Published May 1985 | Version v1
Report

Evidence for submergencew of magnetic flux in a growing active region

Description

In NOAA Active Region 2372 (April 1980), 4 x 10 to the 20th power maxwell of magnetic flux concentrated within a 30'' circular area disappeared overnight. Vector magnetograms show that all components of the magnetic field weakened together. If the field had weakened through diffusion or fluid flow, 80% of the original flux would still have been detected by the magnetograph within a suitably enlarged area. In fact there was at least a threefold decrease in detected flux. Evidently, magnetic field was removed from the photosphere. Since the disappearing flux was located in a region of low magnetic shear and low activity, it is unlikely that the field dissipated through reconnection. The most likely possibility is that flux submerged. Observations suggest that even in the growth phase of active regions, submergence is a strong process comparable in magnitude to emergence

Additional details

Publishing Information

Imprint Title
Measurements of Solar Vector Magnetic Fields
Journal Page Range
vp.
Report number
NASA-CP--2374

Conference

Title
Measurements of Solar Vector Magnetic Fields.
Dates
15 May 1984.
Place
Huntsville, AL (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
18003705
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
MAGNETIC FIELDS; MAGNETIC FLUX; PHOTOSPHERE; SOLAR ACTIVITY; VECTORS
Descriptors DEC
ATMOSPHERES; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; TENSORS