details
1	Ministry of Education (GoI), Department of Higher Education	Sanctioning Authority	https://www.education.gov.in/ict-initiatives
2	Indian Institute of Technology Kharagpur	Host Institute of the Project: The host institute of the project is responsible for providing infrastructure support and hosting the project	https://www.iitkgp.ac.in
3	National Digital Library of India Office, Indian Institute of Technology Kharagpur	The administrative and infrastructural headquarters of the project	Dr. B. Sutradhar bsutra@ndl.gov.in
4	Project PI / Joint PI	Principal Investigator and Joint Principal Investigators of the project	Dr. B. Sutradhar bsutra@ndl.gov.in Prof. Saswat Chakrabarti will be added soon
5	Website/Portal (Helpdesk)	Queries regarding NDLI and its services	support@ndl.gov.in
6	Contents and Copyright Issues	Queries related to content curation and copyright issues	content@ndl.gov.in
7	National Digital Library of India Club (NDLI Club)	Queries related to NDLI Club formation, support, user awareness program, seminar/symposium, collaboration, social media, promotion, and outreach	clubsupport@ndl.gov.in
8	Digital Preservation Centre (DPC)	Assistance with digitizing and archiving copyright-free printed books	dpc@ndl.gov.in
9	IDR Setup or Support	Queries related to establishment and support of Institutional Digital Repository (IDR) and IDR workshops	idr@ndl.gov.in

Coronal Periodmaps : Automated Detection of Wave and Oscillatory Phenomena in Coronal Imaging Data

Propagation and Damping of a Localized Impulsive Longitudinal Perturbation in Coronal Loops

Propagating MHD Waves in Coronal Holes

MHD waves in coronal loops with a shell

Non-reflective Propagation of Kink Waves in Coronal Magnetic Loops

Short Quasi-Periodic MHD Waves in Coronal Structures

Periods and Damping Rates of Fast Sausage Oscillations in Multishelled Coronal Loops

MHD Waves and Heating in Coronal Holes

Motion Magnification in Coronal Seismology

Present and Future Observing Trends in Atmospheric Magnetoseismology

Similar Documents

Coronal Periodmaps : Automated Detection of Wave and Oscillatory Phenomena in Coronal Imaging Data

Propagation and Damping of a Localized Impulsive Longitudinal Perturbation in Coronal Loops

Propagating MHD Waves in Coronal Holes

MHD waves in coronal loops with a shell

Non-reflective Propagation of Kink Waves in Coronal Magnetic Loops

Short Quasi-Periodic MHD Waves in Coronal Structures

Periods and Damping Rates of Fast Sausage Oscillations in Multishelled Coronal Loops

MHD Waves and Heating in Coronal Holes

Motion Magnification in Coronal Seismology

Present and Future Observing Trends in Atmospheric Magnetoseismology