NDLI: A Flare-Triggered Heating of a Quiescent Filament

Content Provider	Springer Nature Link
Author	Ji, H.S. Wang, H. Spirock, T.J. Qiu, J. Yang, G. Goode, P.R.
Copyright Year	2002
Abstract	Using data obtained with the 20-cm Hα full-disk telescope at Big Bear Solar Observatory and Fe xii 195 Å EIT on SOHO, we analyze a sudden disappearance event of a quiescent filament in detail. The filament was located along the common boundary of the active regions NOAA 9672 (S19 E13) and NOAA 9673 (N03 E18). The filament disappeared during a time interval between 17:59 UT and 19:47 UT on 22 October 2001 immediately after the onset of a major flare, which occurred in the active region NOAA 9672. At about 23:23 UT of the same day, the filament began to reappear in Hα and, after about 15 hours, the filament recovered to its steady state with its size being slightly smaller than that before its disappearance. This filament disappearance event belongs to the thermal type of sudden filament disappearances, which is caused by an input of additional heat. The heating mechanism that leads to sudden thermal disappearances of quiescent filaments is still not well understood. This simple event, due to the explicit cause and effect relationship between the flare and the disappearance of the filament, shows us that the flare triggered some kind of heating mechanism which continued several hours. The heat may come from the flare via heat conduction from its ribbon or from the excitation of dissipating Alfvén waves. However, from the data analysis, we conclude that the flare triggered an in-situ heating, which is likely caused by magnetic reconnection.
Starting Page	221
Ending Page	229
Page Count	9
File Format	PDF
ISSN	00380938
Journal	Solar Physics
Volume Number	211
Issue Number	1-2
e-ISSN	1573093X
Language	English
Publisher	Kluwer Academic Publishers
Publisher Date	2002-01-01
Publisher Place	Dordrecht
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Astrophysics
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

Magnetic Causes of the Eruption of a Quiescent Filament

Rapid Formation and Disappearance of a Filament Barb

Analysis Of The Disappearing Filament And Flare Of 7 May 1992

Magnetic source regions of coronal mass ejections

An M1.5 Flare Triggered by a Multireconnection Process

Including Flare Sympathy in a Model for Solar Flare Statistics

Flare loop geometry

Emission lines in the spectrum of the red-dwarf flare star EV Lac: Modeling of the quiescent chromosphere

Shrinking and Cooling of Flare Loops in a Two-Ribbon Flare

A Flare-Triggered Heating of a Quiescent Filament

Similar Documents

Magnetic Causes of the Eruption of a Quiescent Filament

Rapid Formation and Disappearance of a Filament Barb

Analysis Of The Disappearing Filament And Flare Of 7 May 1992

Magnetic source regions of coronal mass ejections

An M1.5 Flare Triggered by a Multireconnection Process

Including Flare Sympathy in a Model for Solar Flare Statistics

Flare loop geometry

Emission lines in the spectrum of the red-dwarf flare star EV Lac: Modeling of the quiescent chromosphere

Shrinking and Cooling of Flare Loops in a Two-Ribbon Flare

A Flare-Triggered Heating of a Quiescent Filament