NDLI: Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data

Please wait, while we are loading the content...

Interpretation of the light curves of “quiescent” X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system

The evolution of close binary systems with intermediate-mass black holes and ultra-luminous X-ray sources

Gravitational darkening coefficients of the stars in the semidetached binary V Puppis

Radial-velocity curves and theoretical spectral-line profiles of the components of low-mass close X-ray binary systems

Limits on the flux of ultrahigh-energy neutrinos from radio astronomical observations

Limits on the mass of dark matter in the Sun from a model for the modern Sun and its previous evolution

The nature of decimeter-wave microburst emission

Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data

Astronomy Reports : Volume 49, Issue 1, January 2005

Astronomy Reports : Volume 48

Astronomy Reports : Volume 47

Astronomy Reports : Volume 46

Astronomy Reports : Volume 45

Astronomy Reports : Volume 44

Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data

Content Provider	Springer Nature Link
Author	Chertok, I. M. Grechnev, V. V.
Copyright Year	2005
Abstract	Large-scale solar disturbances associated with powerful flares and coronal mass ejections (CMEs) during two passages of a grand system of three active regions in October–November 2003 are analyzed using data obtained with the SOHO/EIT EUV telescope. Dimmings (transient coronal holes) and, to a lesser extent, coronal waves (traveling emitting fronts) are studied using fixed-difference derotated images, in which a correction for the solar rotation is applied and a single heliogram preceding the event is subtracted from all subsequent heliograms. This method allows us to study difference heliograms in both the 195 Å line (with an interval of 12 min) and the various-temperature channels of 171, 195, 284, and 304 Å (with an interval of six hours). Our analysis shows, in particular, that the disturbances associated with CMEs demonstrated a global character and occupied almost the entire southern half of the disk in virtually all eruptive events during the two solar rotations. At the same time, the northern half of the disk, which had a large coronal hole, was only slightly disturbed. The dominant dimmings were observed on the disk as narrow, long features stretched mainly between three main, well-separated regions of the system and as long structures located along lines of solar latitude in the south polar sector. For repetitive events with intervals between them being not so long, the dominant dimmings demonstrated a clear homology in their forms and locations. During the very powerful event of October 28, one homologous global set of dimmings changed to another set. Many dimmings were observed to be identical or very similar in the three coronal channels and the transition-region line. It follows from the analysis that rapidly recovering global structures in the corona and transition region were involved in the eruption of running CMEs and the corresponding reconstruction of the large-scale magnetic fields.
Starting Page	155
Ending Page	166
Page Count	12
File Format	PDF
ISSN	10637729
Journal	Astronomy Reports
Volume Number	49
Issue Number	2
e-ISSN	15626881
Language	English
Publisher	Nauka/Interperiodica
Publisher Date	2005-01-01
Publisher Place	Moscow
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	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

Large-scale activity in major solar eruptive events of November 2004 according to SOHO data

Large-scale dimmings produced by solar coronal mass ejections according to SOHO/EIT data in four EUV lines

The Tanaka-Enome criterion and solar activity in October–November 2003 as observed by the Large Pulkovo Radio Telescope

Hybrid Solar Energetic Particle Events Observed on Board Soho

The extreme solar activity during october–november 2003

Soho-Eit image from 27 August 1997, 16:07 UT, showing a huge eruptive prominence inthe HE II resonance line at 304 Å.

Eruptive prominence and associated CME observed with SUMER, CDS and LASCO (SOHO)

The 1 October 2001 Eruptive Prominence: Observed and Modeled Structures

Multiple-Thread Model of a Prominence Observed by Sumer and eit on Soho

Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data

Similar Documents

Large-scale activity in major solar eruptive events of November 2004 according to SOHO data

Large-scale dimmings produced by solar coronal mass ejections according to SOHO/EIT data in four EUV lines

The Tanaka-Enome criterion and solar activity in October–November 2003 as observed by the Large Pulkovo Radio Telescope

Hybrid Solar Energetic Particle Events Observed on Board Soho

The extreme solar activity during october–november 2003

Soho-Eit image from 27 August 1997, 16:07 UT, showing a huge eruptive prominence inthe HE II resonance line at 304 Å.

Eruptive prominence and associated CME observed with SUMER, CDS and LASCO (SOHO)

The 1 October 2001 Eruptive Prominence: Observed and Modeled Structures

Multiple-Thread Model of a Prominence Observed by Sumer and eit on Soho

Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data