Evidence for submergencew of magnetic flux in a growing active region
Creators
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